The multipolar structure of the gravitational radiation from a rotating body

Details The multipolar structure of the gravitational radiation from a rotating body The multipolar structure of the gravitational radiation from a rotating body

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...3..241z&link_type=abstract

(Acta Astrophysica Sinica, vol. 3, no. 2, 1983, 159-164) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, Sept. 1983

Astronomy and Astrophysics

Astrophysics

Gravitational Waves, Relativity, Rotating Bodies, Pulsars, Quadrupoles, Spherical Harmonics

Scientific paper

The metric coefficients of the retarded field of non-plane gravitational waves from a multipolar source at infinity are determined. These results can be used to obtain the expression for the power of the multipole radiation from a slowly rotating body. Calculations of the quadrupole radiation show that the radiation from a rotating body has a strong directivity. The calculated results for the total power of two pulsars are found to be in good agreement with previous estimates.

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