Extreme Light Infrastructure ELI. Recommended to be on the ESFRI Road Map

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Extreme Light Infrastructure ELI Recommended to be on the ESFRI Road Map

ELI Centered around an Exawatt class Laser Few kj.~10fs, >1sh/mn) Modular: 1) front end at 100Hz-kHz, 5fs-5J, PW level, 2) Last stage at the exawatt level@>1shot/mn 3) a 0 ~10 2-10 4

ELI Scientific Program: Rests on Three Scientific Pillars Ultra high Field Science: access to the ultra-relativistic regime, ELI will afford new investigations in particle physics, nuclear physics, gravitational physics, nonlinear field theory, ultrahigh-pressure physics, 1 astrophysics and cosmology. ) Attosecond science: snap-shots in the attosecond scale of the electron dynamics in atoms, molecules, plasmas and solids. High Energy beam facility: ELI will provide ultra-short energetic particle (>10 GeV) and radiation (up to few MeV) beams produced from compact laser plasma accelerators.

Societal Benefits ELI will afford wide benefits to society ranging from improvement of oncology treatment, medical imaging, fast electronics and our understanding of aging nuclear reactor materials to development of new methods of nuclear waste processing.

Relativistics microelectronic ELI devices 1 m RF cavity 100 μm Plasma cavity Courtesy of W. Mori

Extreme Light Infrastructure Exawatt Laser ELI Secondary a cbeam Sources S c Electrons y e n Positron l c e ion h r Muon r a. Neutrino t X o Neutrons f r X rays e s l γ rays Fundamental Interaction Ultra-Relativistic optics Super hot plasma Nuclear Physics Astrophysics General relativity Ultra fast phenomena NLQED Relativistic Engineering Attosecond optics Rel. Microelectronic Rel. Microphotonic Nuclear treatement Nuclear pharmacology Hadron therapy Radiotherapy Material science

Electron beam energy and laser power evolution ELI 10 6 «conventional» technology 10 1 Maximale Electrons Energy (MeV) 10 5 10 4 10 3 10 2 10 LOA *LUND RAL LOA UCLA KEK *LBNL ILE UCLA E L I *LBNL 10 16 10 15 10 14 10 13 10 12 Laser Power (W) LULI 1 1930 1940 1950 1960 190 1980 1990 2000 2010 Years INFN, Frascati, March (2006)

Parameter designs Laser Plasma Accelerators ELI ELI : > 100 GeV P(PW) E(J) 0.12/3.6 τ (fs) 30 n e (cm -3 ) 2e18 W 0 (μm) 15 L(m) 0.009 a 0 4 Q(nC) 1.3 E(Gev) 1.12 1.2/120 100 2e1 4 0.28 4 4 11.2 12/3.6k 300 2e16 150 9 4 13 112 120/120 K 1000 2e15 40 280 4 40 1120 Golp and UCLA Group

Extreme Light Infrastructure ELI ELI A science integrator that will bring many frontiers of contemporary physics, i.e. relativistic plasma physics, particle physics, nuclear physics, gravitational physics, nonlinear field theory, ultrahigh pressure physics, and cosmology together. ELI will provide a new generation of compact accelerators delivering ultra short (fs-as) and energetic particle and radiation beams for European scientists. ELI will work in close contact with synchrotron XFEL community. ELI will also be an Extreme Light technology platform ready to reduce to practice the latest invention and discovery in relativistic engineering

Education and Training: ELI will be the most sophisticated Optoelectronic Grand Instrument (Ultrashort short pulse, Ultra relativistic intensity, High repetition rate, wavefront correction, Coherent Addition of Beams) and will be a fertile ground for Education and Training.

Time line 200 2008 2009 2010 2011 2012 2013 2014 10/20 PW @ 1shot/mn single beam 40/0 PW @ 1Hz single beam 400/00 PW @ 1Hz 10 beams

G.IV ELI budget summary over the first 10 years (in M ) Years 1 2 3 4 5 6 8 9 10 Total Equipment Laser (phase 1) 20 15 10 45 Equipment Laser (phase 2) 30 21 51 Equipment Exp. beamlines 5 3 3 2 20 Total equipment 2 20 13 33 23 116 Building 8 15 Manpower for laser/ beamline 1,5 1,5 1,5 1,5 1,5,5 Manpower for exploitation 0,2 0,6 0,8 1.0 1.0 1.0 1.0 1.0 6.6 Operation and maintenance costs Total/ year 0, 3,2 1,4 29,9 3,6 18,2 4,8 39,6 31,9,5,5,5,5,5 52.5 19,6

ELI Participating Countries France Germany Spain Italy Greece Lithuania Austria

ELI Participants 1 LULI, CNRS-X, CEA, Université Paris XI, 91128 Palaiseau (France) 2 LOA, CNRS-ENSTA-X, 9161 Palaiseau (France) 3 Johannes-Gutenberg-Universitat Mainz, D 55099 Mainz (Germany) 4 GSI, Planckstr.1 64291 Darmstadt (Germany) 5 LLR, CNRS-IN2P3-X, 91128 Palaiseau (France) 6 Thalès, STI, 9204 Colombes cedex (France) 8 General Physics Institute RAS, Moscow 119991 (Russia) 9 IESL (Heraklion) 1110, Crete (Greece) 10 Institut für Angewandte PM, D-855 Neubiberg (Germany) 11 IOTA, Bât 503, 91403 ORSAY Cedex (France) 12 CPO, Bat. 101, 91898 Orsay cedex (France) 13 FASTLITE Bâtiment 403 Campus de l'x 91128 Palaiseau (France) 14 LMU, Am Coulombwall 1, D-8548 Garching (Germany) 15 CENBG, CNRS, IN2P3, Université Bordeaux 1 (France) 16 Max-Planck-Institut fuer Kernphysik, Heidelberg D- 6911 (Germany) 1 Heinrich-Heine-Universitaet Duesseldorf, D-40225 Duesseldorf 18 MPQ, Max-Planck-Institut fur Quantenoptik, D-8548 Garching 19 Imperial College, Imperial College London, SW 2AZ London (U. K.) 20 Dept. of Physics,Univ of Strathclyde, Glasgow G4 0NG (Scotland) 21 Centre de Physique Theorique, CNRS-X, 91128 Palaiseau (France) 22 Dipartimento di Fisica,Universita' di Pisa, 56100 Pisa (Italy) 23 LSI, CNRS-X, F-91128, Palaiseau (France) 24 Department of Quantum Electronics, LT-10222 Vilnius (Lithuania) 25 LIXAM, CNRS-Université Paris XI, Bât 350, 91405 Orsay (France) 26 Institut für Optik und Quantenelektronik, D043 Jena (Germany) 2 ESFR, 6, rue Jules Horowitz,BP 220, Grenoble 38043 (France) 28 Technische Universität Dresden, ITP, 01062 Dresden (Germany) 29 CELIA, Universite Bordeaux 1, 33405 Talence cedex (France) 30 Amolf FOM, Kruislaan 40, 1098 SJ Amsterdam (The Netherlands)