Bogoliubov Coefficients of 2D Charged Black Holes

Details Bogoliubov Coefficients of 2D Charged Black Holes Bogoliubov Coefficients of 2D Charged Black Holes

2000-10-12

arxiv.org/abs/hep-th/0010097v1

Phys.Lett.B501:269-276,2001

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, 1 eps figure

Scientific paper

10.1016/S0370-2693(01)00118-6

We exactly calculate the thermal distribution and temperature of Hawking radiation for a two-dimensional charged dilatonic black hole after it has settled down to an "equilibrium" state. The calculation is carried out using the Bogoliubov coefficients. The background of the process is furnished by a preexisting black hole and not by collapsing matter as considered by Giddings and Nelson for the case of a Schwarzschild black hole. Furthermore, the vanishing of the temperature and/or the Hawking radiation in the extremal case is obtained as a regular limit of the general case.

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