Classical versus quantum completeness
arXiv:1504.05580 · doi:10.1103/PhysRevD.91.125028
Abstract
The notion of quantum-mechanical completeness is adapted to situations where the only adequate description is in terms of quantum field theory in curved space-times. It is then shown that Schwarzschild black holes, although geodesically incomplete, are quantum complete.
5 pages
References in corpus (5)
Cited by in corpus (20)
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