Size Gap for Zero Temperature Black Holes in Semiclassical Gravity

Details Size Gap for Zero Temperature Black Holes in Semiclassical Gravity Size Gap for Zero Temperature Black Holes in Semiclassical Gravity

1998-06-16

arxiv.org/abs/gr-qc/9806069v1

Phys.Rev. D59 (1999) 044007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, ReVTeX, no figures

Scientific paper

10.1103/PhysRevD.59.044007

We show that a gap exists in the allowed sizes of all zero temperature static spherically symmetric black holes in semiclassical gravity when only conformally invariant fields are present. The result holds for both charged and uncharged black holes. By size we mean the proper area of the event horizon. The range of sizes that do not occur depends on the numbers and types of quantized fields that are present. We also derive some general properties that both zero and nonzero temperature black holes have in all classical and semiclassical metric theories of gravity.

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