The Facility for Antiprotonand Ion Research in Europe

Günther Rosner MESON2012, Krakow, 4/6/12 1

FAIR @ Darmstadt

Günther Rosner MESON2012, Krakow, 4/6/12 2

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Facility for Antiproton & Ion Research

Günther Rosner MESON2012, Krakow, 4/6/12

Dense Bulk Plasmas (Ion-beam bunch compression& petawatt-laser)

Materials Science & Radiation Biology (Ion & antiproton beams) Accelerator Physics

UNILAC

SIS18 SIS100/300p-Linac

HESR

CR &RESR

NESR

Cryring

Rare-IsotopeProduction Target

Anti-ProtonProduction Target

100 m

QCD-Phase Diagram(HI beams 2 to 45 GeV/u)

Hadron Physics (Stored and cooled14 GeV/c anti-protons)

Nuclear Structure & Astrophysics(Rare-isotope beams)

Fundamental Symmetries& Ultra-High EM Fields(Antiprotons & highly stripped ions)

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Fast accelerationHigh gradient, variable frequency

Ferrite & MA loaded cavities

Compact & cost effective acceleratorsFast cycling superconducting magnets

dB/dt ~ 4T/s

Precision beamsElectron & stochastic cooling

XHV @ high beam intensitiesExtremely high vacuum ~10-13 mbar

Accelerator Challenges

Günther Rosner MESON2012, Krakow, 4/6/12

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FAIR Experiments

Günther Rosner MESON2012, Krakow, 4/6/12

CBM

PANDANuSTAR

Super-FRS

APPA

Brain Twister INo free quarks observed. They are confined in pairs or triplets in strongly interacting particles (hadrons).

Günther Rosner MESON2012, Krakow, 4/6/12 6

u d

u

Proton (p)938 MeV/c2

u d

d

Neutron (n)939 MeV/c2

ud

π- 140 MeV/c2

Baryons Mesons

Narrow Hadronic States

Günther Rosner MESON2012, Krakow, 4/6/12 7

PANDA @ FAIR

Brain Twister IINormal (heavy) matter consists of pointlike, nearly massless quarks.

99% of the mass of the visible universe is, strictly speaking, energy!

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Anti-Proton Annihilation @ DA

Günther Rosner MESON2012, Krakow, 4/6/12

PANDA

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Gluonic excitations

Günther Rosner MESON2012, Krakow, 4/6/12

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Search for Heavy Glueballs• “Charmed” glueballs

– flavour blind decays• charmed final states!

– only a few charmed mesons around 3 - 4 MeV/c2

• less mixing!

• Exotic glueballs (oddballs), no mixing!– m(2+-) = 4140(50)(200) MeV

– m(0+-) = 4740(70)(230) MeV– decay modes , , J/, J/

– Narrow widths predicted

Günther Rosner MESON2012, Krakow, 4/6/12

Morningstar & Peardon, PRD60(1999)34509Morningstar & Peardon, PRD56(1997)4043

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PANDA & CBM: Hadrons in Nuclei

• Partial restoration of chiral symmetry in nuclear matter Light current quarks sensitive to

quark condensate

• Charmonium states Sensitive to gluon condensate Significant mass shifts expected for

c, ’, (3770): 40, 100, 140 MeV/c2

resp.

• D mesons: the QCD analogue of an H-atom Chiral symmetry to be studied on a

single light quark Theoretical calculations disagree in

size and sign of mass shift (50 MeV/c2 attractive vs. 160 MeV/c2 repulsive)Günther Rosner

Vacuum Nuclearmedium

p

K

25 MeV

100 MeV

K+

K-

p-

p+

Hayaski, PLB 487 (2000) 96Morath, Lee, Weise, priv. Comm.

D-50 MeV

D

D+

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Compressed Baryonic Matter

Günther Rosner

SIS100/300

CBM @ FAIR

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High Baryon Density @ CBM

Günther Rosner

Probes of Dense Phase

No data so far FAIR Range

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NuSTAR

Günther Rosner MESON2012, Krakow, 4/6/12

NuSTAR

Super-FRS

Secondary Beams: Broad range of radioactive ion beams ≤ 2 GeV/u RI- Intensities up to 10 000 over present

Primary HI Beams:• 40Ar18+ 2x1012/s @ 1 – 2 GeV/u• 238U28+: 5x1011/s @ 1 – 2 GeV/u

• 40Ar18+ 2x1010/s @ 1 – 45 GeV/u• 238U92+: 1x1010/s @ 1 – 35 GeV/u100 x 1000 times current intensity

GSI FRS FAIR Super-FRS

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1000 7500

Super-FRS

FRS

NuSTAR

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APPA: Parity-Violation

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PS

PNWFS

EE

QG

522/

Mixing coefficient for states with opposite parities:

Energy levels of He-like uranium

2E1 (PNC)

To “compete” with spontaneous decay channels one needs to induce a two-

photon PNC transition by polarised light with intensity 1020 W/cm2

g NN

ee

Zee

NN

Select case with small splitting!

Large EM Fields

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Sub-fs pulses

Lasers

(adapted from Mourou, Tajima, Bulanov, RMP 78, 2006)

Heavy ions

Large EM fields, zs pulses

Equivalent toI ≥ 1028 W/cm2

Plasmas

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Particles / cm-3

Tem

per

atu

re [

eV]

Jupiter

LaserHeating

Sun Surface

Magnetic Fusion

solid statedensity

PHELIX

Sun Core

Inertial Fusion Energy

XFEL

SIS 18

Ion BeamHeating

SIS 100

Strongly coupled

plasmasIdeal plasmas

FLASH

ESA @ GSI & FAIR

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GCR Charge Contributions

Charge Number

0 5 10 15 20 25 30

% C

ontr

ibut

ion

0.001

0.01

0.1

1

10

100

FluenceDoseDose Eq.

Free Space

Durante & Cucinotta, Nature Rev. Cancer (2008)

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Staging

Günther Rosner

Start Version Phase A(SIS100)

Phase B(SIS300)

Modularised Start Version

Module 0 Module 1 Module 2 Module 3 Module 4 Module 5

SIS100 Exp. halls CBM & APPA

Super-FRS NuSTAR

Antiproton FacilityPANDA & options NuSTAR

LEB, NESR, FLAIR

NuSTAR & APPA

RESRPANDA,

NuSTAR & APPA

2017/18

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Modularised Start Version

Günther Rosner

APPA

CBM/HADES

NuSTAR

PANDAExperiments

M1: APPAM1: CBM/HADESM2: NuSTARM3: PANDA

M0

M1

M2M3

M3

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Costs MSV

Günther Rosner

Accelerators and personnel (including Super-FRS) 502 M€

Civil construction (excluding site related costs) 400 M€

FAIR contribution to experimental end stations * 78 M€

FAIR GmbH personnel & running until 2018 (>8 years) 47 M€

Grand Total MSV, Modules 0 - 3 1027 M€

in 2005 € (inflation escalation until 2018: ca. +50%)

* Total experimental end stations (excluding Super-FRS): ca. 210 M€ (2005) = 315 M€ (2018)

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Funding Modules 0-3Contracting Party Contribution

(in 2005 M€)

Finland 5.00

France 27.00

Germany 705.00

India 36.00

Poland 23.74

Romania 11.87

Russia 178.05

Slovenia 12.00

Sweden 10.00

Total 1.008,66

Günther Rosner

• All numbers in 2005 €(escalation until 2018 ca. +50%)

• Spain expected to join soon (with 11.87 M€)

• China and the UK are potential Associate FAIR Members and will contribute to the experiments (6.6 M€)

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Timelines

Günther Rosner

20122011 2013 201620152014

6

Submission building permits

Site preparation

Civil construction contracts

Building of accelerator & detector components

Completion of civil construction work

Installation & commissioning of accelerators and detectors

Data taking

7 108

2017 2018 2019

12

6

7

8

9

11

12

10

119

Civil Construction

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Start Clearing 6/12/2011

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Test Drilling 31/8/2011

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Thank you very much

Günther Rosner MESON2012, Krakow, 4/6/12 31