Emission of gravitational waves from roto-vibrational modes of a compressible and homogeneous star

Details Emission of gravitational waves from roto-vibrational modes of a compressible and homogeneous star Emission of gravitational waves from roto-vibrational modes of a compressible and homogeneous star

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..115c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 115-123.

Statistics

Computation

2

Compressibility, Computational Astrophysics, Gravitational Waves, Neutron Stars, Stellar Oscillations, Vibration Mode, Eccentricity, Stellar Rotation, Vibration Damping

Scientific paper

Based on Chandrasekhar's and Lebovitz's treatment of the roto-vibrational modes of a homogeneous compressible star, the energy losses and damping rates of each mode by gravitational radiation are computed as a function of the eccentricity e of the equilibrium configuration. Numerical values are estimated for a neutron star. The limit of low eccentricity is considered, compared and contrasted to existing treatments.

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