Constraints on Black Holes in Classical and Semiclassical Theories of Gravity

Details Constraints on Black Holes in Classical and Semiclassical Theories of Gravity Constraints on Black Holes in Classical and Semiclassical Theories of Gravity

1997-07-11

arxiv.org/abs/gr-qc/9707026v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, ReVTeX

Scientific paper

Constraints on the geometry of a static spherically symmetric black hole are obtained by requiring the spacetime curvature to be analytic at the event horizon. For a zero temperature black hole further constraints are obtained by also requiring that the semiclassical trace equation be satisfied when conformally invariant fields are present. It is found that zero temperature black holes whose sizes lie within a certain range do not exist. The range depends on the numbers and types of conformally invariant quantized fields that are present.

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