Physics
Scientific paper
Jul 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55..265c&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 55, July 15, 1985, p. 265-268. Research supported by the University of Victoria.
Physics
14
Energy Dissipation, Gravitational Waves, Relativity, Two Body Problem, Binary Stars, Equations Of State, Gravitational Wave Antennas, Pulsars
Scientific paper
Field contributions and Gauss's theorem for retarded functions lead to a new formula for gravitational-radiation energy loss. It clarifies the applicability of the quadrupole formula for systems with T super ik-dominated motion. Applied to the axially symmetric two-body problem with equation of state epsion = epsilon (e) for short free-fall times, the new formula yields the bulk-motion quadrupole-formula results. This contrasts an earlier larger flux with unconventional equation of state and that of critics claming a quadrupole-formula flux from internal motions. An order-of-magnitude estimate yields potential corrections of quadrupole-formula size after about 100 yr for the binary pulsar.
Cooperstock Fred
Lim Paul H.
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