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Cited by 1,485

The DOI matches its Crossref record.

Black holes and the second law

Bekenstein, J. D.·1972·Lettere Al Nuovo Cimento Series 2
DOI 10.1007/bf02757029
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Overview

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Registry

Crossref · 10.1007/bf02757029

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  • The Bekenstein-Hawking entropy-area relation is S = k_B c3 A[H]/(4ħG).

    “This is encapsulated by the Bekenstein-Hawking entropy-area relation,”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [111]

Citations

Cites

No references could be resolved yet.

Research works printed but not linked: 5

  1. For transcendence of the law of baryon conservation seeJ. D. Bekenstein:Phys. Rev. Lett.,28, 452 (1972);Phys. Rev. D,5, 1239 (1972) and to be published. · DOI
  2. D. Christodoulou:Phys. Rev. Lett.,25, 1596 (1970);D. Christodoulou andR. Ruffini:Phys. Rev. D,4, 3552 (1971). · DOI
  3. S. W. Hawking:Phys. Rev. Lett.,26, 1344 (1971);Comm. Math. Phys.,25, 152 (1972). · DOI
  4. J. D. Bekenstein: Ph. D. Thesis, Princeton University (1972) (unpublished).
  5. J. A. Wheeler: a chapter inRelativity, Groups and Topology, cited byB. DeWitt andC. DeWitt (New York, 1965).

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Metadata

Authors
Bekenstein, J. D.
Venue
Lettere Al Nuovo Cimento Series 2
Publisher
Springer Science and Business Media LLC
Published
1972-08
Volume
4
Issue
15
Pages
737-740
ISSN
1827-613X
DOI
10.1007/bf02757029
Cited by
1,485
References
0
Language
en
Licence
www.springer.com/tdm (tdm)

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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

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