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- W2029256914 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 ${mathcal{r}}_{0}=(3+ensuremath{delta})M$ 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 $Pensuremath{propto}{ensuremath{omega}}^{1ensuremath{-}s}mathrm{exp}(ensuremath{-}frac{2ensuremath{omega}}{{ensuremath{omega}}_{mathrm{crit}}})$. Although they have the common feature of an exponential cutoff above a certain frequency ${ensuremath{omega}}_{mathrm{crit}}=(frac{4}{ensuremath{pi}ensuremath{delta}}){ensuremath{omega}}_{0}$, where ${ensuremath{omega}}_{0}$ is the frequency of the orbit, the tensor case has a much broader frequency spectrum than scalar or vector radiation." @default.
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- W2029256914 date "1973-02-15" @default.
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- W2029256914 title "Vector and Tensor Radiation from Schwarzschild Relativistic Circular Geodesics" @default.
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- W2029256914 doi "https://doi.org/10.1103/physrevd.7.1002" @default.
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