Expansion of True Vacuum Bubbles at the End of Inflation

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dc.creatorRubin, S. G.
dc.date1999-08-04
dc.date2000-07-07
dc.date.accessioned2026-07-07T04:07:45Z
dc.date.available2026-07-07T04:07:45Z
dc.descriptionThe dynamics of false vacuum decay at the end of inflation is studied. It is shown that the creation of a new phase is mainly stimulated by temperature fluctuations. Moving walls of O(3)-symmetric bubbles weakly interact with their surroundings at the inflation stage. Large field fluctuations might arise as a result of wall collisions.
dc.description8p, corrected references
dc.identifierhttps://arxiv.org/abs/hep-ph/9908239
dc.identifierhttp://arxiv.org/abs/hep-ph/9908239
dc.identifierGrav.Cosmol. 5 (1999) 127
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/49262
dc.subjectHigh Energy Physics - Phenomenology
dc.titleExpansion of True Vacuum Bubbles at the End of Inflation
dc.typetext

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