The structure of cosmic time

dc.creatorSparling, George
dc.date2006-06-29
dc.date.accessioned2026-07-07T07:13:14Z
dc.date.available2026-07-07T07:13:14Z
dc.descriptionFollowing the approach of Julien Lesgourgues [astro-ph/0409426], we analyze the mathematical structure of the time co-ordinate of present day cosmological models, where these models include a cosmological constant term to account for the observed acceleration of the universe: we find that in all cases, except for a set of measure zero in the parameter space, the time is given by an (abelian) integral on a torus; the imaginary period of this integral then gives a natural periodicity in imaginary time for the universe; following Stephen Hawking, this periodicity may be interpreted either as giving a fundamental mass scale for the universe, or (using Planck's constant) a fundamental temperature, or both. The precise structure that emerges suggests that the structure of time can be regarded as an order parameter arising perhaps in a phase transition in the early universe; one might hope that this structure would be predictable in any fundamental theory.
dc.description39 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0606129
dc.identifierhttp://arxiv.org/abs/gr-qc/0606129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/112378
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe structure of cosmic time
dc.typetext

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