Anisotropic gravitational instability

Details Anisotropic gravitational instability Anisotropic gravitational instability

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988zhetf..94....1p&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 94, May 1988, p. 1-14. In Russian.

Physics

4

Anisotropic Media, Gravitational Collapse, Rotating Matter, Stellar Systems, Jeans Theory, Rotating Cylinders

Scientific paper

The paper presents exact solutions to problems of the stability of two anisotropic gravitating systems of different geometry: a finite-thickness quiescent layer and a finite-radius rotating cyinder. In both cases, the anisotropic gravitational instability which arises is of the Jeans type and is oscillatory in nature. It is found that, in a gravitating layer, this instability is due to the build-up of exchange-Jeans modes.

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