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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4607
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dc.contributor.authorChakrabarti, N-
dc.contributor.authorPal, B-
dc.contributor.authorKrishan, V-
dc.date.accessioned2009-07-01T14:25:47Z-
dc.date.available2009-07-01T14:25:47Z-
dc.date.issued2008-
dc.identifier.citationHasan, S. S., Gangadhara, R. T. and Krishan, V. eds., Turbulence, dynamos, accretion disks, pulsars and collective plasma processes, First Kodai-Trieste workshop on plasma astrophysics held at the Kodaikanal Observatory., Astrophysics and space science proceedings., Kodaikanal., India, 2007., pp. 281 - 289en
dc.identifier.isbn978-1-4020-8867-4-
dc.identifier.urihttp://hdl.handle.net/2248/4607-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractA 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.en
dc.language.isoenen
dc.publisherSpringer Netherlandsen
dc.relation.urihttp://dx.doi.org/10.1007/978-1-4020-8868-1_19en
dc.relation.urihttp://adsabs.harvard.edu/abs/2008tdad.conf..281Cen
dc.rights© Springeren
dc.subjectAstrophysical Turbulenceen
dc.subjectPulsarsen
dc.subjectDynamosen
dc.subjectSolar and Space Plasmasen
dc.titleNonlinear jeans instability in an uniformly rotating gasen
dc.typeArticleen
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