Numerical simulations of electroweak baryogenesis at preheating

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dc.creatorRajantie, A.
dc.creatorSaffin, P. M.
dc.creatorCopeland, E. J.
dc.date2000-10-31
dc.date.accessioned2026-07-07T03:43:06Z
dc.date.available2026-07-07T03:43:06Z
dc.descriptionIt has recently been suggested that the baryon washout problem of standard electroweak baryogenesis could be avoided if inflation ends at a low enough energy density and a parametric resonance transfers its energy repidly into the standard model fields. We present preliminary results of numerical simulations in a SU(2)xU(1) gauge-Higgs model in which this process was studied.
dc.description8 pages, 1 figure. Talk given by A. Rajantie at COSMO 2000, Cheju, Korea, 4-8 September, 2000
dc.identifierhttps://arxiv.org/abs/hep-ph/0010347
dc.identifierhttp://arxiv.org/abs/hep-ph/0010347
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40103
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNumerical simulations of electroweak baryogenesis at preheating
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