Hostname: page-component-76fb5796d-5g6vh Total loading time: 0 Render date: 2024-04-25T15:58:22.311Z Has data issue: false hasContentIssue false

Two-dimensional semi-Lagrangian Vlasov simulations of laser–plasma interaction in the relativistic regime

Published online by Cambridge University Press:  01 October 1999

M. L. BÉGUÉ
Affiliation:
Laboratoire de Physique des Milieus Ionisés, UPRES A 7040, France
A. GHIZZO
Affiliation:
Laboratoire de Physique des Milieus Ionisés, UPRES A 7040, France
P. BERTRAND
Affiliation:
Laboratoire de Physique des Milieus Ionisés, UPRES A 7040, France
E. SONNENDRÜCKER
Affiliation:
Institut Elie Cartan de Nancy, Université Henri Poincaré Nancy I, BP 239, 54 506 Vandoeuvre les Nancy, Cedex, France
O. COULAUD
Affiliation:
Institut Elie Cartan de Nancy, Université Henri Poincaré Nancy I, BP 239, 54 506 Vandoeuvre les Nancy, Cedex, France

Abstract

A semi-Lagrangian two-dimensional fully relativistic Vlasov code for multicomputer environments is developed to study trapped-particle dynamics in phase space induced by relativistic modulational and Raman instabilities. Attention is focused on the efficiency properties of the numerical scheme, which allows a very fine description of particle dynamics in phase space. Vlasov simulations show the appearance of coherent vortex structures as a result of the nonlinear saturation mechanism of the relativistic modulational instability. Growth rates are computed and found to be in good agreement with theoretical values obtained from the dispersion relation by Quesnel et al, [Phys. Plasmas4, 3358–3368 (1997)] and Guérin et al. [Phys. Plasmas2, 2807–2814 (1995)]. In the case of coupling between the relativistic modulational instability and two-plasmon decay, stochastic behaviour can be observed due to the competition between different plasmas waves.

Type
Research Article
Copyright
© 1999 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)