Abstract
We reexamine the two-point function approaches used to study vacuum fluctuation in wedge-shaped regions and conical backgrounds. The appearance of divergent integrals is discussed and circumvented. The issue is considered in the context of a massless scalar field in cosmic string spacetime.
- Received 26 March 1998
DOI:https://doi.org/10.1103/PhysRevD.58.027502
©1998 American Physical Society