Is the CMB shift parameter connected with the growth of cosmological perturbations?

dc.contributor.authorBasilakos, S.en
dc.contributor.authorNesseris, S.en
dc.contributor.authorPerivolaropoulos, L.en
dc.date.accessioned2015-11-24T18:26:40Z
dc.date.available2015-11-24T18:26:40Z
dc.identifier.issn0035-8711-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/15923
dc.rightsDefault Licence-
dc.subjectcosmic microwave backgrounden
dc.subjectlarge-scale structure of universeen
dc.subjectdark energyen
dc.subjectlambdaen
dc.subjectcomponenten
dc.subjectuniverseen
dc.subjectmodelsen
dc.subjectmatteren
dc.titleIs the CMB shift parameter connected with the growth of cosmological perturbations?en
heal.abstractWe verify numerically that in the context of general relativity (GR), flat models which have the same Omega(m) and cosmic microwave background (CMB) shift parameter R but different H(a) and w(a) also have very similar (within less than 8 per cent) growth of perturbations even though the dark energy density evolution is quite different. This provides a direct connection between geometrical and dynamical tests of dark energy and may be used as a cosmological test of GR.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.primaryDOI 10.1111/j.1365-2966.2008.13303.x-
heal.identifier.secondary<Go to ISI>://000256732700015-
heal.identifier.secondaryhttp://onlinelibrary.wiley.com/store/10.1111/j.1365-2966.2008.13303.x/asset/j.1365-2966.2008.13303.x.pdf?v=1&t=h0xqy3ky&s=d4db6361e654ff96c46d4f62cba72dbf1582cedb-
heal.journalNameMonthly Notices of the Royal Astronomical Societyen
heal.journalTypepeer reviewed-
heal.languageen-
heal.publicationDate2008-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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