Published April 2006 | Version v1
Journal article

Fast-electron transport and heating of solid targets in high-intensity laser interactions measured by Kα fluorescence

  • 1. Laboratoire pour l'Utilisation des Lasers Intenses, UMR7605, CNRS-CEA-Universite Paris VI-Ecole Polytechnique, 91128 Palaiseau (France)
  • 2. Dipartimento di Fisica 'G. Occhialini', Universita di Milano-Bicocca, Piazza della Scienza 3, 20126 Milan (Italy)
  • 3. Commissariat a l'Energie Atomique-DAM, Bruyeres-le-Chatel (France)
  • 4. University of Essex, Colchester CO4 3SQ (United Kingdom)
  • 5. Lawerence Livermore National Laboratory, Livermore, California (United States)
  • 6. University of California Davis, Davis, California (United States)
  • 7. Inertial Fusion Technology Division, Energy Group, General Atomics, San Diego, California 92121 (United States)
  • 8. Central Laser Facility, Rutherford Appleton Laboratory, Chilton (United Kingdom)

Description

We present experimental results on fast-electron energy deposition into solid targets in ultrahigh intensity laser-matter interaction. X-ray Kα emission spectroscopy with absolute photon counting served to diagnose fast-electron propagation in multilayered targets. Target heating was measured from ionization-shifted Kα emission. Data show a 200 μm fast-electron range in solid Al. The relative intensities of spectrally shifted Al Kα lines imply a mean temperature of a few tens of eV up to a 100 μm depth. Experimental results suggest refluxing of the electron beam at target rear side. They were compared with the predictions of both a collisional Monte Carlo and a collisional-electromagnetic, particle-fluid transport code. The validity of the code modeling of heating in such highly transient conditions is discussed

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics
Journal Volume
73
Journal Issue
4
Journal Page Range
p. 046402-046402.5
ISSN
1063-651X
CODEN
PLEEE8

Optional Information

Notes
(c) 2006 The American Physical Society