The tunneling hamiltonian representation of false vacuum decay: III. Application to nucleation of an inflationary universe

dc.creatorBeckwith, A. W.
dc.date2004-06-24
dc.date2004-07-12
dc.date.accessioned2026-07-07T04:31:17Z
dc.date.available2026-07-07T04:31:17Z
dc.descriptionThe tunneling hamiltonian has proven to be a useful method in many body physics to treat particle tunneling between different states represented as wave functions. Here we apply a generalization of a way we formed appropriate wave functionals in CDW to how to present nucleation of an inflationary universe . This allows us to make a generalization of the model used for inflation when the inflaton is trapped in a false vacuum and, after tunneling, makes a first order phase transition to initiate nucleation of an inflationary universe, in which tunneling between states which are wavefunctionals of a scalar quantum field are considered . We explain how we can have particle - anti particle pairs as a model for how nucleation occurs and construct a potential which satisfies the flat slow roll condition even while using a modified false vacuum construction to this problem
dc.description23 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/math-ph/0406054
dc.identifierhttp://arxiv.org/abs/math-ph/0406054
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/57758
dc.subjectMathematical Physics
dc.subject46N50;85A40
dc.titleThe tunneling hamiltonian representation of false vacuum decay: III. Application to nucleation of an inflationary universe
dc.typetext

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