Gravitational radiation from the collapse and explosion of rapidly rotating, homogeneous, gaseous ellipsoids imbedded in halos

Details Gravitational radiation from the collapse and explosion of rapidly rotating, homogeneous, gaseous ellipsoids imbedded in halos Gravitational radiation from the collapse and explosion of rapidly rotating, homogeneous, gaseous ellipsoids imbedded in halos

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..353b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 119, no. 2, Feb. 1986, p. 353-372. Research supported by Queen's Universit

Statistics

Computation

2

Cosmic Gases, Galactic Evolution, Gravitational Collapse, Gravitational Waves, Stellar Evolution, Angular Velocity, Computational Astrophysics, Ellipsoids, Halos

Scientific paper

The nonlinear motion (collapse/explosion) of a homogeneous, rapidly rotating, gaseous ellipsoid has been studied with the effects of an external gravitational field incorporated. The non-axisymmetric motion has been followed using an efficient numerical code based on certain properties of the potential functions. The gravitational radiation associated with the phenomenon was calculated, and the wave forms studied to extract information on the dynamics of the source. Possible implications of the results for various astrophysical processes are discussed.

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