Quenched Hawking Radiation and the Black Hole Pair-Creation Rate

Details Quenched Hawking Radiation and the Black Hole Pair-Creation Rate Quenched Hawking Radiation and the Black Hole Pair-Creation Rate

1995-09-19

arxiv.org/abs/gr-qc/9509031v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX, 18 pages, 5 .eps figures (to appear in the proceedings of the Sixth Moscow Quantum Gravity Seminar, June 12-19, 1995)

Scientific paper

The main topic of this talk is the Hawking effect when the black holes in question are undergoing a uniform acceleration. The semiclassical effect of the acceleration is most striking when the Hawking temperature equals the acceleration temperature. Within the usual late-time approximation, the natural black hole vacuum is then equivalent to the asymptotically empty Minkowskian vacuum, and the accelerated black hole becomes semiclassically stable against the familiar thermal evaporation. An important application of this phenomenon is found in the problem of charged black hole pair-creation.

Affiliated with

Also associated with

No associations

Rating

Quenched Hawking Radiation and the Black Hole Pair-Creation Rate does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Quenched Hawking Radiation and the Black Hole Pair-Creation Rate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quenched Hawking Radiation and the Black Hole Pair-Creation Rate will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-308957