corner
corner

Phys. Rev. A 68, 063201 (2003) [8 pages]

Time-dependent Boltzmann kinetic model of x rays produced by ultrashort-pulse laser irradiation of argon clusters

Download: PDF (108 kB) Buy this article Export: BibTeX or EndNote (RIS)

J. Abdallah, Jr. and G. Csanak
Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

Y. Fukuda, Y. Akahane, M. Aoyama, N. Inoue, H. Ueda, and K. Yamakawa
Advanced Photon Research Center, Japan Atomic Energy Research Institute (JAERI), 8-1 Umemidai, Kizu-cho, Souraku-gun, Kyoto 619-0215, Japan

A. Ya. Faenov, A. I. Magunov, T. A. Pikuz, and I. Yu. Skobelev
Multicharged Ions Spectra Data Center of VNIIFTRI, Mendeleevo, Moscow Region 141570, Russia

Received 18 July 2003; published 12 December 2003

The Boltzmann equation and a detailed collisional-radiative model are solved simultaneously as a function of time to model the time-integrated x-ray spectra of the transient plasma produced by a high intensity ultrafast laser source. Level populations are calculated by solving the rate equations as a function of time using rate coefficients corresponding to a time varying electron energy distribution function (EEDF) determined by the solution to the Boltzmann equation. Electron-electron interactions are included through the solution of the Fokker-Planck equation. It is assumed that all the ions are initially in the Ne-like ground state due to the laser prepulse and that all free electrons have high energy (5 keV) from the fast laser deposition. The collisional-radiative model included over 3000 levels in the Ne-like through H-like ion stages of argon. The results are in agreement with highly resolved F-like to He-like K-shell emission spectra recorded recently during ultrashort laser experiments with argon cluster targets in Japan. The calculated time scale for emission is consistent with estimates of cluster decay times for these conditions. The calculations also show that the typical Li-like and Be-like satellite structure, sometimes attributed to a hot-electron component in the EEDF, can also be due to transient effects in a high-temperature ionizing plasma.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.68.063201
DOI:
10.1103/PhysRevA.68.063201
PACS:
36.40.Vz, 52.50.Jm, 52.70.La