Dilatonic current-carrying cosmic strings

Detalhes bibliográficos
Autor(a) principal: Peter, Patrick
Data de Publicação: 2003
Outros Autores: Guimarães, M. E.X. [UNESP], Andrade, V. C. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.67.123509
http://hdl.handle.net/11449/224343
Resumo: We investigate the nature of ordinary cosmic vortices in some scalar-tensor extensions of gravity. We find solutions for which the dilaton field condenses inside the vortex core. These solutions can be interpreted as raising the degeneracy between the eigenvalues of the effective stress-energy tensor, namely, the energy per unit length U and the tension T, by picking a privileged spacelike or timelike coordinate direction; in the latter case, a phase frequency threshold occurs that is similar to what is found in ordinary neutral current-carrying cosmic strings. We find that the dilaton contribution for the equation of state, once averaged along the string worldsheet, vanishes, leading to an effective Nambu-Goto behavior of such a string network in cosmology, i.e.on very large scales. It is found also that on small scales, the energy per unit length and tension depend on the string internal coordinates in such a way as to permit the existence of centrifugally supported equilibrium configuration, also known as vortons, whose stability, depending on the very short distance (unknown) physics, can lead to catastrophic consequences on the evolution of the Universe. © 2003 The American Physical Society.
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spelling Dilatonic current-carrying cosmic stringsWe investigate the nature of ordinary cosmic vortices in some scalar-tensor extensions of gravity. We find solutions for which the dilaton field condenses inside the vortex core. These solutions can be interpreted as raising the degeneracy between the eigenvalues of the effective stress-energy tensor, namely, the energy per unit length U and the tension T, by picking a privileged spacelike or timelike coordinate direction; in the latter case, a phase frequency threshold occurs that is similar to what is found in ordinary neutral current-carrying cosmic strings. We find that the dilaton contribution for the equation of state, once averaged along the string worldsheet, vanishes, leading to an effective Nambu-Goto behavior of such a string network in cosmology, i.e.on very large scales. It is found also that on small scales, the energy per unit length and tension depend on the string internal coordinates in such a way as to permit the existence of centrifugally supported equilibrium configuration, also known as vortons, whose stability, depending on the very short distance (unknown) physics, can lead to catastrophic consequences on the evolution of the Universe. © 2003 The American Physical Society.Institut d’Astrophysique de Paris GReCO FRE 2435-CNRS, 98bis boulevard Arago, Paris, 75014Instituto de Física Teórica Universidade Estadual Paulista, 01405-900Instituto de Física Teórica Universidade Estadual Paulista, 01405-900FRE 2435-CNRSUniversidade Estadual Paulista (UNESP)Peter, PatrickGuimarães, M. E.X. [UNESP]Andrade, V. C. [UNESP]2022-04-28T19:56:00Z2022-04-28T19:56:00Z2003-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.67.123509Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 12, 2003.1550-23681550-7998http://hdl.handle.net/11449/22434310.1103/PhysRevD.67.1235092-s2.0-0041627473Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T19:56:00Zoai:repositorio.unesp.br:11449/224343Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T19:56Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Dilatonic current-carrying cosmic strings
title Dilatonic current-carrying cosmic strings
spellingShingle Dilatonic current-carrying cosmic strings
Peter, Patrick
title_short Dilatonic current-carrying cosmic strings
title_full Dilatonic current-carrying cosmic strings
title_fullStr Dilatonic current-carrying cosmic strings
title_full_unstemmed Dilatonic current-carrying cosmic strings
title_sort Dilatonic current-carrying cosmic strings
author Peter, Patrick
author_facet Peter, Patrick
Guimarães, M. E.X. [UNESP]
Andrade, V. C. [UNESP]
author_role author
author2 Guimarães, M. E.X. [UNESP]
Andrade, V. C. [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv FRE 2435-CNRS
Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Peter, Patrick
Guimarães, M. E.X. [UNESP]
Andrade, V. C. [UNESP]
description We investigate the nature of ordinary cosmic vortices in some scalar-tensor extensions of gravity. We find solutions for which the dilaton field condenses inside the vortex core. These solutions can be interpreted as raising the degeneracy between the eigenvalues of the effective stress-energy tensor, namely, the energy per unit length U and the tension T, by picking a privileged spacelike or timelike coordinate direction; in the latter case, a phase frequency threshold occurs that is similar to what is found in ordinary neutral current-carrying cosmic strings. We find that the dilaton contribution for the equation of state, once averaged along the string worldsheet, vanishes, leading to an effective Nambu-Goto behavior of such a string network in cosmology, i.e.on very large scales. It is found also that on small scales, the energy per unit length and tension depend on the string internal coordinates in such a way as to permit the existence of centrifugally supported equilibrium configuration, also known as vortons, whose stability, depending on the very short distance (unknown) physics, can lead to catastrophic consequences on the evolution of the Universe. © 2003 The American Physical Society.
publishDate 2003
dc.date.none.fl_str_mv 2003-01-01
2022-04-28T19:56:00Z
2022-04-28T19:56:00Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.67.123509
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 12, 2003.
1550-2368
1550-7998
http://hdl.handle.net/11449/224343
10.1103/PhysRevD.67.123509
2-s2.0-0041627473
url http://dx.doi.org/10.1103/PhysRevD.67.123509
http://hdl.handle.net/11449/224343
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 12, 2003.
1550-2368
1550-7998
10.1103/PhysRevD.67.123509
2-s2.0-0041627473
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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