Topological Defects and Inflation

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dc.creatorLazarides, G.
dc.creatorShafi, Q.
dc.date1995-10-11
dc.date.accessioned2026-07-07T11:35:12Z
dc.date.available2026-07-07T11:35:12Z
dc.descriptionIn the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We find that magnetic monopoles of mass on the order of $10^{13}\ GeV$ can survive inflation and be present in our galaxy at an observable level. We also consider cosmic strings as well as domain walls.
dc.description11 pages, LaTEX
dc.identifierhttps://arxiv.org/abs/hep-ph/9510275
dc.identifierhttp://arxiv.org/abs/hep-ph/9510275
dc.identifierPhys.Lett.B372:20-24,1996
dc.identifierdoi:10.1016/0370-2693(96)00136-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198511
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTopological Defects and Inflation
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