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dc.contributor.authorMukohyama, Shinjien
dc.contributor.alternative向山, 信治ja
dc.date.accessioned2015-01-29T06:21:42Z-
dc.date.available2015-01-29T06:21:42Z-
dc.date.issued2014-12-01-
dc.identifier.issn1475-7516-
dc.identifier.urihttp://hdl.handle.net/2433/193282-
dc.description.abstractWe present a new quasidilaton theory of Poincare invariant massive gravity, based on the recently proposed framework of matter coupling that makes it possible for the kinetic energy of the quasidilaton scalar to couple to both physical and fiducial metrics simultaneously. We find a scaling-type exact solution that expresses a self-accelerating de Sitter universe, and then analyze linear perturbations around it. It is shown that in a range of parameters all physical degrees of freedom have non-vanishing quadratic kinetic terms and are stable in the subhorizon limit, while the effective Newton's constant for the background is kept positive.en
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherIOP Publishingen
dc.rightsArticle funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License.en
dc.subjectgravityen
dc.subjectmodified gravityen
dc.titleA new quasidilaton theory of massive gravityen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.ncidAA11940422-
dc.identifier.jtitleJournal of Cosmology and Astroparticle Physicsen
dc.identifier.volume2014-
dc.identifier.issue12-
dc.relation.doi10.1088/1475-7516/2014/12/011-
dc.textversionpublisher-
dc.identifier.artnum011-
dcterms.accessRightsopen access-
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