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- W4200203002 abstract "We study the scalar radiation emitted by a source orbiting a Schwarzschild--anti--de Sitter black hole in circular geodesics. We obtain the emitted power using quantum field theory in curved spacetimes at tree level with reflective boundary conditions at infinity. We compare our results with the ones obtained in Schwarzschild and Schwarzschild--de Sitter ($mathrm{ensuremath{Lambda}}>0$) spacetimes. In the Schwarzschild--de Sitter spacetime we observe an enhancement of the emitted power associated to the lower multipole modes, when compared with the Schwarzschild case. In contrast, for the Schwarzschild--anti--de Sitter spacetime, the enhancement is rather of the higher multipole modes." @default.
- W4200203002 created "2021-12-31" @default.
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- W4200203002 date "2021-12-29" @default.
- W4200203002 modified "2023-09-27" @default.
- W4200203002 title "Radiation emitted by a source orbiting a Schwarzschild–anti–de Sitter black hole" @default.
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- W4200203002 doi "https://doi.org/10.1103/physrevd.104.124085" @default.
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