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Cited by 102

The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.

Statistical origin of black hole entropy in induced gravity

Frolov, V.P., Fursaev, D.V., Zelnikov, A.I.·1997·Nuclear Physics B
DOI 10.1016/s0550-3213(96)00678-5
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Crossref · 10.1016/s0550-3213(96)00678-5

Cites

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  • In scenarios of gravity induced due to matter loops, the Bekenstein-Hawking entropy is solely due to entanglement due to vacuum fluctuations, where the UV-cutoff dependence can be absorbed in a renormalization of Newton's constant.

    “In particular, in scenarios of gravity induced due to matter loops [221,222], the Bekenstein-Hawking entropy is solely due to entanglement due to vacuum fluctuations [223][224][225], where the UV-cutoff dependence can be absorbed in a renormalization of Newton's constant [130].”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [224]

    Section 4 (Eq. 4.30; page unavailable) says that, in the induced-gravity model studied, Bekenstein–Hawking entropy is not solely a statistical-mechanical entropy: it also requires a horizon term involving scalar-field fluctuations. The authors say that term is not related to counting states and removes divergences. The UV-cutoff renormalization clause is attached to a different citation in the citing sentence. (LLM, conf=0.90)

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  • The null energy condition requires that all asymptotically flat or AdS spacetimes have positive ADM mass.

    “and requires that all asymptotically flat or AdS spacetimes to have positive ADM mass [14,12,13].”

    From The generalized second law implies a quantum singularity theorem (2013) · cites this paper as [14]

    Section 2, “Induced gravity: a simple model,” discusses the induced gravitational and cosmological constants and vacuum black-hole solutions, not a positive-mass requirement. Searches for the null energy condition, asymptotically flat or AdS spacetimes, and positive ADM mass found no passage addressing the claim in our copy. (LLM, conf=0.76)

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  • The GSL and GSL together imply a positive energy theorem.

    “An immediate corollary is that the GSL and GSL together imply a positive energy theorem, by the principles outlined in Ref. [14].”

    From The generalized second law implies a quantum singularity theorem (2013) · cites this paper as [14]

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Citations

Cites

Flagged first, then by citations

Research works printed but not linked: 30

  1. Bekenstein, 1972, Nuov. Cim. Lett., 4, 737, 10.1007/BF02757029 · DOI · Paper page
  2. Bekenstein, 1973, Phys. Rev. D, 7, 2333, 10.1103/PhysRevD.7.2333 · DOI · Paper page
  3. Bekenstein, 1974, Phys. Rev. D, 9, 3292, 10.1103/PhysRevD.9.3292 · DOI · Paper page
  4. Gibbons, 1976, Phys. Rev. D, 15, 2752, 10.1103/PhysRevD.15.2752 · DOI · Paper page
  5. Srednicki, 1993, Phys. Rev. Lett., 71, 666, 10.1103/PhysRevLett.71.666 · DOI · Paper page
  6. Frolov, 1993, Phys. Rev. D, 48, 4545, 10.1103/PhysRevD.48.4545 · DOI · Paper page
  7. Frolov, 1995, Phys. Rev. Lett., 74, 3319, 10.1103/PhysRevLett.74.3319 · DOI
  8. Callan, 1995, Phys. Lett. B, 333, 55, 10.1016/0370-2693(94)91007-3 · DOI · Paper page
  9. Fursaev, 1996, Phys. Lett. B, 365, 51, 10.1016/0370-2693(95)01290-7 · DOI
  10. Demers, 1995, Phys. Rev. D, 52, 2245, 10.1103/PhysRevD.52.2245 · DOI
  11. deAlwis, 1995, Phys. Rev. D, 52, 3529, 10.1103/PhysRevD.52.3529 · DOI
  12. Solodukhin, 1995, Phys. Rev. D, 52, 7046, 10.1103/PhysRevD.52.7046 · DOI
  13. Bytsenko, 1996, Nucl. Phys. B, 458, 267, 10.1016/0550-3213(95)00585-4 · DOI
  14. Kabat, 1995, Nucl. Phys. B, 453, 281, 10.1016/0550-3213(95)00443-V · DOI
  15. Larsen, 1996, Nucl. Phys. B, 458, 49, 10.1016/0550-3213(95)00548-X · DOI
  16. Frolov, 1996, Phys. Rev. D, 54, 2711, 10.1103/PhysRevD.54.2711 · DOI
  17. Mann, 1996, Phys. Rev. D, 54, 3932, 10.1103/PhysRevD.54.3932 · DOI
  18. Cognola, 1996, Phys. Rev. D, 54, 2699, 10.1103/PhysRevD.54.2699 · DOI
  19. Barvinsky, 1996, Nucl. Phys. B, 479, 305, 10.1016/0550-3213(96)00438-5 · DOI
  20. Frolov, 1996, Phys. Lett. B, 382, 220, 10.1016/0370-2693(96)00661-2 · DOI
  21. T. Jacobson, Black Hole Entropy and Induced Gravity, preprint gr-qc/9404039. · arXiv
  22. Sakharov, 1968, Sov. Phys. Doklady, 12, 1040
  23. York, 1986, Phys. Rev. D, 33, 2092, 10.1103/PhysRevD.33.2092 · DOI
  24. Braden, 1990, Phys. Rev. D, 42, 3376, 10.1103/PhysRevD.42.3376 · DOI
  25. Fursaev, 1994, Class. Quantum. Grav., 11, 1431, 10.1088/0264-9381/11/6/008 · DOI
  26. Cognola, 1994, Phys. Rev. D, 49, 1029, 10.1103/PhysRevD.49.1029 · DOI
  27. D.V. Fursaev and G. Miele, Cones, Spins and Heat Kernels, preprint ALBERTA-THY-17-96, hepth/9605153, to appear in Nucl. Phys. B.
  28. Larsen, 1996, Phys. Lett. B, 375, 37, 10.1016/0370-2693(96)00220-1 · DOI
  29. Larsen, 1996, Nucl. Phys. B, 475, 627, 10.1016/0550-3213(96)00318-5 · DOI
  30. Horowitz, 1996, Phys. Lett. B, 383, 151, 10.1016/0370-2693(96)00738-1 · DOI

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Metadata

Authors
Frolov, V. P., Fursaev, D. V., & Zelnikov, A. I.
Venue
Nuclear Physics B
Publisher
Elsevier BV
Published
1997-02
Volume
486
Issue
1-2
Pages
339-352
ISSN
0550-3213
DOI
10.1016/s0550-3213(96)00678-5
Cited by
102
References
4
Language
en
Licence

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