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dc.date.accessioned2017-08-15T13:07:46Z
dc.date.available2017-08-15T13:07:46Z
dc.date.created2012-09-21T15:05:35Z
dc.date.issued2012
dc.identifier.citationHarko, T. Koivisto, Tomi Sebastian Lobo, F. S. N. Olmo, G. J. . Metric-Palatini gravity unifying local constraints and late-time cosmic acceleration. Physical Review D. Particles and fields. 2012, 85(8)
dc.identifier.urihttp://hdl.handle.net/10852/57048
dc.description.abstractWe present a novel approach to modified theories of gravity which consists of adding to the Einstein-Hilbert Lagrangian an f(R) term constructed à la Palatini. Using the respective dynamically equivalent scalar-tensor representation, we show that the theory can pass the Solar System observational constraints even if the scalar field is very light. This implies the existence of a long-range scalar field, which is able to modify the cosmological and galactic dynamics but leaves the Solar System unaffected. We also verify the absence of instabilities in perturbations and provide explicit models which are consistent with local tests and lead to the late-time cosmic acceleration. © 2012 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleMetric-Palatini gravity unifying local constraints and late-time cosmic accelerationen_US
dc.typeJournal articleen_US
dc.creator.authorHarko, T.
dc.creator.authorKoivisto, Tomi Sebastian
dc.creator.authorLobo, F. S. N.
dc.creator.authorOlmo, G. J.
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin945730
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=85&rft.spage=&rft.date=2012
dc.identifier.jtitlePhysical Review D. Particles and fields
dc.identifier.volume85
dc.identifier.issue8
dc.identifier.pagecount5
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevD.85.084016
dc.identifier.urnURN:NBN:no-59791
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2821
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57048/1/PhysRevD.85.084016.pdf
dc.type.versionPublishedVersion


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