Hawking Radiation and Hawking Flux from Spherical Reduction
نویسنده
چکیده
Hawking radiation in D = 4 is regarded as a well-understood quantum theoretical feature of black holes (BH) or of other geometric backgrounds with an event horizon. On the other hand, the dilaton theory emerging after spherical reduction from Einstein gravity (SRG) and generalizations of those theories, only during the last years have been investigated in this connection. If the consideration of spherically reduced actions like
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تاریخ انتشار 2000