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All-optical accelerators

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Presentation on theme: "All-optical accelerators"— Presentation transcript:

1 All-optical accelerators
LOASIS Program: All-optical accelerators Wim Leemans LOASIS Program Accelerator and Fusion Research Division Website:

2 Acknowledgment Staff/students of l’OASIS team
E. Esarey, C.Filip*, G. Fubiani, C. Geddes, E. Michel*, P. Michel, B. Nagler, K. Nakamura, C. Schroeder, B. Shadwick, C. Toth, J. van Tilborg, D. Syversrud, M. Dickinson, N. Ybarrolazza, J. Wallig *University of Nevada, Reno Primary Collaborators S. Hooker, A. Gonsalves- Oxford University D. Jaroszynski-Strathclyde, AlphaX T. Cowan, N. Le Galloudec, H. Ruhl, A. Kemp- UNR J. Cary, D. Bruhwiler, D. Dimitrov-U Colorado Boulder, TechX-Corp DOE -HEP Advanced Accelerator Technology 7 3 2 1 1 1 1 1

3 Challenges Building a high energy collider: Radiation source
Single stage ? 200 m long plasma, BIG laser (200 PW for 1 TeV?) Will beam remain stable ? Will emittance be OK? Multi-stage ? How to stage ? Build 10 GeV module, how to couple beams in and out ? How to manage , PW systems? 100 Hz? Radiation source Coherent emission: THz X-FEL: is beam quality good enough ? Energy spread Emittance Maintaining peak current: bunch propagation Particle source: fs, MeV electron bunches, pC, 10 micron spot, E/E <<

4 Experimental activities/focus
10 TW system High density plasma channels “Low” phase velocity wakes Dark current free structure 100 MeV-class beams Injection physics THz and X-rays 100 TW system Low density plasma channels “High” phase velocity wakes 1 GeV module Capillary discharge: Collab. With Oxford (UK) CCD & Spectrometer 2w probe Interferometer Heater beam e- H, He gas jet Main beam Ignitor Beam

5 + Next step: 1 GeV compact module 100 TW laser + plasma channel Plasma
A. Reitsma et al., PR-STAB 2001 Plasma injector Plasma channel e- beam < 3mm < 10 cm 1.2 GeV Laser 100 TW, 40 fs 10 Hz Collaboration with Oxford University and Alpha-X Bigger laser 2-7 cm long +

6 LWFA’s brightness offers unique opportunities
Brightness = (beam power)/(phase space volume) Brightness Particle energy [GeV] Brightness vs. g SLAC FFTB 10 GeV LWFA 1 GeV LWFA LOA LBNL RAL Photocathode Thermionic Data: Nature 2004

7 Single drive beam experiments have been conducted for laser accelerator produced THz and X-rays
Set-up for E-O effect THz emitted at vacuum-plasma boundary Short bunches result in coherent emission Radiation source+bunch diagnostic Radiation characterized via: Michelson interferometer Semiconductor switching Electro-optic effect in ZnTe THz TR 50fs Probe Beam (800nm) Polarizer Analyzer ZnTe Diode Chamber /4

8 Time Jitter and Stability
Shot-to-shot stability in charge and bunch duration enables scanning E-O sampling technique Time Jitter and Stability Jitter e-beam & probe beam must be << 30 fs Charge Stability over Time < 5 % rms Spectrum consistent with 50 fs bunch THz depends primarily on charge, bunch duration Shot-to-shot stability of those quantities J. Van Tilborg et al., in preparation

9 Ultra-short x-ray generation from laser accelerated e-beams
Betatron emission: “Spontaneously” emitted Detector testing First phase of x-ray diagnostic Collaborations: LLNL UNR lu lx=lu/2g2 Betatron (synchrotron) radiation: E. Esarey et al., PRE 2002 A. Rousse et al., PRL 2004 parameters: Q=03 nC E=100 MeV rb=3 mm ne=2 x1019 cm-3 Lchannel=1 mm

10 LOASIS Program at LBNL Tools: multi-beam, multi-arm laser
Radiation shielded experimental areas+remote control room Two target areas: 10 TW (+10 TW), 3 independent vacuum compressors 100 TW arm Physics: Precision frontier: all-optical injection enabled by discovery of dark current free structure High energy acceleration: Channel guided laser wakefield: 100 MeV (Nature 2004) Capillary discharge + injection: towards 1 GeV Radiation sources: taking advantage of peak brightness Intense THz via coherent transition radiation (PRL 2003, PRE 2004, PRL 2005(submitted)) Incoherent x-rays: betatron, Thomson scattering-gamma rays Coherent x-rays: XFEL

11 LOASIS Program FY05: Staff + visitors and students


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