paper

Regular Black Holes and Topology Change

arXiv:gr-qc/9612057 · doi:10.1103/PhysRevD.55.7615

Abstract

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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