Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..114t&link_type=abstract
(Astronomicheskii Zhurnal, vol. 60, Jan.-Feb. 1983, p. 114-121) Soviet Astronomy (ISSN 0038-5301), vol. 27, Jan.-Feb. 1983, p. 6
Astronomy and Astrophysics
Astronomy
Gravitational Waves, Pulsars, Radiation Distribution, Rotating Fluids, Stellar Radiation, Gravitational Wave Antennas, Newtonian Fluids, Radiant Flux Density, Relativity, Spin
Scientific paper
The angular distribution and total intensity of gravitational wave emission is calculated for a rapidly rotating drop of a homogeneous gravitating liquid which has an asymmetric form due to magnetic strains. General relativity effects are taken into account in the post-Newtonian approximation. Two frequencies ω and 2ω are shown to be present in the spectrum. The possibility of registration of monochromatic gravitational wave emission from pulsars by resonance gravitational antennae and the possibility to obtain in such a way information on their internal structure is discussed. The influence of gravitational wave emission on the pulsar evolution is estimated.
Tsvetkov Pavel V.
Tsyrulev A. N.
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