Breaking Cosmic Strings without Monopoles

dc.creatorEardley, Douglas
dc.creatorHorowitz, Gary
dc.creatorKastor, David
dc.creatorTraschen, Jennie
dc.date1995-06-20
dc.date1995-06-27
dc.date.accessioned2026-07-07T10:34:52Z
dc.date.available2026-07-07T10:34:52Z
dc.descriptionIt is shown that topologically stable cosmic strings can, in fact, appear to end or to break, even in theories without monopoles. This can occur whenever the spatial topology of the universe is nontrivial. For the case of Abelian-Higgs strings, we describe the gauge and scalar field configurations necessary for a string to end on a black hole. We give a lower bound for the rate at which a cosmic string will break via black hole pair production, using an instanton calculation based on the Euclidean C-metric.
dc.description9 pages, no figures; one statement corrected and references added
dc.identifierhttps://arxiv.org/abs/gr-qc/9506041
dc.identifierhttp://arxiv.org/abs/gr-qc/9506041
dc.identifierPhys.Rev.Lett.75:3390-3393,1995
dc.identifierdoi:10.1103/PhysRevLett.75.3390
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179580
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleBreaking Cosmic Strings without Monopoles
dc.typetext

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