FAIR ndash Facility for Antiproton and Ion Research

Austria China Finnland France Germany Greece India Italy Poland Slovenia Spain Sweden Romania Russia UK

Observers

Cosmic matter in the Lab FAiR = The International

Facility for Antiproton and Ion Research Horst Stoumlcker GSI amp FIAS

Quick Tim etrade and aTIFF ( Uncom pr es sed) decom pr esso r

a re n eeded to see th is p ic tur e

100 m

UNILACSIS 18

SIS 100300

HESR

SuperFRS

NESR

CRRESR

ESR

bull Construction in three phases until 2016bull Total cost 12 Beurobull Scientific users 2500 shy 3000 per year

Construction Period Cost Users

bull 65 Federal Government of Germanybull 10 State of Hessenbull 25 Partner Countries FAIR GmbH with International Shareholders

Financing

GSI today Future facilitybull Beam intensities by factors of 100 shy 10000bull Beam energies by a factor 20bull Production of antimatter beamsbull Factor 10000 in beam brilliance via coolingbull Efficient parallel operation of programs

Gain Factors

The Big Challenge

Largest fundamental

science research

project in Europe for

the next decade

FAIR Research Topics and Intershylinks

Jupiter

Sun Surface

Magnetic Fusion

solid statedensity

Tem

pera

ture

[eV

]

Density [cmshy3]

LaserHeating

PHELIX

Ideal plasmas

Sun Core

SIS 18

Ion BeamHeating

SIS 100

InertialCofinement

Fusion

Plasma physics with intense ion bunches andpetawatt Laser pulses

Matter at high energy densities

Strongly coupled

plasmas

Physics of Fast Ignition (another way to clean energy production)

Equation of state of planetary and stellar matter

Production of exotic nuclei in the laboratory

1 GeVu U 3x1011s 1GeVu U + H About 1000 nuclear fragments

identified

AZshyresolution ~10shy3

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

100 m

UNILACSIS 18

SIS 100300

HESR

SuperFRS

NESR

CRRESR

ESR

bull Construction in three phases until 2016bull Total cost 12 Beurobull Scientific users 2500 shy 3000 per year

Construction Period Cost Users

bull 65 Federal Government of Germanybull 10 State of Hessenbull 25 Partner Countries FAIR GmbH with International Shareholders

Financing

GSI today Future facilitybull Beam intensities by factors of 100 shy 10000bull Beam energies by a factor 20bull Production of antimatter beamsbull Factor 10000 in beam brilliance via coolingbull Efficient parallel operation of programs

Gain Factors

The Big Challenge

Largest fundamental

science research

project in Europe for

the next decade

FAIR Research Topics and Intershylinks

Jupiter

Sun Surface

Magnetic Fusion

solid statedensity

Tem

pera

ture

[eV

]

Density [cmshy3]

LaserHeating

PHELIX

Ideal plasmas

Sun Core

SIS 18

Ion BeamHeating

SIS 100

InertialCofinement

Fusion

Plasma physics with intense ion bunches andpetawatt Laser pulses

Matter at high energy densities

Strongly coupled

plasmas

Physics of Fast Ignition (another way to clean energy production)

Equation of state of planetary and stellar matter

Production of exotic nuclei in the laboratory

1 GeVu U 3x1011s 1GeVu U + H About 1000 nuclear fragments

identified

AZshyresolution ~10shy3

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

FAIR Research Topics and Intershylinks

Jupiter

Sun Surface

Magnetic Fusion

solid statedensity

Tem

pera

ture

[eV

]

Density [cmshy3]

LaserHeating

PHELIX

Ideal plasmas

Sun Core

SIS 18

Ion BeamHeating

SIS 100

InertialCofinement

Fusion

Plasma physics with intense ion bunches andpetawatt Laser pulses

Matter at high energy densities

Strongly coupled

plasmas

Physics of Fast Ignition (another way to clean energy production)

Equation of state of planetary and stellar matter

Production of exotic nuclei in the laboratory

1 GeVu U 3x1011s 1GeVu U + H About 1000 nuclear fragments

identified

AZshyresolution ~10shy3

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Jupiter

Sun Surface

Magnetic Fusion

solid statedensity

Tem

pera

ture

[eV

]

Density [cmshy3]

LaserHeating

PHELIX

Ideal plasmas

Sun Core

SIS 18

Ion BeamHeating

SIS 100

InertialCofinement

Fusion

Plasma physics with intense ion bunches andpetawatt Laser pulses

Matter at high energy densities

Strongly coupled

plasmas

Physics of Fast Ignition (another way to clean energy production)

Equation of state of planetary and stellar matter

Production of exotic nuclei in the laboratory

1 GeVu U 3x1011s 1GeVu U + H About 1000 nuclear fragments

identified

AZshyresolution ~10shy3

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Production of exotic nuclei in the laboratory

1 GeVu U 3x1011s 1GeVu U + H About 1000 nuclear fragments

identified

AZshyresolution ~10shy3

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Comparison of FRS with SupershyFRS intensity gain

FRS

SupershyFRS

FAIR 2s

FAIR 65h

FAIR 8s

FAIR109s

FAIR108s

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Important beam parametersshy All elements from H to Ushy Intensity ~ 3x1011 ionssec

shy Beam energies up to 15 GeVushy Fast and slow extraction

NUSTARFAIR

SIS

MainshySeparatorPreshySeparator

LowshyEnergy Cave

CR complex

NESR

Energy Buncher

HighshyEnergyCave

SupershyFRS eAshyCollider

gas target

Production Target

Beams p shy U1500 MeVu10 ions s

12

20 Tm

from SIS100

from SIS18

Superconducting fragment separator+ Highshyenergy branch with reactiondetector+ Storage ring complex (CR RESR NESR eA)+ Lowshyenergy branch with energy focusing

and post shy acceleration

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Mass spectrometry New Experimental Storage Ring ILIMA

Mass determination of more than 1100 nuclei

Mass accuracy SMS ~ 30 keVc2

IMS ~ 100 keVc2

Results ~ 350 new mass values ~ 300 improved mass values

Singleshyion detectionm∆m=2106

SMS

IMSrpshyprocess path rshyprocess path

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Experiments with slowedshydown stopped and postshyaccelerated (single) ions at the lowshyenergy branch

MATS

LASPEC

DESPEC

Degraderstation

Stop cellEnergy focusing and degrader station

HISPEC

NEUTRON DETECTOR

GE γshyARRAY

RADIOACTIVEBEAM

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Reaction experiments with relativistic radioactive beams at SupershyFRS (R3B)

Neutron detectors

Highshyresolution momentum determination

of heavy fragments

Protons and heavy fragments modest momentum resolution

Target trackercalorimeter

Exotic nuclei

superconducting dipole magnet with high momentumshy amp High angular acceptance

Exclusive reaction studies via kinematically complete measurements

Determination of energy and momentum of all reaction products reaction microscope

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Pygmyshydipole resonance neutron skins and equation of state of matter

GSI FAIRMeasuring time 10 d 100 sEnergy resolution 1 MeV 01 MeV

Coulomb excitation Photoabsorption

P Adrich et al PRL 95 (2005) 132501

E ρNminusZ

A =E 0ρ a4p0

ρ0

2

ρminusρ 0 sdot NminusZA

2

Oscillation of neutronskin versus nuclear core

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

HypHI Project at GSIFAIR

HypHI project started design studyPlanned Experimentsbull 3

ΛH 4ΛH and 5

ΛHebull protonshyrich hypernucleibull neutronshy rich hypernuclei at

R3BNuSTARFAIRHypernuclear separatorbull Hypernuclear magnetic momentsbull Hypernuclear dripshylines

2008

2010

2012

~20142010

Phase 0

Phase 1

Phase 3

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

AAntronic et al

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

calculations based on

Yields of light nuclei at AGS enery and thermal model calculations

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Production yields of exotic hypernuclei

SIS300 energy

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

FAIR QCDshyPhysics Program with Antiprotons

Jψ spectroscopy confinement inshy medium effects

hidden and open charm in nuclei

glueballs (ggg) hybrids (ccg)

strange and charmed (antishy)

baryons in

nuclear field

inverted deeply virtual Compton scattering

CPshyviolation (DΛ shy sector)

fundamental symmetries p in traps

spin structure of the proton polarized antiprotons in PAX

HESR ConsortiumJuumllich Uppsala Stockholm GSI

FLAIR

PANDA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Flair FAIR Research Topics with

LowshyEnergy Antiprotons fundamental interactions shy CPT (antihydrogen HFS magnetic

moment)

shy gravitation of antimatter

bull atomic collision studies

shy ionization

shy energy loss

shy mattershyantimatter collisions

bull antishy protonic atoms

shy formation

shy strong nuclear interaction

and surface effects

shy trapping antishy protons in nuclei

short lived bound states

Later perhaps Low Energy Antishy He

ρ = 5minus10 x ρ0

IMishustin L Satarov HSt W Greiner

Cold Nuclear Compression by

Vector Attraction of

pshybars in medium

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Compressed baryonic matter exps start at SIS100

Rigidity Bρ = 100 TmAu beam 10 AGeVNi beam 14 AGeVp beam 30 GeV

HADES electrons hadronsCBM light (magnet Silicon tracker TOF) p K π Λ Ξ Ω flow fluctuations up to Au+Au

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Dipolmagnet

The Compressed Baryonic Matter Experiment

Ring ImagingCherenkovDetector

Transition Radiation Detectors

ResistivePlate Chambers(TOF)

ElectroshymagneticCalorimeter

SiliconTrackingStations

Tracking Detector

Muondetection System

Projectile SpectatorDetector(Calorimeter)

VertexDetector

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Compressed Baryonic Matter CBM Physics Topics

Probing the high density EoS collapse of coll flow of protons

QshyH phase boundaryhigh ρB multishystrange + charmed prod

QCD critical point EshybyshyE fluctuations Energydep Hadron Yield

Chiral symmetry rest at high ρB open charm dilepton prod

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Big Bangshy amp Neutron Starshymatter CBM FAIRQCD phases at High Density ρB

SiS30045 GeV

SiS10010 GeV

Bravina Zabrodin

Tenfold Compression Crossing that 1 Order Transition

Nonequil

Equilibr

UrQMD

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Ideal Hadron Gas differs strongly from

Chiral SU(3) hadron model with mushycritSA=7shy10

Stefan Schramm D Zschiesche G Zeeb

BiS

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

30AGeV 3Dim 3shyFluid First Order Baeuchle Bleicher HSt

30AGeVmpg

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

CBM rich physics program near the critical point

bull bull yields and particle ratiosyields and particle ratiosrarr T and microB

bull bull identified particle elliptic flow videntified particle elliptic flow v1212

rarr collapse of proton flow

bullbull KKππ p pππ langlangppTTrangrang fluctuations fluctuationsrarr critical point signal

bull bull scale dependence of fluctuationsscale dependence of fluctuationsrarr source of the signal

bullbull vv22 fluctuations fluctuationsrarr promising new frontier

highest luminosity=gt rare probes

bull bull rare particle production at thresholdrare particle production at thresholdrarr EOS

bull bull flow of charm melting of quarkoniaflow of charm melting of quarkonia (Jψ ψ D0 Dplusmn Λc)

rarr deconfinement bull bull in medium modific of vector mesons in medium modific of vector mesons (ρωφ rarre+eshy(μ+μshy) D)

rarr chiral symmetry restoration

bullbull Strange matter droplets

low luminosity=gt abundant probes

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

collision evolution

particle detectors

collision overlap zone

QGP phasequark and gluon

degrees of freedom

τ ~ 10 fmc

hadronization

kineticfreezeshyout

lumpy initial energy density

τ0~1 fmcτ ~ 0 fmc

distributions and

correlations of produced

particles

quantum fluctuations

Heavyshyion Collisions Rapid Expansion

expansion and cooling

The Universe Slow Expansion

credit NASA

Analogy to the early universe evolution of critical fluctuations

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Production yields of possible exotic kaon clusters

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Collapse of Shock at Phase Transition in EoS

D RischkeNPA 610 c88 (lsquo96)

Later dubbed ldquosoftest pointrdquo of EoS

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

bull Au+Au 8GeV b=3fm Triple differential Cross section

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Proton ldquoAntishyFlowrdquo observed in Pb+Pb40AGeV NA49 A WetzlerPreliminary

ldquoAntishyFlowrdquo discovered =gt 1 Order Phase Transition

v1 le 0RED Central Collisions

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Excitation Function Elliptic flow

Wetzler NA49 data Collapse of proton flow at 40AGeV

NA49 PRC C68 034903 (2003)

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Other measures to look for

bull Disappearance of partonic signatures from RHICndash Disappearance of quark scaling in particle identified

high momentum elliptic flow ndash Disappearance of ideal hydro description in low

momentum elliptic flow ndash Disappearance of nuclear suppression at high

momentum

bull To probe the system shy resonancesndash Hadronic lifetime measurements through resonance

rescattering and regenerationndash Chiral symmetry restoration through chiral resonance

partners (eg ρ and a1)

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

100 m

UNILACSIS 18

SIS 100300

HESRFZ Juumllich

SuperFRS

NESR

CRRESR

GSI

FAIR

ESR

FLAIR

RareshyIsotopeProduction Target

AntiprotonProduction Target

CBM

PPamp APHadron Structure QCD amp Medium Cooled antiprotons lt 15 GeV 500 users Nuclear Astrophys NUSTAR

RI beamshy fragmentation 600 usersWarm Dense Plasmas Bunchshycompression amp Petawattshy Laser 250 users

QCDshyPhase Diagram CBM HI beams 2 to 45 AGeV 400 users

Materials Science Spaceshy and Radiation Biology(Ionshy amp antiprotonshy beams 350 users

Fundamental SymmetriesUltrashyHigh EM Fields SPARC FLAIRAntiprotons HishyZ ions 250 users

Accelerator Physics amp Gym Eight Rings amp two Linacs

FAIR Research Highlights

Panda

PshyLinac

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Highest Intensity upgrade

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA

Synthesis and study of the heaviest elements

NUSTAR UNILACSynthesis of the elements 107shy112Chemistry of the elements 107 108 (112)

IUPACElement 110 is named ldquoDarmstadtiumrdquo Chemical symbol is Ds

Chemistry

Atomic structureNuclear structure

Synthesis

SHE

270Ds

266Hs

SHIP and TASCA