Penrose Model potential, compared with Coleman-Weinberg Potential for early universe scalar evolution

dc.creatorBeckwith, A. W.
dc.date2007-09-04
dc.date.accessioned2026-07-07T11:19:04Z
dc.date.available2026-07-07T11:19:04Z
dc.descriptionWe present an overview of Dr. Penrose's model of a cyclic universe, minus the big crunch which relies upon black hole collection of matter after an a long term expansion phase from an initial big bang . We affirm that the suggested evolution equation presented at his lecture for his model meets requirements as to an emergent quintessence field from a vacuum state . We try to offer suggestions as to how to investigate his controversial conformal mapping of matter/energy via Hawkings radiation from a potentially infinite number of black holes to a new big bang. This is his 'ripples in a pond' effect which we find highly unusual but worth serious study and investigation.
dc.description9 pages, 0 figures. In response to Dr. Penrose presenting his cyclic universe model, minus the big crunch presentation at the IGC inagural converence at Penn state, summer 2007
dc.identifierhttps://arxiv.org/abs/0709.0330
dc.identifierhttp://arxiv.org/abs/0709.0330
dc.identifierElectron.J.Theor.Phys.5N17:95-106,2008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193558
dc.subjectGeneral Physics
dc.titlePenrose Model potential, compared with Coleman-Weinberg Potential for early universe scalar evolution
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