PIC Modeling of Relativistic Electron Transport Experiments on Omega EP

POSTER

Abstract

Recent experiments on the Omega EP laser system have used an intense laser ($I \sim 10^{19} W/{cm}^2$, $\tau \sim 8ps$) striking Au foil to generate a relativistic electron beam, which is subsequently transported through either CH plasma or room temperature CH foam, and then diagnosed with Cu $K \alpha$ from a Cu foil. An order of magnitude lower $K \alpha$ emission is seen in the plasma case compared to the cold case. We use the particle-in-cell code OSIRIS to model the experiment in the case of pre-formed plasma. Our 2D simulations show a similarly broad transverse profile as experiment. We also see a strong filamentary B-field in the CH region directly adjacent to the gold, with filaments similarly diverging from the laser spot. Increasing the CH density dampens these filaments, and leads to a more intense and more collimated electron spectrum in the Cu region, consistent with experiment.

*The authors acknowledge support by Fusion Science Center for Matter Under Extreme Conditions, NSF under PHY-0904039, DOE under DE-FG52-09NA29552, and of the HiPER project (EC FP7 project number 211737).

Authors

  • Josh May

    • UCLA
  • J. Tonge

    • UCLA
  • W.B. Mori

    • UCLA
  • F. Beg

    • UCSD
  • C. McGuffey

    • UCSD
  • M. Wei

    • UCSD
  • R. Fonseca

    • GoLP/IPFN\&IST