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Cited by 311

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Conserved Energy Flux for the Spherically Symmetric System and the Backreaction Problem in the Black Hole Evaporation

Kodama, H.·1980·Progress of Theoretical Physics
DOI 10.1143/ptp.63.1217
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Abstract

For the spherically symmetric system, we prove the existence o{ a new locally cotEen·ecl flux which can be interpreted to represent the total energy flux of matter and gravitational field. ·with the aid of this conservation law, we study the relation between the behavior of the event horizon and the energy flux across it and look for constraints imposed on the total energy radiated to infinity. Some implications of the results of this study to the backreaction problem in the black hole evaporation are discussed.

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Metadata

Authors
Kodama, H.
Venue
Progress of Theoretical Physics
Publisher
Oxford University Press (OUP)
Published
1980-04-01
Volume
63
Issue
4
Pages
1217-1228
ISSN
  • 0033-068X (ISSN-L)
  • 1347-4081
DOI
10.1143/ptp.63.1217
OpenAlex
W2160245112
Cited by
311
References
0
FWCI
0.63
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Conserved Energy Flux for the Spherically Symmetric System and the Backreaction Problem in the Black Hole Evaporation. https://app.cochat.ai/papers/10.1143/ptp.63.1217
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Kodama, H. (1980). Conserved Energy Flux for the Spherically Symmetric System and the Backreaction Problem in the Black Hole Evaporation. Progress of Theoretical Physics. https://doi.org/10.1143/ptp.63.1217

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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