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• W2168567247 abstract "We analyse the scalar radiation emitted from a source rotating around a Schwarzschild black hole using the framework of quantum field theory at the tree level. We show that for relativistic circular orbits the emitted power is about 20-30% smaller than what would be obtained in Minkowski spacetime. We also show that most of the emitted energy escapes to infinity. Our formalism can readily be adapted to investigate similar processes." @default.
• W2168567247 created "2016-06-24" @default.
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• W2168567247 date "1999-11-30" @default.
• W2168567247 modified "2023-10-18" @default.
• W2168567247 title "Scalar radiation emitted from a source rotating around a black hole" @default.
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• W2168567247 doi "https://doi.org/10.1088/0264-9381/17/1/303" @default.
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