Hide metadata

dc.date.accessioned2017-08-15T12:53:39Z
dc.date.available2017-08-15T12:53:39Z
dc.date.created2013-01-09T09:25:42Z
dc.date.issued2012
dc.identifier.citationKoivisto, Tomi Sebastian Mota, David Zumalacárregui, Miguel . Screening Modifications of Gravity Through Disformally Coupled Fields. Physical Review Letters. 2012, 109(24)
dc.identifier.urihttp://hdl.handle.net/10852/57040
dc.description.abstractIt is shown that extensions to general relativity, which introduce a strongly coupled scalar field, can be viable if the interaction has a nonconformal form. Such disformal coupling depends upon the gradients of the scalar field. Thus, if the field is locally static and smooth, the coupling becomes invisible in the Solar System: this is the disformal screening mechanism. A cosmological model is considered where the disformal coupling triggers the onset of accelerated expansion after a scaling matter era, giving a good fit to a wide range of background observational data. Moreover, the interaction leaves signatures in the formation of large-scale structure that can be used to probe such couplings. © 2012 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleScreening Modifications of Gravity Through Disformally Coupled Fieldsen_US
dc.typeJournal articleen_US
dc.creator.authorKoivisto, Tomi Sebastian
dc.creator.authorMota, David
dc.creator.authorZumalacárregui, Miguel
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin984160
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 Letters&rft.volume=109&rft.spage=&rft.date=2012
dc.identifier.jtitlePhysical Review Letters
dc.identifier.volume109
dc.identifier.issue24
dc.identifier.pagecount5
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevLett.109.241102
dc.identifier.urnURN:NBN:no-59773
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0031-9007
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57040/2/PhysRevLett.109.241102.pdf
dc.type.versionPublishedVersion
cristin.articleid241102


Files in this item

Appears in the following Collection

Hide metadata