Radiation-condensation instability in a self-gravitating dusty astrophysical plasma

P. K. Shukla and I. Sandberg
Phys. Rev. E 67, 036401 – Published 7 March 2003
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Abstract

Properties of radiation-condensation instability in a partially-ionized self-gravitating dusty astrophysical plasmas are studied. For this purpose, new dispersion relations for coupled dusty plasma and condensation modes in both unmagnetized and magnetized plasmas are derived. The dispersion relations are numerically analyzed to investigate the interplay between self-gravitation and impurity losses, as well as to study the effects of the external magnetic field and finite plasma beta on instabilities we found.

  • Received 10 October 2002

DOI:https://doi.org/10.1103/PhysRevE.67.036401

©2003 American Physical Society

Authors & Affiliations

P. K. Shukla* and I. Sandberg

  • Institut für Theoretische Physik IV, Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany

  • *Also at the Department of Plasma Physics, Umeå University, SE-90187 Umeå, Sweden, and at the Center for Interdisciplinary Plasma Science, Max-Planck-Institut für Extraterrestrische Physik und Plasmaphysik, D-45740 Garching, Germany.

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Vol. 67, Iss. 3 — March 2003

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