Semi-local cosmic strings and the cosmological constant problem
- Autores
- Edelstein Glaubach, José Daniel
- Año de publicación
- 1997
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gauge group SU (2)global × U (1)local. The model we consider is known to admit string-like configurations, the so-called semi-local cosmic strings. We show that the stability of these solitonic solutions is provided by supersymmetry through the existence of a lower bound for the energy, even though the manifold of the Higgs vacuum does not contain non-contractible loops. Charged Killing spinors do exist over configurations that saturate the Bogomol'nyi bound, as a consequence of an Aharonov-Bohmlike effect. Nevertheless, there are no physical fermionic zero modes on these backgrounds. The exact vanishing of the cosmological constant does not imply, then, Bose-Fermi degeneracy. This provides a non-trivial example of the recent claim made by Witten on the vanishing of the cosmological constant in three dimensions without unphysical degeneracies.
Facultad de Ciencias Exactas - Materia
-
Física
Ciencias Exactas
Supersymmetry
Gauge group
Cosmic string
Higgs boson
Supergravity - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/122981
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Semi-local cosmic strings and the cosmological constant problemEdelstein Glaubach, José DanielFísicaCiencias ExactasSupersymmetryGauge groupCosmic stringHiggs bosonSupergravityWe study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gauge group SU (2)<sub>global</sub> × U (1)<sub>local</sub>. The model we consider is known to admit string-like configurations, the so-called semi-local cosmic strings. We show that the stability of these solitonic solutions is provided by supersymmetry through the existence of a lower bound for the energy, even though the manifold of the Higgs vacuum does not contain non-contractible loops. Charged Killing spinors do exist over configurations that saturate the Bogomol'nyi bound, as a consequence of an Aharonov-Bohmlike effect. Nevertheless, there are no physical fermionic zero modes on these backgrounds. The exact vanishing of the cosmological constant does not imply, then, Bose-Fermi degeneracy. This provides a non-trivial example of the recent claim made by Witten on the vanishing of the cosmological constant in three dimensions without unphysical degeneracies.Facultad de Ciencias Exactas1997info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf101-106http://sedici.unlp.edu.ar/handle/10915/122981enginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0370269396013858?via%3Dihubinfo:eu-repo/semantics/altIdentifier/issn/0370-2693info:eu-repo/semantics/altIdentifier/arxiv/hep-th/9610163info:eu-repo/semantics/altIdentifier/doi/10.1016/s0370-2693(96)01385-8info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:21:08Zoai:sedici.unlp.edu.ar:10915/122981Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:21:08.835SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Semi-local cosmic strings and the cosmological constant problem |
title |
Semi-local cosmic strings and the cosmological constant problem |
spellingShingle |
Semi-local cosmic strings and the cosmological constant problem Edelstein Glaubach, José Daniel Física Ciencias Exactas Supersymmetry Gauge group Cosmic string Higgs boson Supergravity |
title_short |
Semi-local cosmic strings and the cosmological constant problem |
title_full |
Semi-local cosmic strings and the cosmological constant problem |
title_fullStr |
Semi-local cosmic strings and the cosmological constant problem |
title_full_unstemmed |
Semi-local cosmic strings and the cosmological constant problem |
title_sort |
Semi-local cosmic strings and the cosmological constant problem |
dc.creator.none.fl_str_mv |
Edelstein Glaubach, José Daniel |
author |
Edelstein Glaubach, José Daniel |
author_facet |
Edelstein Glaubach, José Daniel |
author_role |
author |
dc.subject.none.fl_str_mv |
Física Ciencias Exactas Supersymmetry Gauge group Cosmic string Higgs boson Supergravity |
topic |
Física Ciencias Exactas Supersymmetry Gauge group Cosmic string Higgs boson Supergravity |
dc.description.none.fl_txt_mv |
We study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gauge group SU (2)<sub>global</sub> × U (1)<sub>local</sub>. The model we consider is known to admit string-like configurations, the so-called semi-local cosmic strings. We show that the stability of these solitonic solutions is provided by supersymmetry through the existence of a lower bound for the energy, even though the manifold of the Higgs vacuum does not contain non-contractible loops. Charged Killing spinors do exist over configurations that saturate the Bogomol'nyi bound, as a consequence of an Aharonov-Bohmlike effect. Nevertheless, there are no physical fermionic zero modes on these backgrounds. The exact vanishing of the cosmological constant does not imply, then, Bose-Fermi degeneracy. This provides a non-trivial example of the recent claim made by Witten on the vanishing of the cosmological constant in three dimensions without unphysical degeneracies. Facultad de Ciencias Exactas |
description |
We study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gauge group SU (2)<sub>global</sub> × U (1)<sub>local</sub>. The model we consider is known to admit string-like configurations, the so-called semi-local cosmic strings. We show that the stability of these solitonic solutions is provided by supersymmetry through the existence of a lower bound for the energy, even though the manifold of the Higgs vacuum does not contain non-contractible loops. Charged Killing spinors do exist over configurations that saturate the Bogomol'nyi bound, as a consequence of an Aharonov-Bohmlike effect. Nevertheless, there are no physical fermionic zero modes on these backgrounds. The exact vanishing of the cosmological constant does not imply, then, Bose-Fermi degeneracy. This provides a non-trivial example of the recent claim made by Witten on the vanishing of the cosmological constant in three dimensions without unphysical degeneracies. |
publishDate |
1997 |
dc.date.none.fl_str_mv |
1997 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/122981 |
url |
http://sedici.unlp.edu.ar/handle/10915/122981 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0370269396013858?via%3Dihub info:eu-repo/semantics/altIdentifier/issn/0370-2693 info:eu-repo/semantics/altIdentifier/arxiv/hep-th/9610163 info:eu-repo/semantics/altIdentifier/doi/10.1016/s0370-2693(96)01385-8 |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
eu_rights_str_mv |
openAccess |
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http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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application/pdf 101-106 |
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