Vector and Tensor Radiation from Schwarzschild Relativistic Circular Geodesics

Details Vector and Tensor Radiation from Schwarzschild Relativistic Circular Geodesics Vector and Tensor Radiation from Schwarzschild Relativistic Circular Geodesics

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvd...7.1002b&link_type=abstract

Physical Review D, vol. 7, Issue 4, pp. 1002-1007

Physics

18

Scientific paper

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 r0=(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~ω1-sexp(-2ωωcrit). Although they have the common feature of an exponential cutoff above a certain frequency ωcrit=(4πδ)ω0, where ω0 is the frequency of the orbit, the tensor case has a much broader frequency spectrum than scalar or vector radiation.

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