Cosmic Growth and Expansion Conjoined

dc.contributor.authorLinder, Eric V.
dc.date.accessioned2017-08-24T10:51:13Z
dc.date.available2017-08-24T10:51:13Z
dc.date.issued2016-10-17
dc.description.abstractCosmological measurements of both the expansion history and growth history have matured, and the two together provide an important test of general relativity. We consider their joint evolutionary track, showing that this has advantages in distinguishing cosmologies relative to considering them individually or at isolated redshifts. In particular, the joint comparison relaxes the shape degeneracy that makes f 8(z) curves difficult to separate from the overall growth amplitude. The conjoined method further helps visualization of which combinations of redshift ranges provide the clearest discrimination. We examine standard dark energy cosmologies, modified gravity, and “stuttering” growth, each showing distinct signatures.ru_RU
dc.identifier.citationLinder, Eric V. (2016) Cosmic Growth and Expansion Conjoined. International conference "ECL17: Exploring the Energetic Universe 2017", Nazarbayev University Energetic Cosmic Laboratoryru_RU
dc.identifier.urihttp://arxiv.org/abs/1610.05321v1
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/2549
dc.language.isoenru_RU
dc.publisherInternational conference "ECL17: Exploring the Energetic Universe 2017", Nazarbayev University Energetic Cosmic Laboratoryru_RU
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectcosmologyru_RU
dc.subjectdark energyru_RU
dc.subjectcosmic growthru_RU
dc.subjectgravityru_RU
dc.subjectResearch Subject Categories::NATURAL SCIENCES::Physics::Astronomy and astrophysics::Cosmology
dc.titleCosmic Growth and Expansion Conjoinedru_RU
dc.typeArticleru_RU

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