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On the quantum structure of a black hole
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“The thermal partition function is given by Z(β) = exp(-I(X)), where I(X) is the euclidean effective action evaluated on X.As a function of β, it is interpreted as the canonical free energy, and determines all thermodynamic functions, including the correct black-hole entropy [17]:”
From Very long time scales and black hole thermal equilibrium (2003) · cites this paper as [17]
In the citing paper
“This special topology guarantees the emergence of a classical contribution to the entropy [17].”
From Very long time scales and black hole thermal equilibrium (2003) · cites this paper as [17]
Citations
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Metadata
- Authors
- 't Hooft, G.
- Venue
- Nuclear Physics B
- Publisher
- Elsevier BV
- Published
- 1985-01
- Volume
- 256
- Pages
- 727-745
- ISSN
- 0550-3213 (ISSN-L)
- OpenAlex
- W2043483422
- Cited by
- 1,311
- References
- 17
- Citations by year
- 2026: 24 · 2025: 48 · 2024: 54 · 2023: 48 · 2022: 33 · 2021: 36 · 2020: 39 · 2019: 31 · 2018: 32 · 2017: 44 · 2016: 56 · 2015: 30 · 2014: 44 · 2013: 43 · 2012: 38
- FWCI
- 4.00
- Type
- journal article
- Language
- en
- Open access
- green
- dspace.library.uu.nl
- Licence
- Locations
- Nuclear Physics B (publishedVersion)
- Utrecht University Repository (Utrecht University) (submittedVersion, other-oa)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Keywords
- black holes, general coordinate invariance, general relativity, quantum gravity, black hole thermodynamics
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