Breuer, R. A. ; Ruffini, R. ; Tiomno, J. ; Vishveshwara, C. V.
(1973)
*Vector and tensor radiation from Schwarzschild relativistic circular geodesics*
Physical Review D - Particles, Fields, Gravitation and Cosmology, 7
(4).
pp. 1002-1007.
ISSN 1550-7998

Full text not available from this repository.

Official URL: http://prd.aps.org/abstract/PRD/v7/i4/p1002_1

Related URL: http://dx.doi.org/10.1103/PhysRevD.7.1002

## Abstract

For the case of high multipoles we give an analytic form of the spectrum of gravitational and electromagnetic radiation produced by a particle in a highly relativistic orbit r_{0}=(3+δ)M around a Schwarzschild black hole of mass M. The general dependence of the power spectrum on the frequency in all three spin cases (s=0 for scalar, s=1 for vector, and s=2 for tensor fields) are summarized by power P∝ ω^{1−s}exp(−2ω/ω_{crit}). Although they have the common feature of an exponential cutoff above a certain frequency ω_{crit}=(4/πδ)ω_{0}, where ω_{ 0} is the frequency of the orbit, the tensor case has a much broader frequency spectrum than scalar or vector radiation.

Item Type: | Article |
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Source: | Copyright of this article belongs to The American Physical Society. |

ID Code: | 58658 |

Deposited On: | 02 Sep 2011 03:52 |

Last Modified: | 02 Sep 2011 03:52 |

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