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Scalar waves from a star orbiting a BTZ black hole

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arxiv 1512.05108 v3 pith:TEQS5UN7 submitted 2015-12-16 hep-th gr-qc

classification hep-thgr-qc
keywords blackcorrespondingdecayorbitingratesscalarstarwaves
verification ladder T0 review T1 audit T2 compute T3 formal
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In this paper we compute the decay rates of massless scalar waves excited by a star circularly orbiting around the non-extremal (general) and extremal BTZ black holes. These decay rates are compared with the corresponding quantities computed in the corresponding dual conformal field theories respectively. We find that matches are achieved in both cases.

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