The DOI matches its Crossref record.
Supergravity and a Bogomol'nyi bound in three dimensions
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?
In the citing paper
“More precisely, the unbroken supersymmetries are those generated by a parameter of the form L (θ) = e -1 2 iθ 0L ,(7.5) where 0 satisfies the projector condition γ 12 0 = -iγ 5 0 [9,10].”
From Bubbles of nothing and supersymmetric compactifications (2016) · cites this paper as [9]
In the citing paper
“Actually, the resulting configuration is a half-BPS vortex solution that is known to exist in our model [9,10].”
From Bubbles of nothing and supersymmetric compactifications (2016) · cites this paper as [9]
In the citing paper
“It is worth mentioning that the relation (A.7) is precisely the condition which ensures that the locally supersymmetric Abelian-Higgs model admits a critical cosmic string solutions of winding n ∈ Z.”
From Bubbles of nothing and supersymmetric compactifications (2016) · cites this paper as [9]
In the citing paper
“Such solutions have a deficit angle of ∆ = 2π, and thus their background geometry asymptotes to M 3 × S 1 far away from the centre of the string, where supersymmetry is also fully preserved [9,10].”
From Bubbles of nothing and supersymmetric compactifications (2016) · cites this paper as [9]
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: 33
- Belavin, 1975, Phys. Lett. B, 59, 85, 10.1016/0370-2693(75)90163-X · DOI
- Bogomol'nyi, 1976, Sov. J. Nucl. Phys., 24, 449
- de Vega, 1976, Phys. Rev. D, 14, 1100, 10.1103/PhysRevD.14.1100 · DOI
- Salam, 1975, Nucl. Phys. B, 97, 293, 10.1016/0550-3213(75)90036-X · DOI
- Fayet, 1976, Il Nuovo Cimento A, 31, 626, 10.1007/BF02734654 · DOI
- Di Vecchia, 1977, Nucl. Phys. B, 130, 93, 10.1016/0550-3213(77)90394-7 · DOI
- Witten, 1978, Phys. Lett. B, 78, 77, 10.1016/0370-2693(78)90357-X · DOI
- Hlousek, 1992, Nucl. Phys. B, 370, 43, 10.1016/0550-3213(92)90348-F · DOI
- Hlousek, 1993, Nucl. Phys. B, 397, 173, 10.1016/0550-3213(93)90340-U · DOI
- Hlousek, 1992, Phys. Lett. B, 283, 75, 10.1016/0370-2693(92)91430-H · DOI
- Hlousek, 1992, Mod. Phys. Lett. A, 7, 3403, 10.1142/S0217732392002809 · DOI
- Lee, 1990, Phys. Lett. B, 243, 105, 10.1016/0370-2693(90)90964-8 · DOI
- Edelstein, 1994, Phys. Lett. B, 329, 39, 10.1016/0370-2693(94)90514-2 · DOI
- Hull, 1984, Nucl. Phys. B, 239, 541, 10.1016/0550-3213(84)90262-1 · DOI
- Teitelboim, 1977, Phys. Lett. B, 69, 240, 10.1016/0370-2693(77)90653-0 · DOI
- Deser, 1977, Phys. Rev. Lett., 39, 249, 10.1103/PhysRevLett.39.249 · DOI · Paper page
- Grisaru, 1978, Phys. Lett. B, 73, 249, 10.1016/0370-2693(78)90837-7 · DOI
- Witten, 1981, Commun. Math. Phys., 80, 381, 10.1007/BF01208277 · DOI · Paper page
- Nester, 1981, Phys. Lett. A, 83, 241, 10.1016/0375-9601(81)90972-5 · DOI
- Israel, 1981, Phys. Lett. A, 85, 259, 10.1016/0375-9601(81)90951-8 · DOI
- Gibbons, 1982, Phys. Lett. B, 109, 190, 10.1016/0370-2693(82)90751-1 · DOI
- Gibbons, 1983, Nucl. Phys. B, 218, 173, 10.1016/0550-3213(83)90480-7 · DOI
- Freedman, 1984, Nucl. Phys. B, 233, 24, 10.1016/0550-3213(84)90168-8 · DOI
- Kalosh, 1992, Phys. Rev. D, 46, 5278, 10.1103/PhysRevD.46.5278 · DOI
- Gibbons, 1994, Nucl. Phys. B, 416, 850, 10.1016/0550-3213(94)90558-4 · DOI
- Cvetič, 1992, Nucl. Phys. B, 381, 301, 10.1016/0550-3213(92)90649-V · DOI
- Witten, 1995, Int. J. Mod. Phys. A, 10, 1247, 10.1142/S0217751X95000590 · DOI · Paper page
- E. Witten, Strong Coupling and the Cosmological Constant, hep-th/9506101. · arXiv
- Becker, 1995, Phys. Rev. D, 51, 6603, 10.1103/PhysRevD.51.R6603 · DOI · Paper page
- Cremmer, 1979, Nucl. Phys. B, 159, 141, 10.1016/0550-3213(79)90331-6 · DOI
- Scherk, 1979, Phys. Lett. B, 82, 60, 10.1016/0370-2693(79)90425-8 · DOI · Paper page
- Ferrara, 1983, Nucl. Phys.B, 223, 191, 10.1016/0550-3213(83)90101-3 · DOI
- Comtet, 1988, Nucl. Phys. B, 299, 719, 10.1016/0550-3213(88)90370-7 · DOI
Cited by
Bubbles of nothing and supersymmetric compactifications
Blanco-Pillado, J. J., Shlaer, B., Sousa, K., & Urrestilla, J. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/10/002 · Cited by 27
Metadata
- Authors
- Edelstein, J., Núñez, C., & Schaposnik, F. A.
- Venue
- Nuclear Physics B
- Publisher
- Elsevier BV
- Published
- 1996-01
- Volume
- 458
- Issue
- 1-2
- Pages
- 165-188
- ISSN
- 0550-3213
- Cited by
- 35
- References
- 0
- Language
- en
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
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.