Journal article
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
Authors
- Journal:
- Physical review D: Particles and fields More from this journal
- 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
- ARK identifier:
Terms of use
- Copyright date:
- 1986
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