Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma
Joint Authors
Kaothekar, Sachin
Chhajlani, R. K.
Source
ISRN Astronomy and Astrophysics
Issue
Vol. 2012, Issue 2012 (31 Dec. 2012), pp.1-14, 14 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2012-09-29
Country of Publication
Egypt
No. of Pages
14
Main Subjects
Abstract EN
The effect of radiative heat-loss function and finite ion Larmor radius (FLR) corrections on the self-gravitational instability of infinite homogeneous viscous plasma has been investigated incorporating the effects of thermal conductivity and finite electrical resistivity for the formation of a star in astrophysical plasma.
The general dispersion relation is derived using the normal mode analysis method with the help of relevant linearized perturbation equations of the problem.
Furthermore the wave propagation along and perpendicular to the direction of external magnetic field has been discussed.
Stability of the medium is discussed by applying Routh Hurwitz’s criterion.
We find that the presence of radiative heat-loss function and thermal conductivity modify the fundamental Jeans criterion of gravitational instability into radiative instability criterion.
From the curves we see that temperature dependent heat-loss function, FLR corrections and viscosity have stabilizing effect, while density dependent heat-loss function has destabilizing effect on the growth rate of self-gravitational instability.
Our result shows that the FLR corrections and radiative heat-loss functions affect the star formation.
American Psychological Association (APA)
Kaothekar, Sachin& Chhajlani, R. K.. 2012. Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma. ISRN Astronomy and Astrophysics،Vol. 2012, no. 2012, pp.1-14.
https://search.emarefa.net/detail/BIM-470876
Modern Language Association (MLA)
Kaothekar, Sachin& Chhajlani, R. K.. Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma. ISRN Astronomy and Astrophysics No. 2012 (2012), pp.1-14.
https://search.emarefa.net/detail/BIM-470876
American Medical Association (AMA)
Kaothekar, Sachin& Chhajlani, R. K.. Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma. ISRN Astronomy and Astrophysics. 2012. Vol. 2012, no. 2012, pp.1-14.
https://search.emarefa.net/detail/BIM-470876
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-470876