Mathematics
Scientific paper
Dec 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60.1107t&link_type=abstract
(Astronomicheskii Zhurnal, vol. 60, Nov.-Dec. 1983, p. 1107-1113) Soviet Astronomy (ISSN 0038-5301), vol. 27, Nov.-Dec. 1983, p.
Mathematics
Gravitational Waves, Neutron Stars, Rotating Fluids, Stellar Magnetic Fields, Branching (Mathematics), Galactic Nuclei, Gravitational Wave Antennas, Thermodynamic Equilibrium
Scientific paper
The influence which a magnetic field has on an ellipsoidal figure of equilibrium is studied, taking into account effects which deform the figure nonlinearly. Near the bifurcation point, the magnetic field turns out to be the chief factor controlling the form of an ellipsoidal figure, and thereby the development of a time-variable quadrupole mass moment. Calculations of the total intensity and the spectrum of the gravitational radiation emitted near the bifurcation point show that when a typical neutron star is born, it will release gravitational waves at a power of 10 to the 50th to 10 to the 47th erg/sec for the first 1000 sec. Prospects are good for second-generation gravitational antennas to detect such events in the galactic nucleus.
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