Using fluctuations of Entropy as a starting point for obtaining behavior of scalar fields permitting collapse of thin wall approximation

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dc.creatorBeckwith, A. W.
dc.date2004-12-15
dc.date2004-12-16
dc.date.accessioned2026-07-07T04:31:45Z
dc.date.available2026-07-07T04:31:45Z
dc.descriptionWe have shown that a scalar field can be used, employing Scherrer's k essence cosmological sound calculation, to model how we evolve from a dark matter- dark energy mix to a cosmological constant. Here, we are exploring what initiates the decay of the near perfect thin wall approximation on that scalar field to circumstances permitting a k essence speed-of-sound argument in favor of traditional models of Einstein's cosmological constant as a driving force for inflationary expansion.
dc.description7 pages, no figures: Minor spelling errors (two) fixed abstract & text
dc.identifierhttps://arxiv.org/abs/math-ph/0412053
dc.identifierhttp://arxiv.org/abs/math-ph/0412053
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/57931
dc.subjectMathematical Physics
dc.subject85A40
dc.titleUsing fluctuations of Entropy as a starting point for obtaining behavior of scalar fields permitting collapse of thin wall approximation
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