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Hawking radiation of extended objects

Abstract:
We compute the effects on the temperature and precise spectrum of Hawking radiation from a Schwarzschild black hole when the emitted object is taken to be spatially extended. We find that in the low-momentum regime, the power emitted is exponentially suppressed for sufficiently large radiated objects, or sufficiently small black holes, though the temperature of emission is unchanged. We numerically determine the magnitude of this suppression as a function of the size and mass of the object and the black hole, and discuss the implications for various extended objects in nature.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1007/jhep04(2020)205

Authors


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Institution:
University of Oxford
Role:
Author
More by this author
Institution:
University of Oxford
Role:
Author


Publisher:
Springer
Journal:
Journal of High Energy Physics More from this journal
Volume:
2020
Issue:
4
Article number:
205
Publication date:
2020-04-30
Acceptance date:
2020-04-14
DOI:
EISSN:
1029-8479
ISSN:
1126-6708


Language:
English
Keywords:
Source identifiers:
2592298
Deposit date:
2025-01-14
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