Formation of monopoles and domain walls after brane inflation

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dc.creatorMatsuda, Tomohiro
dc.date2004-06-07
dc.date2004-10-19
dc.date.accessioned2026-07-07T10:49:07Z
dc.date.available2026-07-07T10:49:07Z
dc.descriptionWe study cosmological defect formation after brane inflation. The cosmological defects are corresponding to the branes that have less than three spacial dimensions in the uncompactified spacetime. Contrary to the previous arguments, production of monopoles and domain walls are not always negligible. Monopoles and domain walls are formed by the branes extended between mother branes.
dc.description27pages, 7 figures, many comments, footnotes and reviews are added, to appear in JHEP
dc.identifierhttps://arxiv.org/abs/hep-ph/0406064
dc.identifierhttp://arxiv.org/abs/hep-ph/0406064
dc.identifierJHEP0410:042,2004
dc.identifierdoi:10.1088/1126-6708/2004/10/042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184110
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleFormation of monopoles and domain walls after brane inflation
dc.typetext

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