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Path-integral derivation of black-hole radiance
Abstract
The Feynman path-integral method is applied to the quantum mechanics of a scalar particle moving in the background geometry of a Schwarzschild black hole. The amplitude for the black hole to emit a scalar particle in a particular mode is expressed as a sum over paths connecting the future singularity and infinity. By analytic continuation in the complexified Schwarzschild space this amplitude is related to that for a particle to propagate from the past singularity to infinity and hence by time reversal to the amplitude for the black hole to absorb a particle in the same mode. The form of the connection between the emission and absorption probabilities shows that a Schwarzschild black hole will emit scalar particles with a thermal spectrum characterized by a temperature which is related to its mass, $M$, by $T=\frac{\ensuremath{\hbar}{c}^{3}}{8\ensuremath{\pi}}\mathrm{GMk}$. Thereby a conceptually simple derivation of black-hole radiance is obtained. The extension of this result to other spin fields and other black-hole geometries is discussed.
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Citations
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Metadata
- Authors
- Hartle, J. B., & Hawking, S. W.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1976-04-15
- Volume
- 13
- Issue
- 8
- Pages
- 2188-2203
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2131856183
- Cited by
- 1,115
- References
- 2
- FWCI
- 10.93
- Type
- journal article
- Language
- en
- Open access
- closed
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