Effects of background pressure on high repetition rate, relativistic laser-driven MeV ion and electron acceleration

ORAL

Abstract

The relativistic laser-plasma interaction (LPI) can produce energetic electrons, ions, and photons. LPI studies are increasingly moving towards high repetition rate in order to collect more data and demonstrate real world applicability. Liquid targets can provide repeatable, thin targets for high repetition rate LPI experiments, but may require higher vacuum pressure than what is commonly used. Therefore, it is important to understand how the chamber pressure effects particle acceleration and determine necessary pressure limits for target development. We present results from a series of experiments on the effect of background pressure on particle acceleration with pressures ranging from 30 mTorr to >10 Torr. In particular, we show a substantial increase in conversion efficiency to target normal ions when the chamber pressure drops below ~1 Torr. These studies facilitate future experimental design on particle acceleration and inform target development for high repetition rate LPI experiments.

*This research was sponsored by the Air Force Office of Scientific Research through program managers Dr. Enrique Parra and Dr. Jean-Luc Cambier. This research was partially funded through the HPCMP High Performance Computing Internship Program and the AFRL Summer Faculty Fellowship Program.

Presenters

  • Joseph C Snyder

    • Miami University, Hamilton, OH
    • Miami Univ
    • Miami Univ - Hamilton

Authors

  • Joseph C Snyder

    • Miami University, Hamilton, OH
    • Miami Univ
    • Miami Univ - Hamilton
  • John T Morrison

    • Innovative Scientific Solutions, Inc., Dayton, OH
    • Innovative Scientific Solutions Inc., Dayton, OH
    • Innovative Scientific Solutions Inc. - Dayton, OH
    • Innovative Scientific Solutions, Inc.
    • Innovative Scientific Solutions Inc.
  • Kevin M George

    • Innovative Scientific Solutions Inc., Dayton, OH
    • Innovative Scientific Solutions Inc. - Dayton, OH
    • Innovative Scientific Solutions, Inc.
    • Innovative Scientific Solutions Inc.
  • Gregory K. Ngirmang

    • Innovative Scientific Solutions, Inc., Dayton, OH
    • Innovative Scientific Solutions Inc., Dayton, OH
    • Ohio State Univ - Columbus
    • Innovative Scientific Solutions, Inc.
    • Innovative Scientific Solutions Inc.
  • Scott B Feister

    • The University of Chicago, Flash Center, Chicago, IL
    • Univ of Chicago
  • Joe R Smith

    • The Ohio State University, Department of Physics, Columbus, OH
    • Ohio State Univ - Columbus
  • Manh S Le

    • The Ohio State University, Department of Physics, Columbus, OH
  • Kyle Frische

    • Innovative Scientific Solutions Inc., Dayton, OH
    • Innovative Scientific Solutions Inc. - Dayton, OH
    • Innovative Scientific Solutions, Inc.
    • Innovative Scientific Solutions Inc.
  • Enam A Chowdhury

    • The Ohio State University, Department of Physics, Columbus, OH
    • The Ohio State University, Department of Physics, Columbus, OH, Intense Energy Solutions Inc., Dayton, OH
    • Ohio State Univ - Columbus
    • The Ohio State University, Department of Physics, Columbus, OH, Intense Energy Solutions, Inc., Dayton, OH
  • Chris M Orban

    • Innovative Scientific Solutions, Inc., Dayton, OH, The Ohio State University, Department of Physics, Columbus, OH
    • The Ohio State University, Department of Physics, Columbus, OH, Innovative Scientific Solutions Inc., Dayton, OH
    • Ohio State Univ - Columbus
    • The Ohio State University, Department of Physics, Columbus, OH, Innovative Scientific Solutions, Inc.
  • William M Roquemore

    • Air Force Research Laboratory, Aerospace Directorate, WPAFB, OH