Analytical approximation of < phi**2 > for a massive scalar field in static spherically symmetric space-times - INSPIRE

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Analytical approximation of < phi**2 > for a massive scalar field in static spherically symmetric space-times

Sergey V. Sushkov
(
- Kazan State Pedagogical Inst.
)

Jan, 2000

13 pages

Published in:

Phys.Rev.D 62 (2000) 064007

e-Print:

gr-qc/0001058 [gr-qc]

DOI:

10.1103/PhysRevD.62.064007

Report number:

KGPU-99-01

View in:

ADS Abstract Service

reference search12 citations

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Abstract: (arXiv)

An analitical approximation of

<\phi^2>

for a massive scalar field in a zero temperature vacuum state in static spherically symmetric spacetimes is obtained. The calculations are based on the method for computing vacuum expectations values for scalar fields in general static spherically symmetric spacetimes derived by Anderson, Hiscock and Samuel [Phys. Rev. D {\bf 51}, 4337 (1995)]. The analitical approximation is used to compute

<\phi^2>

in Schwarzschild and wormhole spacetimes.

field theory: scalar
massive
space-time: static
symmetry: rotation
analytic properties
WKB approximation
renormalization
vacuum polarization
space-time: Schwarzschild
wormhole

References(19)

Figures(0)

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