The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Classical and quantum gravity of brane black holes
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.
Integrity signals
Registry
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.
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?
There are several examples of higher-dimensional static braneworld black holes, both analytically and numerically constructed.
“In fact, there are several examples of higher-dimensional static braneworld black holes, both analytically and numerically constructed [67][68][69][70][71][72][201][202][203][204][205][206][207][208].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [202]
The boundary CFT stress-tensor can be computed in full using holographic renormalization methods, leading to ⟨T ij ⟩ = - 3ħN 2 32π 2 l 4 4 g ij .
“To see this, consider the boundary CFT stress-tensor, which can be computed in full using holographic renormalization methods, leading to [202]”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [202]
The stability structure remains the same with branes included.
“The stability structure remains the same with branes included [202].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [202]
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
Anti-de Sitter space, thermal phase transition, and confinement in gauge theories
Witten, E. (1998) · Advances in Theoretical and Mathematical Physics · doi:10.4310/atmp.1998.v2.n3.a3 · Cited by 3,915
Flagged first, then by citations
Research works printed but not linked: 29
- S. W. Hawking, Commun. Math. Phys. 43, 199 (1975)
- L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690 (1999), hep-th/9906064. · arXiv
- J. M. Maldacena, Adv. Theor. Math. Phys. 2, 231 (1998), hep-th/9711200. · arXiv
- S. S. Gubser, Phys. Rev. D 63, 084017 (2001), hep-th/9912001. · arXiv
- M. J. Duff and J. T. Liu, Phys. Rev. Lett. 85, 2052 (2000), hep-th/0003237. · arXiv
- M. J. Duff, J. T. Liu and H. Sati, Phys. Rev. D 69, 085012 (2004), hep-th/0207003. · arXiv
- T. Tanaka, Prog. Theor. Phys. Suppl. 148 (2003) 307-316, gr-qc/0203082. · arXiv
- R. Emparan, A. Fabbri, and N. Kaloper, JHEP 08 (2002) 043, hep-th/0206155. · arXiv
- A. L. Fitzpatrick, L. Randall, and T. Wiseman, JHEP 11 (2006) 033, hep-th/0608208. · arXiv
- P. Binetruy, C. Deffayet and D. Langlois, Nucl. Phys. B 565, 269 (2000), hep-th/9905012. · arXiv
- N. Kaloper, Phys. Rev. D 60, 123506 (1999), hep-th/9905210. · arXiv
- P. Bowcock, C. Charmousis and R. Gregory, Class. Quant. Grav. 17, 4745 (2000), hep-th/0007177. · arXiv
- A. Chamblin, S. W. Hawking, and H. S. Reall, Phys. Rev. D61 (2000) 065007, hep-th/9909205. · arXiv
- R. Gregory, Class. Quant. Grav. 17, L125 (2000), hep-th/0004101. · arXiv
- A. Fabbri and G. P. Procopio, Class. Quant. Grav. 24, 5371 (2007), 0704.3728 [hep-th].
- C. Charmousis and R. Gregory, Class. Quant. Grav. 21, 527 (2004), gr-qc/0306069. · arXiv
- R. Emparan, J. Garcia-Bellido, and N. Kaloper, JHEP 01 (2003) 079, hep-th/0212132. · arXiv
- H. Kudoh, T. Tanaka, and T. Nakamura, Phys. Rev. D68 (2003) 024035, gr-qc/0301089. · arXiv
- H. Kudoh, Phys. Rev. D69 (2004) 104019, hep-th/0401229. · arXiv
- A. Karch and L. Randall, JHEP 05 (2001) 008, hep-th/0011156. · arXiv
- A. Chamblin and A. Karch, Phys. Rev. D 72, 066011 (2005), arXiv:hep-th/0412017 · arXiv
- T. Hirayama and G. Kang, Phys. Rev. D 64 (2001) 064010, hep-th/0104213. · arXiv
- N. Seiberg and E. Witten, JHEP 04 (1999) 017, hep-th/9903224. · arXiv
- E. Witten and S.-T. Yau, Adv. Theor. Math. Phys. 3 (1999) 1635-1655, hep-th/9910245. · arXiv
- V. Balasubramanian and P. Kraus, Commun. Math. Phys. 208 (1999) 413-428, hep-th/9902121. · arXiv
- M. Henningson and K. Skenderis, JHEP 07 (1998) 023, hep-th/9806087. · arXiv
- S. de Haro, S. N. Solodukhin, and K. Skenderis, Commun. Math. Phys. 217 (2001) 595-622, hep-th/0002230. · arXiv
- E. Witten, Adv. Theor. Math. Phys. 2, 505 (1998) [arXiv:hep-th/9803131]. · arXiv
- S. Hemming and L. Thorlacius, arXiv:0709.3738[hep-th]. · arXiv
Cited by
Sorted by citations
Three-Dimensional Quantum Black Holes: A Primer
Panella, E., Pedraza, J. F., & Svesko, A. (2024) · Universe · doi:10.3390/universe10090358 · Cited by 24
Metadata
- Authors
- Gregory, R., Ross, S. F., & Zegers, R.
- Venue
- Journal of High Energy Physics
- Published
- 2008-09-05
- Volume
- 2008
- Issue
- 09
- Pages
- 029-029
- ISSN
- 1029-8479
- Cited by
- 39
- References
- 1
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
