The No-Boundary Probability for the Universe starting at the top of the hill

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dc.creatorClunan, Tim
dc.date2007-04-16
dc.date.accessioned2026-07-07T07:56:45Z
dc.date.available2026-07-07T07:56:45Z
dc.descriptionWe use the Hartle-Hawking No-Boundary Proposal to make a comparison between the probabilities of the universe starting near, and at, the top of a hill in the effective potential. In the context of top-down cosmology, our calculation finds that the universe doesn't start at the top.
dc.description8 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0704.2042
dc.identifierhttp://arxiv.org/abs/0704.2042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127423
dc.subjectHigh Energy Physics - Theory
dc.titleThe No-Boundary Probability for the Universe starting at the top of the hill
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