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Cosmological evolution in vector-tensor theories of gravity

dc.contributor.authorLópez Maroto, Antonio
dc.contributor.authorBeltrán Jiménez, José
dc.date.accessioned2023-06-20T03:44:01Z
dc.date.available2023-06-20T03:44:01Z
dc.date.issued2009-09
dc.description© 2009 The American Physical Society. This work has been supported by Ministerio de Ciencia e Innovacion (Spain) Project Nos. FIS 2008-01323 and FPA 2008 00592, UCM-Santander PR34/07-15875, and UCM-BSCH GR58/08910309 and MEC Grant No. BES-200612059.
dc.description.abstractWe present a detailed study of the cosmological evolution in general vector-tensor theories of gravity without potential terms. We consider the evolution of the vector field throughout the expansion history of the Universe and carry out a classification of models according to the behavior of the vector field in each cosmological epoch. We also analyze the case in which the Universe is dominated by the vector field, performing a complete analysis of the system phase map and identifying those attracting solutions which give rise to accelerated expansion. Moreover, we consider the evolution in a universe filled with a pressureless fluid in addition to the vector field and study the existence of attractors in which we can have a transition from matter domination to vector domination with accelerated expansion so that the vector field may play the role of dark energy. We find that the existence of solutions with late-time accelerated expansion is a generic prediction of vector tensor theories and that such solutions typically lead to the presence of future singularities. Finally, limits from local gravity tests are used to get constraints on the value of the vector field at small (Solar System) scales.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (Spain)
dc.description.sponsorshipUCM-Santander
dc.description.sponsorshipUCM-BSCH
dc.description.sponsorshipMEC
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/26505
dc.identifier.doi10.1103/PhysRevD.80.063512
dc.identifier.issn550-7998
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.80.063512
dc.identifier.relatedurlhttp://journals.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44340
dc.issue.number6
dc.journal.titlePhysical Review D
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDFIS 2008-01323
dc.relation.projectIDFPA 2008-00592
dc.relation.projectIDPR34/07-15875
dc.relation.projectIDGR58/08910309
dc.relation.projectIDBES-200612059
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordPreferred-Frame Theories
dc.subject.keywordProbe Wmap Observations
dc.subject.keywordEquation of-State
dc.subject.keywordDark Energy
dc.subject.keywordRelativistic Gravity
dc.subject.keywordConservation Laws
dc.subject.keywordConstraints
dc.subject.keywordSupernovae
dc.subject.keywordInflation
dc.subject.keywordSpace
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleCosmological evolution in vector-tensor theories of gravity
dc.typejournal article
dc.volume.number80
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