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.
- Received 22 April 2015
DOI:https://doi.org/10.1103/PhysRevD.91.125028
© 2015 American Physical Society
