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dc.date.accessioned2017-08-15T12:57:31Z
dc.date.available2017-08-15T12:57:31Z
dc.date.created2013-08-29T15:33:26Z
dc.date.issued2013
dc.identifier.citationBiswas, T. Brandenberger, R. Koivisto, Tomi Sebastian Mazumdar, A. . Cosmological perturbations from statistical thermal fluctuations. Physical Review D. Particles and fields. 2013, 88(2)
dc.identifier.urihttp://hdl.handle.net/10852/57043
dc.description.abstractCosmological perturbations due to statistical thermal fluctuations in a single fluid characterized by an arbitrary equation of state are computed. Formulas to predict the scalar and tensor perturbation spectra and non-Gaussianity parameters at a given temperature are derived. These results are relevant to cosmological scenarios, such as cyclic or emergent universes, where cosmic structures may have been seeded thermally instead of originating purely from quantum vacuum fluctuations. © 2013 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleCosmological perturbations from statistical thermal fluctuationsen_US
dc.typeJournal articleen_US
dc.creator.authorBiswas, T.
dc.creator.authorBrandenberger, R.
dc.creator.authorKoivisto, Tomi Sebastian
dc.creator.authorMazumdar, A.
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin1045777
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review D. Particles and fields&rft.volume=88&rft.spage=&rft.date=2013
dc.identifier.jtitlePhysical Review D. Particles and fields
dc.identifier.volume88
dc.identifier.issue2
dc.identifier.pagecount10
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevD.88.023517
dc.identifier.urnURN:NBN:no-59775
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2821
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57043/2/PhysRevD.88.023517.pdf
dc.type.versionPublishedVersion
cristin.articleid023517


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