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Jeans instability in a magneto-radiative dusty plasma

Published online by Cambridge University Press:  01 December 2008

N. L. TSINTSADZE
Affiliation:
Institute of Physics, Tbilisi, GeorgiaDepartment of Physics, G. C. University, Lahore 54000, Pakistan (hashah.gcl@gmail.com)Salam Chair in Physics, G. C. University, Lahore 54000, Pakistan
ROZINA CHAUDHARY
Affiliation:
Department of Physics, G. C. University, Lahore 54000, Pakistan (hashah.gcl@gmail.com)Salam Chair in Physics, G. C. University, Lahore 54000, Pakistan
H. A. SHAH
Affiliation:
Department of Physics, G. C. University, Lahore 54000, Pakistan (hashah.gcl@gmail.com)
G. MURTAZA
Affiliation:
Salam Chair in Physics, G. C. University, Lahore 54000, Pakistan
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Abstract

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The importance of thermal radiation on the Jeans instability is discussed for a magnetized dusty plasma with gravitational effects. The one-fluid MHD equations are developed by assuming that the entropy of each subsystem of plasma is conserved, when the temperature of the plasma species is non-relativistic. The dispersion relation in this case shows that thermal radiation helps to stabilize the Jeans instability. It is shown that the plasma is stable in a certain range of wavelengths. The magnetic field stabilizes the Jeans instability when the wave propagates across the magnetic field. However, for oblique propagation it is seen that the magnetic field does not stabilize the Jeans instability.

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Copyright
Copyright © Cambridge University Press 2008