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Relativistic plasma surfaces as an efficient second harmonic generator

  • M. J.V. Streeter
  • , P. S. Foster
  • , F. H. Cameron
  • , M. Borghesi
  • , C. Brenner
  • , D. C. Carroll
  • , E. Divall
  • , N. P. Dover
  • , B. Dromey
  • , P. Gallegos
  • , J. S. Green
  • , S. Hawkes
  • , C. J. Hooker
  • , S. Kar
  • , P. McKenna
  • , S. R. Nagel
  • , Z. Najmudin
  • , C. A.J. Palmer
  • , R. Prasad
  • , K. E. Quinn
  • P. P. Rajeev, A. P.L. Robinson, L. Romagnani, J. Schreiber, C. Spindloe, S. Ter-Avetisyan, O. Tresca, M. Zepf, D. Neely
  • Central Laser Facility
  • Imperial College London
  • Queen's University of Belfast
  • University of Strathclyde
  • CEA/UVSQ/CNRS
  • Max-Planck Institut für Quantenoptik
  • Universität München

Research output: Contribution to journalArticlepeer-review

Abstract

We report on the characterization of the specular reflection of 50 fs laser pulses in the intensity range 1017-1021Wcm-2 obliquely incident with p-polarization onto solid density plasmas. These measurements show that the absorbed energy fraction remains approximately constant and that second harmonic generation (SHG) achieves efficiencies of 22±8% for intensities approaching 1021Wcm-2. A simple model based on the relativistic oscillating mirror concept reproduces the observed intensity scaling, indicating that this is the dominant process involved for these conditions. This method may prove to be superior to SHG by sum frequency mixing in crystals as it is free from dispersion and retains high spatial coherence at high intensity.

Original languageEnglish
Article number023041
JournalNew Journal of Physics
Volume13
DOIs
Publication statusPublished - 1 Jan 2011
Externally publishedYes

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