Computing the spectrum of black hole radiation in the presence of high frequency dispersion: an analytical approach

Steven Corley

doi:10.1103/PhysRevD.57.6280

paper

Computing the spectrum of black hole radiation in the presence of high frequency dispersion: an analytical approach

arXiv:hep-th/9710075 · doi:10.1103/PhysRevD.57.6280

Abstract

We present a method for computing the spectrum of black hole radiation of a scalar field satisfying a wave equation with high frequency dispersion. The method involves a combination of Laplace transform and WKB techniques for finding approximate solutions to ordinary differential equations. The modified wave equation is obtained by adding a higher order derivative term suppressed by powers of a fundamental momentum scale $k_{0}$ to the ordinary wave equation. Depending on the sign of this new term, high frequency modes propagate either superluminally or subluminally. We show that the resulting spectrum of created particles is thermal at the Hawking temperature, and further that the out-state is a thermal state at the Hawking temperature, to leading order in $k_{0}$ , for either modification.

26 pages, plain latex, 6 figures included using psfig

Computing the spectrum of black hole radiation in the presence of high frequency dispersion: an analytical approach

Abstract

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