Summary
A nonlinear stability analysis of a uniformly rotating gas in a gravitational field has been performed. One dimensional non-linear equations have been solved by the double-Lagrangian transformation method. An explosive instability is shown to exist in contrast to the linear Jeans instability wherein a uniform rotation of the gas quenches the instability.
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References
Jeans, J. H., 1902, Phillosophical. Trans., 199, 1.
Chandrasekhar, S., 1961, Hydrodynamics and Hydromagnetic Stability, (Oxford Univ. Press) p-588.
Kolb, E. W., & Turner, M. S. 1990, The Early Universe, (Addision-Wesley Publishing Co.).
Krishan, V., 1999, Astrophysical Plasmas and fluids(Kluwer Academic Publisher) p-270
Monte-Lima, I. & Ortega, V. G. 2004, New Astronomy, 9, 365.
Griv, E., Gedalim, M. & Yuan, C. 2002, Astronomy and Astrophysics, 383, 338.
Dawson, J. M. 1959, Physical Review, 113, 383.
Davidson, R. C. & Schram, P. P. 1968, Nuclear Fusion, 8, 183.
Infeld, E. & Rowlands, G. 1987, Phys. Rev. Letters, 58, 2063.
Davidson, R. C. 1972, Methods in Nonlinear Plasma Theory, (Academic, New York).
Pipes, L. A., & Harvill, L. R. 1971, Applied mathematics for Engineers and Physicists, p-560.
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Chakrabarti, N., Pal, B., Krishan, V. (2009). Nonlinear Jeans Instability in an Uniformly Rotating Gas. In: Hasan, S.S., Gangadhara, R.T., Krishan, V. (eds) Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-8868-1_19
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DOI: https://doi.org/10.1007/978-1-4020-8868-1_19
Publisher Name: Springer, Dordrecht
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Online ISBN: 978-1-4020-8868-1
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