Finite size effect in gravitational radiation from very close binary systems

Details Finite size effect in gravitational radiation from very close binary systems Finite size effect in gravitational radiation from very close binary systems

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apl....17..119c&link_type=abstract

Astrophysical Letters, vol. 17, no. 3, 1976, p. 119-121.

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Gravitational Waves, Gravitational Fields, Mass Distribution, Quadrupoles, Tides, X Ray Stars

Scientific paper

The correction to the gravitational radiation from a very close binary
system because of effects of finite size of the components is
calculated. It is shown that this would be zero if there is no departure
from spherical symmetry, small in 'normal' systems but very significant
in systems like a white dwarf orbiting about a massive black hole.

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