Greeings from M. Spiro
Transcription
Greeings from M. Spiro
IZEST-LLNL July 17-18 2012 3rd IZEST SYMOSIUM - Peter Higgs Chris Barty Gerard Mourou Toshiki Tajima150th Anniversary of Politecnico di Milano 29/01/2014 IZEST-LLNL MOUROU - Charles H. Townes IZEST: Laser Transition from Atomic to Subatomic Physics from Particle to Photon 29/01/2014 IZEST-LLNL MOUROU 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 Extreme Light Road Map LMJ/NIF, 2MJ, 3B€ MJ Vacuum Polarization Ep=mpc2 Ee=m0c2 TeV IZEST C3 kJ J mJ 29/01/2014 ELI, kJ .3 B€ XCELS IZEST-LLNL MOUROU GeV MeV MeV eV 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 The Pulse Duration-Intensity Conjecture G.A. Mourou and T. Tajima, “More intense Shorter Pulse”, SCIENCE VOL 331 , 7 , p 41JANUARY 2011 29/01/2014 IZEST-LLNL MOUROU IZEST Benefits from the largest Pump Lasers Up to the MJ 29/01/2014 PETAL-LMJ IZEST-LLNL MOUROU NIF LLNL IZEST Particle Physics Ascent 1TeV-PETAL, LFEX, NIF, XCELS 100GeV-PETAL 2015 LFEX 10GeV-GSI 2013 29/01/2014 1GeV IZEST-LLNL MOUROU 29/01/2014 IZEST-LLNL MOUROU IZEST’s Mission: Responding to Suzuki’s New Paradigm Challenge PeV Leptogenesis SUSY breaking Extra dimension Dark matter Supersymmetry TeV Atsuto Suzuki: KEK Director General, 29/01/2014 ICFA Chair IZEST-LLNL MOUROU Standard Model Quarks Leptons Laser Wake Field Acceleration Source of high energy electrons and photons 29/01/2014 IZEST-LLNL MOUROU T. Tajima J. Dawson PeV Accelerator With conventional Technology The accelerator would Girdle the Earth: Fermi’s vision (1954) 1km laser Plasma accelerator with LIL or LMJ (Vision 2011) 29/01/2014 IZEST-LLNL MOUROU 130GeV Experiment on the PETAL laser 29/01/2014 IZEST-LLNL MOUROU From N. Narozhny nperp -1 4 º npar -1 7 29/01/2014 IZEST-LLNL MOUROU 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. 29/01/2014 IZEST-LLNL MOUROU 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 29/01/2014 IZEST-LLNL MOUROU IZEST Technology 29/01/2014 IZEST-LLNL MOUROU 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 Amplification: Backward Raman or Brillouin Amplification Electron Plasma Wave or Ion-acoustic Wave in the Strong-Coupled Regime LCell = cTpump 2 Backwards Raman Amplification(BRA) V. M. Malkin, G. Shvets, and N. J. Fisch, “Phys. Rev. Lett. 82, 4448(1999). S. Suckewer et al. Nature Phys. Oct. 2007 29/01/2014 IZEST-LLNL MOUROU 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 29/01/2014 IZEST-LLNL MOUROU Focusing Ultrahigh Intensity Beam Plasma Optics 5-10 kJ/cm2 Damage Threshold Optics 100kJ~ 3cm diameter 29/01/2014 IZEST-LLNL MOUROU Towards the MW Average Power The ICAN project 29/01/2014 IZEST-LLNL MOUROU ICAN European Commission Project TeV Collider 29/01/2014 IZEST-LLNL MOUROU Laser Wake field Acceleration 40W GeV, 100 pC ~ 100mW. 29/01/2014 IZEST-LLNL MOUROU 1TGV=10MW .4TGV 29/01/2014 IZEST-LLNL MOUROU HIGH PEAK POWER LASER AVERAGE POWER: FROM THE LIGHT BULB(W) TO TGV(MW) 10MW 50W 29/01/2014 IZEST-LLNL MOUROU Nature Photonics April, 2013 IZEST-LLNL MOUROU 29/01/2014 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 » 29/01/2014 IZEST-LLNL MOUROU 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….. 29/01/2014 IZEST-LLNL MOUROU 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 Laser-Based High Energy and Fundamental Physics: Exawatt to Zettawatt ELI IZEST 2010 29/01/2014 2015 XCELS 2020 2025 IZEST-LLNL MOUROU 2030 LMJ, NIF Organization Chart - Provisional Steering Committee COPIL Secretary tbd Director, G. Mourou Deputy Director, T. Tajima Financial & Administrative coordinator FAC - C. Sarrazin Scientific Advisory Board SAB Executive Manager tbd Participant Council PaC Public Relation tbd European Commission 100 Gev PM : K. Nakajima WP1 - Mnagement WP2 - Guiding WP3 - Injection WP4 - Simulation WP5 - Diagnostics WP6 - Control WP7 - Petal integration WP8 - Relevance to PETAL CAEP(*) A S I A KEK C3 PM : J. Fuchs Dark Fields PM : K. Homma WP1 - Management WP2 - Light Matter through Wall (LIL or LMJ) WP3 - Degenerate Four-Wave mixing WP1 - Management WP2 - plasma mirrors WP3 - amplification SBS WP4 - amplification SRS WP5 - self-compression WP6 - OPCPA WP7 - Target WP8 - Diagnostics KPSI APRI LeCosPa(*) SIOM ILE LLMS-ICR IHIP 29/01/2014 (*)Pending Technology transfer tbc N O R T H FERMILAB LLNL A M E R I C A CUOS PULIP TCHILS(*) INRS IZEST-LLNL MOUROU E U R O P E ICAN -International High Average Power laser and applications -Coordinator : G. Mourou PM : B. Brocklesby WP1 - Management WP21 - Fiber laser components WP22 - Fiber laser systems WP3 - Applications WP4 - Other laser solution to make high energy WP5 - Industrial involvment WP6 - Public relations WP7 - Socio economic al impact CERN JAI GSI Strathclyde University HHU IAP ELI-NP JINR(*) CLPU NRNU MEPhI 100GeV Work Package 29/01/2014 IZEST-LLNL MOUROU 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 Strathclyde -IZEST 2012 Laser Ascent to High Energy Physics THANK YOU! 29/01/2014 IZEST-LLNL MOUROU IZEST Meeting at Styrathclide Nov. 12 .2012 ‘’Sharing a Laugth with P. Higgs’’ 29/01/2014 IZEST-LLNL MOUROU