15–16 Oct 2015
Europe/Zurich timezone

Betatron radiation and laser wakefield acceleration at large scale high energy density science facilities

Speaker

felicie albert (Lawrence Livermore National Laboratory)

Description

The High Energy Density science facilities such as OMEGA, the National Ignition Facility, and in the future the Laser Mega Joule (LMJ), are now uniquely able to recreate in the laboratory conditions of temperature and pressure that were thought to be only attainable in the interiors of stars and planets. To diagnose such transient and extreme states of matter, the development of efficient, versatile and fast (sub-picosecond scale) x-ray probes with energies larger than 50 kilo-electronvolts has become essential for HED science experiments on these specific facilities. We will present results from a recent experiment performed using the Titan laser (150 J, 1 ps) at the Jupiter Laser Facility, LLNL, showing evidence of Betatron x-ray production in the self-modulated regime of laser wakefield acceleration. When a 0.5-1 ps laser pulse with an intensity approaching $10^{20}$ W/cm$^2$ is focused on a gas target (electron density $10^{19}$ cm$^{-3}$), electrons can be accelerated via the self-modulated laser wakefield (SMLWF) regime and the direct laser acceleration (DLA) regime. In SMLWF acceleration, electrons are accelerated by the plasma wave created in the wake of the light pulse, whereas in DLA, electrons are accelerated from the interaction of the laser field with the focusing force of the plasma channel. Experimentally, these two regimes can be distinguished by looking at the laser spectrum transmitted through the gas cell with an optical spectrometer. If the SMLWF mechanism dominates, ($<10^{20}$ W/cm$^2$), the transmitted laser spectrum exhibits intense Raman satellites which measured shifts depend on the electron plasma density. Although Betatron radiation has been observed with picosecond-scale lasers in the DLA regime [1, 2], for normalized vector potentials a0 greater than 10, this experiment constitutes the first observation of Betatron radiation in the SMLWF regime, for a0 ~ 1-3. This was made possible by the addition of a long focal length optics (F/10), favorable for guiding laser pulses in gas targets. We will show a detailed Betatron x-ray source characterization, as well as electron spectra above 200 MeV and forward laser spectra indicating a strongly self-modulated laser wakefield acceleration regime. Perspectives for future experiments on OMEGA-EP, NIF-ARC and LMJ-PETAL will also be discussed. [1] S.P.D. Mangles et al, Phys. Rev. Lett., 94, 245001 (2005). [2] S. Kneip et al, Phys. Rev. Lett., 100, 105006 (2008). *Work performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract DE-AC52-07NA27344 and supported by the LLNL LDRD program under tracking code 13-LW-076.

Primary author

felicie albert (Lawrence Livermore National Laboratory)

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