Gravitational radiation emitted by N particles in circular orbits

Details Gravitational radiation emitted by N particles in circular orbits Gravitational radiation emitted by N particles in circular orbits

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phla...98..403n&link_type=abstract

Physics Letters A, Volume 98, Issue 8-9, p. 403-406.

Physics

8

Scientific paper

We have computed the gravitational radiation emitted by N particles of equal mass in a circular orbit around a Schwarzschild black hole. It is found that the luminosity decreases sharp with the increase of N due to the phase cancellation effect. The application of the Bekenstein's octopole formula shows the decay time of the orbit of a triple compact star each of mass 1.4 M⊚ with a period of 10 min can be 5.4 x 109 yr.

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