Greeings from M. Spiro - École Polytechnique
Transcript of Greeings from M. Spiro - École Polytechnique
- Peter Higgs
- Charles H. Townes Chris Barty
Gerard Mourou
Toshiki Tajima150th Anniversary of
Politecnico di Milano
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IZEST-LLNL July 17-18 2012
3rd IZEST SYMOSIUM
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IZEST: Laser Transition from Atomic to Subatomic Physics
from Particle to Photon
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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, .)
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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
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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.
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The Pulse Duration-Intensity Conjecture
G.A. Mourou and T. Tajima, “More intense Shorter Pulse”, SCIENCE VOL 331 , 7 , p 41JANUARY 2011
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IZEST Benefits from the largest Pump Lasers Up to the MJ
PETAL-LMJ NIF LLNL 29/01/2014 IZEST-LLNL MOUROU
IZEST Particle Physics Ascent
1GeV
100GeV-PETAL 2015 LFEX
1TeV-PETAL, LFEX, NIF, XCELS
10GeV-GSI 2013
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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
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Laser Wake Field Acceleration Source of high energy electrons and photons
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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)
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130GeV Experiment
on the PETAL laser
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From N. Narozhny
nperp -1
npar -1º
4
7
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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.
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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
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IZEST Technology
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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
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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
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S. Suckewer et al. Nature Phys. Oct. 2007
Electron Plasma Wave or Ion-acoustic Wave in the Strong-Coupled Regime
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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
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Focusing Ultrahigh Intensity Beam
Plasma Optics 5-10 kJ/cm2 Damage Threshold Optics
100kJ~ 3cm diameter
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Towards the MW Average Power The ICAN project
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ICAN European Commission Project
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TeV Collider
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Laser Wake field Acceleration
GeV, 100 pC ~ 100mW.
40W
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.4TGV
1TGV=10MW
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HIGH PEAK POWER LASER AVERAGE POWER: FROM THE LIGHT BULB(W) TO TGV(MW)
50W
10MW
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Nature Photonics April, 2013
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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 »
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Conventional Accelerator Technology
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…..
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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
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Laser-Based High Energy and Fundamental Physics: Exawatt to Zettawatt
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2015 2010 2020 2025 2030
IZEST XCELS LMJ, NIF ELI
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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
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100GeV Work Package
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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
Strathclyde -IZEST 2012 Laser Ascent to High Energy Physics
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THANK YOU!
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IZEST Meeting at Styrathclide Nov. 12 .2012 ‘’Sharing a Laugth with P. Higgs’’
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