Quiescent Cosmology and the Final State of the Universe

dc.contributor.authorHoehn, Philipp
dc.contributor.authorScott, Susan M
dc.date.accessioned2015-12-08T22:38:01Z
dc.date.available2015-12-08T22:38:01Z
dc.date.issued2008
dc.date.updated2015-12-08T10:05:15Z
dc.description.abstractIt has long been a primary objective of cosmology to understand the apparent isotropy in our universe and to provide a mathematical formulation for its evolution. A promising school of thought for its explanation is quiescent cosmology, which already possesses a mathematical framework, namely the definition of an isotropic singularity, but only for the initial state of the universe. A complementary framework is necessary in order to also describe possible final states of the universe. Our new definitions of an anisotropic future endless universe and an anisotropic future singularity, whose structure and properties differ significantly from those of the isotropic singularity, offer a promising realization for this framework. The combination of the three definitions together may then provides the first complete formalization of the quiescent cosmology concept.
dc.identifier.issn1793-6594
dc.identifier.urihttp://hdl.handle.net/1885/35770
dc.publisherWorld Scientific Publishing Company
dc.sourceInternational Journal of Modern Physics D:
dc.subjectKeywords: Cosmological futures; Quiescent cosmology; Weyl curvature hypothesis
dc.titleQuiescent Cosmology and the Final State of the Universe
dc.typeJournal article
local.bibliographicCitation.issue3&4
local.bibliographicCitation.lastpage576
local.bibliographicCitation.startpage571
local.contributor.affiliationHoehn, Philipp, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidHoehn, Philipp, u4282188
local.contributor.authoruidScott, Susan M, u8911327
local.description.notesImported from ARIES
local.identifier.absfor020105 - General Relativity and Gravitational Waves
local.identifier.ariespublicationu4103646xPUB128
local.identifier.citationvolume17
local.identifier.doi10.1142/S0218271808012280
local.identifier.scopusID2-s2.0-43949096938
local.identifier.thomsonID000255610500022
local.type.statusPublished Version

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