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dc.contributor.authorForgács, Péter
dc.contributor.authorLukacs, Arpad Laszlo
dc.date.accessioned2020-08-07T08:02:07Z
dc.date.available2020-08-07T08:02:07Z
dc.date.issued2020-07-06
dc.identifier.citationPhysical Review D 102 : (2020) // Article ID 023009es_ES
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/10810/45908
dc.description.abstract[EN] The stability of “visible” electroweak-type cosmic strings is investigated in an extension of the Standard Model by a minimal dark sector, consisting of a Uð1Þ gauge field, broken spontaneously by a scalar. The visible and dark sectors are coupled through a Higgs-portal and a gauge-kinetic mixing term. It is found that strings whose core is “filled” with a dark scalar condensate exhibit better stability properties than their analogues in the Standard Model, when the electroweak mixing angle is close to θW ¼ π=2. They become unstable as one lets θW approach its physical value. The instability mechanism appears to be a W-boson condensation mechanism found in previous studies on the stability of electroweak strings.es_ES
dc.description.sponsorshipFunded by SCOAP.
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.titleElectroweak strings with dark scalar condensates and their stabilityes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.es_ES
dc.relation.publisherversionhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.023009es_ES
dc.identifier.doi10.1103/PhysRevD.102.023009
dc.departamentoesFísica teórica e historia de la cienciaes_ES
dc.departamentoeuFisika teorikoa eta zientziaren historiaes_ES


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Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.
Except where otherwise noted, this item's license is described as Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.