arXiv · hep-th/0201162
Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry
Abstract
We present a complete relativistic analysis for the scalar radiation emitted by a particle in circular orbit around a Schwarzschild-anti-de Sitter black hole. If the black hole is large, then the radiation is concentrated in narrow angles- high multipolar distribution- i.e., the radiation is synchrotronic. However, small black holes exhibit a totally different behavior: in the small black hole regime, the radiation is concentrated in low multipoles. There is a transition mass at $M=0.427 R$, where $R$ is the AdS radius. This behavior is new, it is not present in asymptotically flat spacetimes.
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Vitor Cardoso, Jose' P. S. Lemos. 2002-05-18. Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry. https://doi.org/10.1103/physrevd.65.104033
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