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dc.contributor.authorBaker, T.en
dc.contributor.authorPsaltis, D.en
dc.contributor.authorSkordis, C.en
dc.creatorBaker, T.en
dc.creatorPsaltis, D.en
dc.creatorSkordis, C.en
dc.date.accessioned2019-12-02T15:28:42Z
dc.date.available2019-12-02T15:28:42Z
dc.date.issued2015
dc.identifier.issn0004-637X
dc.identifier.urihttp://gnosis.library.ucy.ac.cy/handle/7/58518
dc.description.abstractThe current effort to test general relativity (GR) employs multiple disparate formalisms for different observables, obscuring the relations between laboratory, astrophysical, and cosmological constraints. To remedy this situation, we develop a parameter space for comparing tests of gravity on all scales in the universe. In particular, we present new methods for linking cosmological large-scale structure, the cosmic microwave background, and gravitational waves with classic PPN tests of gravity. Diagrams of this gravitational parameter space reveal a noticeable untested regime. The untested window, which separates small-scale systems from the troubled cosmological regime, could potentially hide the onset of corrections to GR. © 2015. The American Astronomical Society. All rights reserved.en
dc.sourceAstrophysical Journalen
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84925812332&doi=10.1088%2f0004-637X%2f802%2f1%2f63&partnerID=40&md5=b646f2ddd668c10994b0db25b8216b02
dc.subjectdark energyen
dc.subjectgravitationen
dc.titleLinking tests of gravity on all scales: From the strong-field regime to cosmologyen
dc.typeinfo:eu-repo/semantics/article
dc.identifier.doi10.1088/0004-637X/802/1/63
dc.description.volume802
dc.description.issue1
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 :25</p>en
dc.source.abbreviationAstrophys.J.en
dc.contributor.orcidSkordis, C. [0000-0001-5873-4259]
dc.gnosis.orcid0000-0001-5873-4259


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