A method to compute < Phi**2 > in asymptotically flat, static, spherically symmetric space-times - INSPIRE

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A method to compute < Phi**2 > in asymptotically flat, static, spherically symmetric space-times

P.R. Anderson
(
- Montana State U.
)

1990

11 pages

Published in:

Phys.Rev.D 41 (1990) 1152-1162

DOI:

10.1103/PhysRevD.41.1152

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Abstract: (APS)

A method is presented which allows for the computation of 〈φ2〉 for scalar fields at zero and nonzero temperatures in asymptotically flat, static, spherically symmetric spacetimes. If a spacetime has event horizons, the method works in the region exterior to the outermost event horizon. The method is used to compute 〈φ2〉 for massless and massive scalar fields in Reissner-Nordström and extreme Reissner-Nordström spacetimes.

space-time
symmetry: rotation
field theory: scalar
finite temperature
two-point function
renormalization: regularization
partial wave analysis
approximation: semiclassical
numerical calculations

References(27)

Figures(0)

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