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Hawking radiation and Hawking flux from spherical reduction

W. Kummer, D. V. Vassilevich

gr-qcarXiv:gr-qc/0009051

Abstract

Using heat kernel techniques we show that the relation between Hawking temperature and radiation flux known from Einstein gravity in D dimensions can be reproduced from the spherically reduced action. A recent controversy regarding the D=2 anomaly for that case is discussed. The generalized effective Polyakov action in the presence of a dilaton field is presented.

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