How false vacuum synthesis of a universe sets initial conditions which permit the onset of variations of a nucleation rate per Hubble volume per Hubble time

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dc.creatorBeckwith, A. W.
dc.date2004-10-28
dc.date.accessioned2026-07-07T04:31:34Z
dc.date.available2026-07-07T04:31:34Z
dc.descriptionUsing Bogomil'nyi inequality and the vanishing of topological charge at the unset of nucleation of a new universe permits a simpler,more direct insight into how topological defects (kinks and anti kinks) contribute to initial conditions at the onset of inflationary cosmology. Currently, there are few bridges between initial conditions for cosmological inflation and the nucleation of a new universe. This presentation shows how this can be done while still employing Venezianos prescription for forming a link between quanta of length, the magnitude of a dilaton field and forces gravitational and gauge alike.
dc.description15 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/math-ph/0410060
dc.identifierhttp://arxiv.org/abs/math-ph/0410060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/57865
dc.subjectMathematical Physics
dc.subject31C99;85A40
dc.titleHow false vacuum synthesis of a universe sets initial conditions which permit the onset of variations of a nucleation rate per Hubble volume per Hubble time
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