Numerical Modeling of Relativistic Harmonic Structure from Plasma Mirrors: Insights into Relativistic Plasma Dynamics

POSTER

Abstract

Specular reflection of intense lasers from relativistic plasma mirrors produces a source of high-power, broad bandwidth radiation which, in addition to being a useful secondary light source for probing electron dynamics, encodes the information of the complex plasma dynamics that takes place during extreme light-matter interactions. The appearance of harmonic peaks in the reflected spectrum can be explained as a result of periodically spaced attosecond pulses emitted once every laser cycle. For multi-cycle laser pulses, cycle-to-cycle emission times of attosecond pulses varies due to evolving laser and plasma parameters. In this work, we use particle-in-cell simulations to relate the temporal spacing of attosecond pulses to different observed harmonic structure, including harmonic broadening, harmonic splitting, and the appearance of integer and half-integer harmonics. We demonstrate how a small amount of temporal chirp applied to the driving laser can compensate for the non-periodic emission time of attosecond pulses which results in narrower, more intense individual harmonics. The results of this work provides insight into the rapidly evolving plasma dynamics of intense laser-solid interactions and how these dynamics are encoded in the reflected radiation.

*The EPOCH code was developed as part of the UK EPSRC 300 360 funded project EP/G054940/1. This work was supported by NSF Grant No. PHY 1806911, DOE grant No. DE-SC0017907, and from the Program of Plasma Science and Technology (PPST).

Authors

  • Nicholas Fasano

    • Princeton Univ.
    • Princeton University
  • Julia Mikhailova

    • Princeton University