Towards black hole scattering
Open accessAbstract
We study black holes in three-dimensional Chern–Simons gravity with a negative cosmological constant. In particular, we identify how the Chern–Simons interactions between a scattering particle and a black hole project the particle wavefunction onto a wavefunction in the black hole background. We also analyze the set of spacetimes that should be allowed in the theory and the way in which boundary conditions affect the spectrum of spacetimes.
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
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?
In Chern-Simons scattering computations, imposing invariance under the mapping class group is necessary to recover the correct classical limit.
“In each case, it is only when one imposes invariance under the mapping class group that one recovers the correct classical limit.”
From Quantum Gravity in 2 + 1 Dimensions: The Case of a Closed Universe (2005) · cites this paper as [259]
In “Scattering off a black hole” (page unavailable), the paper says that the braiding projection makes a probe wave-function periodic and reconstructs its semiclassical form on a BTZ black-hole background. This supports the role of projection in that scattering calculation, but our copy does not establish the broader claim that mapping-class-group invariance is necessary in each case to recover the correct classical limit. (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.
Cites
No references could be resolved yet.
Research works printed but not linked: 13
- M. Banados, C. Teitelboim, J. Zanelli, Phys. Rev. Lett. 69 (1992) 1849, hep-th/9204099. · arXiv
- M. Banados, M. Henneaux, C. Teitelboim, J. Zanelli, Phys. Rev. D 48 (1993) 1506, gr-qc/9302012. · arXiv
- O. Coussaert, M. Henneaux, hep-th/9407181. · arXiv
- M. Vergne, Representations of Lie groups and the Orbit method, in: Emmy Noether in Bryn Mawr, Proceedings of a Symposium, Springer-Verlag, New York, 1983.
- O. Coussaert, M. Henneaux, P. van Driel, Class. Quantum Grav. 12 (1995) 2961, gr-qc/9506019. · arXiv
- M. Natsuume, Y. Satoh, Int. J. Mod. Phys. A 13 (1998) 1229, hep-th/9611041. · arXiv
- D. Birmingham, I. Sachs, S. Sen, Int. J. Mod. Phys. D 10 (2001) 833, hep-th/0102155. · arXiv
- S.M. Carroll, E. Farhi, A.H. Guth, hep-th/9207037. · arXiv
- J. Khoury, B.A. Ovrut, N. Seiberg, P.J. Steinhardt, N. Turok, Phys. Rev. D 65 (2002) 086007, hep-th/0108187. · arXiv
- P. Kraus, H. Ooguri, S. Shenker, Phys. Rev. D 67 (2003) 124022, hep-th/0212277. · arXiv
- J. Teschner, Nucl. Phys. B 546 (1999) 390, hep-th/9712256. · arXiv
- A. Giveon, D. Kutasov, N. Seiberg, Adv. Theor. Math. Phys. 2 (1998) 733, hep-th/9806194. · arXiv
- J. Theor. Phys. 38 (1999) 1113, hep-th/9711200. · arXiv
Cited by
Sorted by citations
Quantum Gravity in 2 + 1 Dimensions: The Case of a Closed Universe
Carlip, S. (2005) · Living Reviews in Relativity · doi:10.12942/lrr-2005-1 · Cited by 172 · see citing works
- Authors
- Troost, J., & Tsuchiya, A.
- Affiliations
- Massachusetts Institute of Technology (US)
- Corresponding author
- Tsuchiya, Asato
- ORCID
- Tsuchiya, Asato
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 2003-11
- Volume
- 574
- Issue
- 3-4
- Pages
- 301-308
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2090588494
- Cited by
- 2
- References
- 0
- FWCI
- 0.16
- Type
- journal article
- Language
- en
- Open access
- hybrid
- doi.org
- Licence
- Locations
- Physics Letters B (publishedVersion, cc-by)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion)
- arXiv (Cornell University)
- Funders
- U.S. Department of Energy (FC02-94ER40818, DE-FC02-94 ER40818)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Keywords
- black hole scattering, Chern-Simons gravity, three-dimensional gravity, negative cosmological constant, black holes, boundary conditions
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