Black Hole Radiation (with and) without Weyl Anomaly

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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13 pages, LaTex. [Typographical error in Eq.(36) was corrected. Comments on the relation between our 2D-gravity results and so

Scientific paper

10.1088/0264-9381/13/5/010

In the semiclassical analysis of black hole radiation in matter-coupled
dilaton gravity, a one-parameter ``$k$"-family of measures for the path
integral quantization of the matter fields is considered. The Weyl anomaly is
proportional to the parameter $k$, but the black hole radiation seen by
minkowskian observers at future null infinity is $k$-independent.

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