Hawking radiation in GHS blackhole, Effective action and Covariant Boundary condition

Details Hawking radiation in GHS blackhole, Effective action and Covariant Boundary condition Hawking radiation in GHS blackhole, Effective action and Covariant Boundary condition

2007-12-19

arxiv.org/abs/0712.3095v2

Phys.Rev.D77:064027,2008

Physics

High Energy Physics

High Energy Physics - Theory

5 pages Latex file, minor modifications, some additional material added

Scientific paper

10.1103/PhysRevD.77.064027

We exploit the expression for the anomalous (chiral) effective action to obtain the Hawking radiation from the GHS (stringy) blackhole falling in the class of the most general spherically symmetric blackholes $(\sqrt{-g}\neq1)$, using only covariant boundary condition at the event horizon. The connection between the anomalous and the normal energy-momentum tensors is also established from the effective action approach.

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