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dc.contributor.authorFerreira, P. G.en
dc.contributor.authorBaker, T.en
dc.contributor.authorSkordis, C.en
dc.creatorFerreira, P. G.en
dc.creatorBaker, T.en
dc.creatorSkordis, C.en
dc.date.accessioned2019-12-02T15:30:20Z
dc.date.available2019-12-02T15:30:20Z
dc.date.issued2014
dc.identifier.urihttp://gnosis.library.ucy.ac.cy/handle/7/58683
dc.description.abstractMore than half a century after the Chapel Hill meeting of 1957, the landscape of general relativity has been transformed. In relativistic cosmology we are entering an era in which we can seriously consider testing some of the most fundamental assumptions that go into our view of the Universe. We propose that precision tests of gravity on cosmological scales may be feasible with up-and-coming surveys of galaxies. To achieve the most accurate general constraints yet we briefly describe a formalism which is applicable on the largest scales: the parametrized post-Friedmann approach. We sketch out the steps that need to be taken to link realistic, cosmological observables with fundamental properties of general relativity. © 2014, Springer Science+Business Media New York.en
dc.sourceGeneral Relativity and Gravitationen
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85028165298&doi=10.1007%2fs10714-014-1788-x&partnerID=40&md5=86425fcf4d0a7a1c28298118a1f14f28
dc.subjectCosmologyen
dc.subjectGeneral relativityen
dc.subjectAstrophysicsen
dc.titleTesting general relativity with cosmology: a synopsis of the parametrized post-Friedmann approachen
dc.typeinfo:eu-repo/semantics/article
dc.identifier.doi10.1007/s10714-014-1788-x
dc.description.volume46
dc.description.issue9
dc.author.facultyΣχολή Θετικών και Εφαρμοσμένων Επιστημών / Faculty of Pure and Applied Sciences
dc.author.departmentΤμήμα Φυσικής / Department of Physics
dc.type.uhtypeArticleen
dc.description.notes<p>Cited By :3</p>en
dc.source.abbreviationGen.Relativ.Gravit.en
dc.contributor.orcidSkordis, C. [0000-0001-5873-4259]
dc.gnosis.orcid0000-0001-5873-4259


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