Stress-energy of a quantized scalar field in static wormhole spacetimes
arXiv:hep-th/0109166 · doi:10.1103/PhysRevD.64.104005
Abstract
An analytical approximation of for a quantized scalar field in a static spherically symmetric spacetime with a topology is obtained. The gravitational background is assumed slowly varying. The scalar field is assumed to be both massive and massless, with an arbitrary coupling to the scalar curvature and in a zero temperature vacuum state. It is demonstrated that for some values of curvature coupling the stress-energy has the properties needed to support the wormhole geometry.
21 pages, revtex
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- Spherically symmetric wormhole solutions in a general anisotropic matter field
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- Vacuum polarization of a quantized scalar field in the thermal state in a long throat