The relativistic corrections to gravitational radiation from rapidly rotating magnetized neutron stars

Details The relativistic corrections to gravitational radiation from rapidly rotating magnetized neutron stars The relativistic corrections to gravitational radiation from rapidly rotating magnetized neutron stars

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1117t&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 1117-1120. In Russian.

Statistics

Computation

Gravitational Waves, Magnetic Stars, Neutron Stars, Relativistic Effects, Stellar Models, Stellar Rotation, Computational Astrophysics, Error Analysis

Scientific paper

A method for calculating relativistic corrections to the total intensity
of gravitational radiation from rapidly rotating neutron stars in the
model of an oblique rotator is developed. The concrete values of these
corrections are calculated and their analysis for various parameters of
neutron stars is made.

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