Cited by 59Black Holes and Theoretical PhysicsRelativity and Gravitational TheoryCosmology and Gravitation Theories

The DOI matches its Crossref record.

Cosmic p-branes

Open access
Gregory, Ruth·1996·Nuclear Physics B

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1016/0550-3213(96)00089-2

Cites

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

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 theory has black brane solutions with the necessary properties.

    “The theory does have black brane solutions with the necessary properties [14,15].”

    From Transdimensional tunneling in the multiverse (2010) · cites this paper as [15]

    Section 5 (General Charged Branes; page unavailable) gives metrics for charged p-branes and describes the solutions as boost-symmetric, supporting the existence of brane solutions. But the claim does not specify the “necessary properties”; the paper also says its solutions suffer from singularities and leaves their stability unresolved. Our copy therefore cannot establish that they have all the properties the citing authors require. (LLM, conf=0.78)

    Experimental — accuracy not yet measured
  • Using results of [15] and [14], it can be shown that (46) is the only solution which is both non-singular and boost-invariant.

    “Using the results of Refs.[15] and [14], it can be shown that ( 46) is the only solution which is both non-singular and boost-invariant.”

    From Transdimensional tunneling in the multiverse (2010) · cites this paper as [15]

    Section 5, “General Charged Branes” (page unavailable), identifies boost-symmetric solutions, but does not establish that any particular solution is uniquely both boost-invariant and non-singular. The Discussion (page unavailable) says the exact solutions generically have naked singularities at the brane core and proposes that a defect core might smooth them out. The cited paper therefore supports the boost-symmetry aspect, not the claimed non-singularity or uniqueness of equation (46). (LLM, conf=0.82)

    Experimental — accuracy not yet measured
  • Einstein-Maxwell theory with Λ6=0 has magnetically charged, asymptotically flat black brane solutions.

    “It is well known that Einstein-Maxwell theory with Λ 6 = 0 has magnetically charged, asymptotically flat black brane solutions [14,15].”

    From Transdimensional tunneling in the multiverse (2010) · cites this paper as [15]

    Section 4 (page unavailable) imposes asymptotically Minkowskian boundary conditions, and Section 5 derives magnetically charged p-brane solutions with unrestricted dilaton coupling. But Section 6 says the paper’s solutions have a singularity at r+ rather than inside an event horizon, so they do not establish the claimed black-brane solutions. The cited passages also do not state the Λ6=0 condition explicitly. (LLM, conf=0.84)

    Experimental — accuracy not yet measured

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cites

No references could be resolved yet.

Research works printed but not linked: 32

  1. Gibbons, 1988, Nucl. Phys. B, 298, 741, 10.1016/0550-3213(88)90006-5 · DOI
  2. Horowitz, 1991, Nucl. Phys. B, 360, 197, 10.1016/0550-3213(91)90440-9 · DOI
  3. Gregory, 1993, Phys. Rev. Lett., 70, 2837, 10.1103/PhysRevLett.70.2837 · DOI · Paper page
  4. Gregory, 1994, Nucl. Phys. B, 428, 399, 10.1016/0550-3213(94)90206-2 · DOI · Paper page
  5. Gregory, 1995, Phys. Rev. D, 51, 305, 10.1103/PhysRevD.51.R305 · DOI
  6. Hindmarsh, 1995, Rep. Prog. Phys., 58, 477, 10.1088/0034-4885/58/5/001 · DOI
  7. R.H. Brandenberger, Modern cosmology and structure formation, astro-ph/9412049. · arXiv
  8. Hawking, 1995, Phys. Rev. Lett., 75, 3382, 10.1103/PhysRevLett.75.3382 · DOI
  9. Emparan, 1995, Phys. Rev. Lett., 75, 3386, 10.1103/PhysRevLett.75.3386 · DOI
  10. Eardley, 1995, Phys. Rev. Lett., 75, 3390, 10.1103/PhysRevLett.75.3390 · DOI
  11. Gregory, 1995, Phys. Rev. D, 52, 5598, 10.1103/PhysRevD.52.5598 · DOI
  12. Bogomolnyi, 1976, Yad. Fz., 24, 861
  13. Bogomolnyi, 1976, Sov. J. Nucl. Phys., 24, 449
  14. Kinnersley, 1970, Phys. Rev. D, 2, 1359, 10.1103/PhysRevD.2.1359 · DOI
  15. Garfinkle, 1985, Phys. Rev. D, 32, 1323, 10.1103/PhysRevD.32.1323 · DOI
  16. Gregory, 1987, Phys. Rev. Lett., 59, 740, 10.1103/PhysRevLett.59.740 · DOI
  17. Skyrme, 1961, 260, 127
  18. Bizon, 1992, Phys. Lett. B, 297, 55, 10.1016/0370-2693(92)91069-L · DOI
  19. Brans, 1961, Phys. Rev., 124, 925, 10.1103/PhysRev.124.925 · DOI · Paper page
  20. Brans, 1962, Phys. Rev., 125, 2194, 10.1103/PhysRev.125.2194 · DOI
  21. S. Kalyana-Rama, Singularities in low energy D = 4 heterotic string and Brans-Dicke theories, hep-th/9309046. · arXiv
  22. Reasenberg, 1979, Astrophys. J., 234, L219, 10.1086/183144 · DOI
  23. Duff, 1995, Phys. Rep., 259, 213, 10.1016/0370-1573(95)00002-X · DOI
  24. Garfinkle, 1991, Phys. Rev. D, 43, 3140, 10.1103/PhysRevD.43.3140 · DOI
  25. Ortiz, 1992, Phys. Rev. D, 45, 2586, 10.1103/PhysRevD.45.R2586 · DOI
  26. Lee, 1992, Phys. Rev. D, 45, 2751, 10.1103/PhysRevD.45.2751 · DOI
  27. Duff, 1994, Nucl. Phys. B, 416, 301, 10.1016/0550-3213(94)90586-X · DOI
  28. Dabholkar, 1989, Phys. Rev. Lett., 63, 719, 10.1103/PhysRevLett.63.478 · DOI
  29. Tseytlin, 1995, Phys. Lett. B, 363, 223, 10.1016/0370-2693(95)01228-7 · DOI
  30. Martinec, 1995, Class. Quant. Grav., 12, 941, 10.1088/0264-9381/12/4/005 · DOI
  31. Witten, 1982, Nucl. Phys. B, 195, 481, 10.1016/0550-3213(82)90007-4 · DOI · Paper page
  32. F. Dowker, J.P. Gauntlett, G.W. Gibbons and G.T. Horowitz, The decay of magnetic fields in Kaluza-Klein theory, hep-th/9507143. · arXiv

Cited by

Sorted by citations

Metadata

Authors
Gregory, R.
Affiliations
Durham University (GB)
Corresponding author
Gregory, Ruth
Venue
Nuclear Physics B
Publisher
Elsevier BV
Published
1996-05
Volume
467
Issue
1-2
Pages
159-182
ISSN
0550-3213 (ISSN-L)
OpenAlex
W2037498162
Cited by
59
References
0
Citations by year
2026: 1 · 2022: 2 · 2017: 1 · 2016: 1 · 2015: 2 · 2014: 1 · 2013: 1 · 2012: 2
FWCI
0.22
Type
journal article
Language
en
Open access
Locations
  • Nuclear Physics B (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • 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
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords
cosmic strings, p-branes, Einstein-Maxwell-dilaton gravity, boost symmetry, naked singularities, Kaluza-Klein reduction, higher-dimensional spacetime, brane solutions

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