Regular Black Holes and Topology Change

Details Regular Black Holes and Topology Change Regular Black Holes and Topology Change

1996-12-20

arxiv.org/abs/gr-qc/9612057v1

Phys.Rev. D55 (1997) 7615-7617

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Nine pages. One Figure. The figure will emerge automatically if you print via "dvips"

Scientific paper

10.1103/PhysRevD.55.7615

The conditions are clarified under which regular (i.e., singularity-free)
black holes can exist. It is shown that in a large class of spacetimes that
satisfy the weak energy condition the existence of a regular black hole
requires topology change.

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