greeings from m. spiro - École polytechnique

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- Peter Higgs - Charles H. Townes Chris Barty Gerard Mourou Toshiki Tajima150th Anniversary of Politecnico di Milano IZEST-LLNL MOUROU IZEST-LLNL July 17-18 2012 3rd IZEST SYMOSIUM 29/01/2014

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Page 1: Greeings from M. Spiro - École Polytechnique

- Peter Higgs

- Charles H. Townes Chris Barty

Gerard Mourou

Toshiki Tajima150th Anniversary of

Politecnico di Milano

IZEST-LLNL MOUROU

IZEST-LLNL July 17-18 2012

3rd IZEST SYMOSIUM

29/01/2014

Page 2: Greeings from M. Spiro - École Polytechnique

IZEST: Laser Transition from Atomic to Subatomic Physics

from Particle to Photon

IZEST-LLNL MOUROU 29/01/2014

Page 3: Greeings from M. Spiro - École Polytechnique

Contents IZEST Two Prong Effort

• Utrahigh Peak Power: Reaching the EW-ZW Regime – Damageless Optics: Gratings, focusing optics

– Applications: Particle Physics

• Ultra High Peak Power and Average Power the CAN (Coherent Amplification concept) MW average power with >30%, Concept and Validation – Scientific Applications (collider, Protons, Neutron, ..,

Sources)

– Societal Applications (Transmutation, Free electron laser, lithography,.Proton Therapy, .)

29/01/2014 IZEST-LLNL MOUROU

Page 4: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

Vacuum Polarization IZEST C3

Extreme Light Road Map

MeV

eV

MeV

GeV

TeV

J

MJ

kJ

mJ

Ep=mpc2

Ee=m0c2

LMJ/NIF, 2MJ, 3B€

ELI, kJ .3 B€ XCELS

29/01/2014

Page 5: Greeings from M. Spiro - École Polytechnique

IZEST a New Paradigm in Laser and High

Energy Physics

• IZEST is based on large scale facilities

developped over the past 20 years for laser

fusion

• It is also based on the large laser fusion, High

Field Science, Particle Physics communities.

• IZEST benefits from the huge body of works

developped in Laser Plasma Physics over 50

years.

29/01/2014 IZEST-LLNL MOUROU

Page 6: Greeings from M. Spiro - École Polytechnique

The Pulse Duration-Intensity Conjecture

G.A. Mourou and T. Tajima, “More intense Shorter Pulse”, SCIENCE VOL 331 , 7 , p 41JANUARY 2011

IZEST-LLNL MOUROU 29/01/2014

Page 7: Greeings from M. Spiro - École Polytechnique

IZEST Benefits from the largest Pump Lasers Up to the MJ

PETAL-LMJ NIF LLNL 29/01/2014 IZEST-LLNL MOUROU

Page 8: Greeings from M. Spiro - École Polytechnique

IZEST Particle Physics Ascent

1GeV

100GeV-PETAL 2015 LFEX

1TeV-PETAL, LFEX, NIF, XCELS

10GeV-GSI 2013

29/01/2014 IZEST-LLNL MOUROU

Page 9: Greeings from M. Spiro - École Polytechnique

29/01/2014 IZEST-LLNL MOUROU

Page 10: Greeings from M. Spiro - École Polytechnique

New Paradigm PeV

TeV Standard Model Quarks Leptons

Extra dimension Dark matter Supersymmetry

Leptogenesis SUSY breaking

Atsuto Suzuki: KEK Director General,

ICFA Chair

IZEST’s Mission: Responding to Suzuki’s Challenge

IZEST-LLNL MOUROU 29/01/2014

Page 11: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU T. Tajima J. Dawson

Laser Wake Field Acceleration Source of high energy electrons and photons

29/01/2014

Page 12: Greeings from M. Spiro - École Polytechnique

PeV Accelerator

1km laser Plasma accelerator with LIL or LMJ

(Vision 2011)

With conventional Technology The accelerator would Girdle the Earth: Fermi’s vision (1954)

IZEST-LLNL MOUROU 29/01/2014

Page 13: Greeings from M. Spiro - École Polytechnique

130GeV Experiment

on the PETAL laser

IZEST-LLNL MOUROU 29/01/2014

Page 14: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

From N. Narozhny

nperp -1

npar -1º

4

7

29/01/2014

Page 15: Greeings from M. Spiro - École Polytechnique

Dark Matter Quantum Vacuum

• Weekly interacting particles like axion or axion-like ,

U(1) gauge bosons with low mass in the subelectron volt.

• Non linear effect in large electromagnetic fields, light shinning

Through walls.

IZEST-LLNL MOUROU 29/01/2014

Page 16: Greeings from M. Spiro - École Polytechnique

Laser-Based High Energy Physics Low Luminosity Paradigm

• Nonlinear Effects in Vacuum • Dark Energy and Dark Matter • Physics beyond TeV with the Non-Collider

Paradigm • TeV-PeV Astrophysics • Lorentz Invariance (gamma rays, neutrino, ...... ) • as /zs Ultrafast Science • Radiation near the Schwinger field • Precision particle/Radiation Metrology • Exawatt and Zettawatt Laser Technology

IZEST-LLNL MOUROU 29/01/2014

Page 17: Greeings from M. Spiro - École Polytechnique

IZEST Technology

29/01/2014 IZEST-LLNL MOUROU

Page 18: Greeings from M. Spiro - École Polytechnique

To Reach its Ambitious Goal, IZEST Triggered a

Revolution in

Laser Technology

• Highest Peak Power demands higher damage components: IZEST

introduced damage less optics based on Plasma optics for diffraction gratings and mirrors:

J/cm2 to 10kJ/cm2

• IZEST works on Laser Acceleration at 100GeV single stage to reach TeV multistage:

GeV-PeV level

• Scientific and Societal Applications will require much higher and efficient average power. We invented a new laser Architecture CAN Coherent Amplification Network:

Moving from Watt to Megawatt, with High Efficiency

29/01/2014 IZEST-LLNL MOUROU

Page 19: Greeings from M. Spiro - École Polytechnique

Amplification: Backward Raman or Brillouin Amplification

Backwards Raman Amplification(BRA) V. M. Malkin, G. Shvets, and N. J. Fisch, “Phys. Rev. Lett. 82, 4448(1999).

LCell =cTpump

2

IZEST-LLNL MOUROU

S. Suckewer et al. Nature Phys. Oct. 2007

Electron Plasma Wave or Ion-acoustic Wave in the Strong-Coupled Regime

29/01/2014

Page 20: Greeings from M. Spiro - École Polytechnique

Cascaded Compression Conversion C3

G. A. Mouroua,N. J. Fischb,*, V.M Malkinb, Z. Torokerb, E.A. Khazanovc, A.M. Sergeevc, T. Tajimad, B. Le Garrec, Exawatt Zettawatt Generation and Applications, Optics Communications 285 (2011) 720–724

IZEST-LLNL MOUROU 29/01/2014

Page 21: Greeings from M. Spiro - École Polytechnique

Focusing Ultrahigh Intensity Beam

Plasma Optics 5-10 kJ/cm2 Damage Threshold Optics

100kJ~ 3cm diameter

IZEST-LLNL MOUROU 29/01/2014

Page 22: Greeings from M. Spiro - École Polytechnique

Towards the MW Average Power The ICAN project

29/01/2014 IZEST-LLNL MOUROU

Page 23: Greeings from M. Spiro - École Polytechnique

ICAN European Commission Project

Page 24: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

TeV Collider

29/01/2014

Page 25: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

Laser Wake field Acceleration

GeV, 100 pC ~ 100mW.

40W

29/01/2014

Page 26: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

.4TGV

1TGV=10MW

29/01/2014

Page 27: Greeings from M. Spiro - École Polytechnique

HIGH PEAK POWER LASER AVERAGE POWER: FROM THE LIGHT BULB(W) TO TGV(MW)

50W

10MW

29/01/2014 IZEST-LLNL MOUROU

Page 28: Greeings from M. Spiro - École Polytechnique

Nature Photonics April, 2013

29/01/2014 IZEST-LLNL MOUROU

Page 29: Greeings from M. Spiro - École Polytechnique

ICAN (European Project) CAN Coherent Amplification Network

G. Mourou, W. Brocklesby, J. Limpert, T. Tajima, Nature Photonics April 2013 « The future of Acceletaor is Fiber »

IZEST-LLNL MOUROU 29/01/2014

Page 30: Greeings from M. Spiro - École Polytechnique

Conventional Accelerator Technology

Page 31: Greeings from M. Spiro - École Polytechnique

Radiation Pressure Acceleration Source of Relativistic Proton

• Scientific Applications

Electron-positron Collider

• Proton Collider (Tevatron, LHC)

• Neutron source (ESS)

• Neutrino Source(SNS, ESS)

• Radioactive Ion Beam (FRIB, Eurisol)

• Muon collider

• Free Electron laser at 10kHz

• Higgs Factory

• Societal Applcations • Gamma ray source Fukushima

• Accelerator Driven System (Ch-ADS,MYRRHA)

• Nuclear Pharmacology

• Proton Therapy

• And much more…..

Page 32: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU 29/01/2014

Page 33: Greeings from M. Spiro - École Polytechnique

To respond to its ambitious challenge ICAN requires

A World Effort

WE-CAN World Effort Coherent Amplification Net Work

G. MOUROU, W. LEEMANS FOR HORIZON 2020

29/01/2014 IZEST-LLNL MOUROU

Page 34: Greeings from M. Spiro - École Polytechnique

Laser-Based High Energy and Fundamental Physics: Exawatt to Zettawatt

IZEST-LLNL MOUROU

2015 2010 2020 2025 2030

IZEST XCELS LMJ, NIF ELI

29/01/2014

Page 35: Greeings from M. Spiro - École Polytechnique

Organization Chart - Provisional

(*)Pending

Director, G. MourouDeputy Director, T. Tajima

Financial & Administrative coordinator FAC - C. Sarrazin

100 GevPM : K. Nakajima

WP1 - MnagementWP2 - GuidingWP3 - InjectionWP4 - SimulationWP5 - DiagnosticsWP6 - ControlWP7 - Petal integrationWP8 - Relevance to PETAL

C3PM : J. Fuchs

WP1 - Management WP2 - plasma mirrorsWP3 - amplification SBS WP4 - amplification SRS WP5 - self-compressionWP6 - OPCPAWP7 - TargetWP8 - Diagnostics

ICAN -International High Average Power laser and applications -Coordinator : G.

MourouPM : B. Brocklesby

WP1 - ManagementWP21 - Fiber laser componentsWP22 - Fiber laser systemsWP3 - ApplicationsWP4 - Other laser solution to make high energyWP5 - Industrial involvmentWP6 - Public relationsWP7 - Socio economic al impact

Participant Council PaCTechnology transfer

tbcPublic Relation

tbd

Scientific Advisory Board SAB

Secretarytbd

Executive Manager tbd

Dark FieldsPM : K. Homma

WP1 - ManagementWP2 - Light Matter through Wall (LIL or LMJ)WP3 - Degenerate Four-Wave mixing

Steering Committee COPIL

European Commission

FERMILAB

ELI-NPLLMS-ICRILE

SIOM

KEK

LeCosPa(*)

KPSI

APRI

CLPU

NRNU -MEPhI

GSI

JINR(*)

CERN JAI

HHUStrathclydeUniversity

LLNL

INRS

CUOS PULIP

CAEP(*)

IHIP

IAP

TCHILS(*)

ASIA

EUROPE

NORTH

AMERICA

29/01/2014 IZEST-LLNL MOUROU

Page 36: Greeings from M. Spiro - École Polytechnique

100GeV Work Package

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IZEST-LLNL

Scientific Advisory Board (SAB)

SPIRO Michel President of the CERN council (President of SAB) CHAO Alexander SLAC, Stanford University CALDWELL Allen Director, Max-Planck-Institute (Werner-Heiseberg- Institute) Munich CESARSKY Catherine Former « Haut Commissaire » at CEA, Institut de France (Paris) CHEN Pisin National Taiwan University, Leung Center for Cosmology and Particle Astrophysics (LeCosPA) and Stanford University EBISUZAKI Toshikazu Spokesman JEM-EUSO (Extreme Universe Space Observatory), Principal Researcher, RIKEN, Tokyo LAVAL Guy CNRS MOSES Edward NIF Director LLNL OKADA Yasuhiro Executive Director of KEK

Page 38: Greeings from M. Spiro - École Polytechnique

Strathclyde -IZEST 2012 Laser Ascent to High Energy Physics

29/01/2014 IZEST-LLNL MOUROU

THANK YOU!

Page 39: Greeings from M. Spiro - École Polytechnique

IZEST-LLNL MOUROU

IZEST Meeting at Styrathclide Nov. 12 .2012 ‘’Sharing a Laugth with P. Higgs’’

29/01/2014