CoChat
Sign Up
Cited by 673

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

Internal structure of black holes

Poisson, Eric, Israel, Werner·1990·Physical Review D
DOI 10.1103/physrevd.41.1796
Open this paper in CoChat — free account

Abstract

The gravitational effects associated with the radiative tail produced by a gravitational collapse with rotation are investigated. It is shown that the infinite blueshift of the tail's energy density occurring at the Cauchy horizon of the resulting black hole causes a classically unbounded inflation of the effective internal gravitational-mass parameter of the hole. Since this effect is causally disconnected from any external observer, the black-hole external mass remains bounded. The mass inflation phenomenon causes the spacetime curvature to grow to Planckian scales on a spacelike hypersurface in the vicinity of the Cauchy horizon, beyond which the classical laws of general relativity break down. A consequence is that an observer's trip to this hypersurface embraces all but the last Planck time of the entire black-hole classical history.

Overview

Integrity signals

Registry

Crossref · 10.1103/physrevd.41.1796

Cites

2 of 2 references verified0 citation errors · 0 not checkable

Statistics

Recomputing p-values needs the paper’s full text.

Verification

Claims the paper makes

This paper’s full text isn’t openly available, so its claims and self-check weren’t run. The registry and citation checks still apply.

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • The infinitely blue-shifted energy of a particle entering from the exterior of the black hole should result in a large backreaction so as to turn the smooth inner Cauchy horizon into a non-smooth barrier.

    “Conceivably, however, the infinitely blue-shifted energy of a particle entering from the exterior of the black hole should result in a large backreaction so as to turn the smooth (regular) inner Cauchy horizon into a non-smooth barrier [294,295].”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [295]

Citations

Cites

Flagged first, then by citations

Research works printed but not linked: 38

  1. R. Penrose, 1978, Theoretical Principles in Astrophysics and General Relativity
  2. W. Israel, 1986, Can. J. Phys., 64, 120, 10.1139/p86-018 · DOI
  3. R. H. Price, 1972, Phys. Rev. D, 5, 2419, 10.1103/PhysRevD.5.2419 · DOI
  4. R. H. Price, 1972, Phys. Rev. D, 5, 2439, 10.1103/PhysRevD.5.2439 · DOI
  5. A. G. Doroshkevich, 1978, Zh. Eksp. Teor. Fiz., 74, 3
  6. E. Poisson, 1988, Class. Quantum Grav., 5, L201, 10.1088/0264-9381/5/12/002 · DOI
  7. J. M. McNamara, 1978, Proc. R. Soc. London, A358, 449
  8. J. M. McNamara, 1978, Proc. R. Soc. London, A364, 121, 10.1098/rspa.1978.0191 · DOI
  9. Y. Gürsel, 1979, Phys. Rev. D, 19, 413, 10.1103/PhysRevD.19.413 · DOI
  10. R. A. Matzner, 1979, Phys. Rev. D, 19, 2821, 10.1103/PhysRevD.19.2821 · DOI
  11. S. Chandrasekhar, 1982, Proc. R. Soc. London, A284, 301, 10.1098/rspa.1982.0160 · DOI
  12. N. Zamorano, 1982, Phys. Rev. D, 26, 2564, 10.1103/PhysRevD.26.2564 · DOI
  13. E. Poisson, 1989, Phys. Rev. Lett., 63, 1663, 10.1103/PhysRevLett.63.1663 · DOI
  14. E. Poisson, 1989, Phys. Lett. B, 233, 74, 10.1016/0370-2693(89)90618-7 · DOI
  15. R. A. Isaacson, 1968, Phys. Rev., 160, 1263, 10.1103/PhysRev.166.1263 · DOI
  16. R. A. Isaacson, 1968, Phys. Rev., 160, 1272, 10.1103/PhysRev.166.1272 · DOI
  17. M. A. Markov, 1982, Pis'ma Zh. Eksp. Teor. Fiz., 36, 214
  18. M. R. Bernstein, 1984, Bull. Am. Phys. Soc., 16, 1016
  19. V. Frolov, 1989, Phys. Lett. B, 216, 272, 10.1016/0370-2693(89)91114-3 · DOI · Paper page
  20. V. Frolov, 1990, Phys. Rev. D, 41, 383, 10.1103/PhysRevD.41.383 · DOI · Paper page
  21. V. A. Berezin, 1987, Phys. Rev. D, 36, 2919, 10.1103/PhysRevD.36.2919 · DOI · Paper page
  22. W. B. Bonnor, 1970, Gen. Relativ. Gravit., 1, 127, 10.1007/BF00756891 · DOI
  23. B. T. Sullivan, 1980, Phys. Lett., 79A, 371, 10.1016/0375-9601(80)90266-2 · DOI
  24. I. H. Redmount, 1985, Prog. Theor. Phys., 73, 1401, 10.1143/PTP.73.1401 · DOI
  25. T. Dray, 1985, Commun. Math. Phys., 99, 613, 10.1007/BF01215912 · DOI
  26. S. K. Blau, 1989, Phys. Rev. D, 39, 2901, 10.1103/PhysRevD.39.2901 · DOI
  27. D. M. Eardley, 1974, Phys. Rev. Lett., 33, 442, 10.1103/PhysRevLett.33.442 · DOI
  28. Y. Nambu, 1988, Prog. Theor. Phys., 79, 96, 10.1143/PTP.79.96 · DOI
  29. V. A. Belinskii, 1972, Zh. Eksp. Teor. Fiz., 63, 1121
  30. R. Laflamme, 1987, Phys. Rev. D, 35, 2315, 10.1103/PhysRevD.35.2315 · DOI
  31. J. A. Wheeler, 1977, Gen. Relativ. Gravit., 8, 713, 10.1007/BF00756325 · DOI
  32. J. Madore, 1985, Phys. Lett., 111A, 283, 10.1016/0375-9601(85)90627-9 · DOI
  33. B. Zumino, 1986, Phys. Rep., 109, 109, 10.1016/0370-1573(86)90076-1 · DOI
  34. H. Ishihara, 1986, Phys. Lett. B, 179, 217, 10.1016/0370-2693(86)90569-1 · DOI
  35. K. Maeda, 1987, Phys. Lett. B, 186, 151, 10.1016/0370-2693(87)90508-9 · DOI
  36. R. Penrose, 1979, General Relativity: An Einstein Centenary Survey
  37. C. W. Misner, 1973, Gravitation
  38. B. Waugh, 1986, Phys. Rev. D, 34, 2978, 10.1103/PhysRevD.34.2978 · DOI

Cited by

Sorted by citations

Metadata

Authors
Poisson, E., & Israel, W.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
1990-03-15
Volume
41
Issue
6
Pages
1796-1809
ISSN
0556-2821
DOI
10.1103/physrevd.41.1796
Cited by
673
References
2
Language
en
Licence
link.aps.org/licenses/aps-default-license (vor)

About these checks

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.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review