Backreaction of linear perturbations and dark energy

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dc.contributor.author Räsänen, Syksy
dc.date.accessioned 2020-01-23T11:43:01Z
dc.date.available 2020-01-23T11:43:01Z
dc.date.issued 2004-08-17
dc.identifier.citation Räsänen , S 2004 ' Backreaction of linear perturbations and dark energy ' arXiv . < https://arxiv.org/abs/astro-ph/0407317 >
dc.identifier.other PURE: 130559908
dc.identifier.other PURE UUID: 72a474cb-29f5-46b3-9cf8-03269c103c33
dc.identifier.other ORCID: /0000-0003-2296-302X/work/68615178
dc.identifier.uri http://hdl.handle.net/10138/310237
dc.description.abstract A simple discussion on the backreaction of inhomogeneities in cosmology, focusing on the possibility that it could explain the present acceleration and solve the coincidence problem. en
dc.format.extent 4
dc.language.iso eng
dc.rights other
dc.rights.uri info:eu-repo/semantics/openAccess
dc.subject 114 Physical sciences
dc.title Backreaction of linear perturbations and dark energy en
dc.type Working paper
dc.contributor.organization Department of Physics
dc.rights.accesslevel openAccess
dc.type.version publishedVersion
dc.identifier.url https://arxiv.org/abs/astro-ph/0407317

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