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Feynman Green function inside a Schwarzschild black hole.

Abstract:
A representation is given for the Feynman Green function corresponding to a scalar field that propagates in Schwarzschild spacetime and which is subject to the Hartle-Hawking boundary conditions. This representation is valid for all values of the Schwarzschild radial coordinate r and is used to obtain an expression for cphi2reg for the region interior to the horizon. This expression is evaluated numerically for the range 0.5M
Publication status:
Published

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Publisher copy:
10.1103/physrevd.33.1596

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Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author
Journal:
Physical review D: Particles and fields
Volume:
33
Issue:
6
Pages:
1596-1603
Publication date:
1986-03-01
DOI:
ISSN:
0556-2821
Language:
English
Pubs id:
pubs:9821
UUID:
uuid:67778501-826c-41e8-8ffb-05a62cf5554c
Local pid:
pubs:9821
Source identifiers:
9821
Deposit date:
2012-12-19

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