Heavy cosmic strings

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dc.creatorDonaire, M.
dc.creatorRajantie, A.
dc.date2005-08-26
dc.date2006-03-29
dc.date.accessioned2026-07-07T06:42:06Z
dc.date.available2026-07-07T06:42:06Z
dc.descriptionWe argue that cosmic strings with high winding numbers generally form in first-order gauge symmetry breaking phase transitions, and we demonstrate this using computer simulations. These strings are heavier than single-winding strings and therefore more easily observable. Their cosmological evolution may also be very different.
dc.description4 pages, updated to match the published version
dc.identifierhttps://arxiv.org/abs/hep-ph/0508272
dc.identifierhttp://arxiv.org/abs/hep-ph/0508272
dc.identifierPhys.Rev. D73 (2006) 063517
dc.identifierdoi:10.1103/PhysRevD.73.063517
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/101914
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Lattice
dc.subjectHigh Energy Physics - Theory
dc.titleHeavy cosmic strings
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