Detectable gravitational radiation from stellar collapse

Details Detectable gravitational radiation from stellar collapse Detectable gravitational radiation from stellar collapse

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phrvl..39.1429e&link_type=abstract

Physical Review Letters, vol. 39, Dec. 5, 1977, p. 1429-1432.

Astronomy and Astrophysics

Astrophysics

11

Gravitational Collapse, Gravitational Waves, Radiation Sources, Stellar Evolution, Main Sequence Stars, Stellar Models, Stellar Rotation, Stellar Structure

Scientific paper

The problem of astrophysical sources of detectable gravitational radiation is considered from the stellar-evolution viewpoint. Calculations are presented which indicate that the final stages of evolution may well be dominated by rapidly rotating, collapsing cores which develop nonaxisymmetric configurations. Such events emit large amounts of gravitational radiation which should be detectable in the near future.

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