Cited by 424Noncommutative and Quantum Gravity TheoriesBlack Holes and Theoretical PhysicsRelativity and Gravitational Theory

Black-hole entropy from quantum geometry

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Domagala, Marcin, Lewandowski, Jerzy·2004·Classical and Quantum Gravity

Abstract

Quantum geometry (the modern loop quantum gravity involving graphs and spin-networks instead of the loops) provides microscopic degrees of freedom that account for black-hole entropy. However, the procedure for state counting used in the literature contains an error and the number of the relevant horizon states is underestimated. In our paper a correct method of counting is presented. Our results lead to a revision of the literature of the subject. It turns out that the contribution of spins greater than 1/2 to the entropy is not negligible. Hence, the value of the Barbero–Immirzi parameter involved in the spectra of all the geometric and physical operators in this theory is different than previously derived. Also, the conjectured relation between quantum geometry and the black-hole quasi-normal modes should be understood again.

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Crossref · 10.1088/0264-9381/21/22/014

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  • The coefficient of the logarithmic term in the black hole entropy is fixed to -1/2.

    “and resolve the controversy (summarized in [17]) about the coefficient of the logarithmic term fixing it to -1 2 .”

    From Black-hole entropy in loop quantum gravity (2004) · cites this paper as [17]

    The Introduction and Results (p. 3) says that subleading entropy terms were calculated in an accompanying paper, but the equation giving the result is not decoded in our copy. Searches for the logarithmic term and −1/2 found no readable passage stating its coefficient, so our copy cannot verify the claimed value. (LLM, conf=0.74)

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Research works printed but not linked: 4

  1. [1][1] Thiemann T 2003 Lectures on Loop Quantum Gravity in Quantum Gravity: From Theory to Experimental Search Lecture Notes in Physics Preprint gr-qc0112038 Thiemann T 2004 Modern Canonical Quantum General Relativity (Cambridge: Cambridge University Press) at press gr-qc/0110034 - · arXiv
  2. [3][3] Ashtekar A and Lewandowski J 2004 Background Independent Quantum Gravity: A Status Report Class. Quantum Grav. 21 R1-R100 gr-qc/0404018 - · arXiv
  3. [13][13] Ashtekar A and Krishnan B 2004 Isolated and Dynamical Horizons and Their Applications gr-qc/0407042 Ashtekar A, Beetle C, Dreyer O, Fairhurst S, Krishnan B, Lewandowski J, Wisniewski J 2000 Generic Isolated Horizons and their Applications Phys.Rev.Lett. 85 3564-3567 - · arXiv
  4. [14][14] Domagala M 2004 Kwantowy operator pola powierzchni oraz entropia czarnej dziury Diploma Thesis, Uniwersytet Warszawski, Warsaw, Poland

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Authors
Domagala, M., & Lewandowski, J.
Affiliations
  • University of Warsaw (PL)
  • Pennsylvania State University (US)
Venue
Classical and Quantum Gravity
Published
2004-10-29
Volume
21
Issue
22
Pages
5233-5243
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2067931892
Cited by
424
References
4
Citations by year
2026: 15 · 2025: 42 · 2024: 19 · 2023: 14 · 2022: 15 · 2021: 20 · 2020: 10 · 2019: 8 · 2018: 18 · 2017: 6 · 2016: 18 · 2015: 17 · 2014: 22 · 2013: 13 · 2012: 21
FWCI
17.05
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
Keywords
black hole entropy, loop quantum gravity, spin networks, state counting, Barbero-Immirzi parameter, quantum geometry, black hole quasinormal modes

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