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Cosmological density perturbations in modified gravity theories

dc.book.titlePhysics and mathematics of gravitation
dc.contributor.authorCruz Dombriz, Álvaro de la
dc.contributor.authorDobado González, Antonio
dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-20T13:39:25Z
dc.date.available2023-06-20T13:39:25Z
dc.date.issued2009
dc.description© American Institute of Physics. Spanish Relativity Conference (31. 2008. Salamanca, España). We would like to thank J. A. R. Cembranos and J. Beltran. This work has been supported by the DGICYT (Spain) under projects FPA 2004-02602 and 2005-02327, CAM/UCM 910309 and by UCM-SantanderPR34/07-15875
dc.description.abstractIn the context of f(R) theories of gravity, we study the cosmological evolution of scalar perturbations by using a completely general procedure. We find that the exact fourth-order differential equation for the matter density perturbations in the longitudinal gauge, reduces to a second-order equation for sub-Hubble modes. This simplification is compared with the standard (quasi-static) equation used in the literature. We show that for general f(R) functions the quasi-static approximation is not justified. However for those f(R) adequately describing the present phase of accelerated expansion and satisfying local gravity tests, it does give a correct description for the evolution of perturbations.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipDGICYT (Spain)
dc.description.sponsorshipUCM-Santander
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/21422
dc.identifier.isbn978-0-7354-0658-2
dc.identifier.issn0094-243X
dc.identifier.officialurlhttp://dx.doi.org/10.1063/1.3141280
dc.identifier.relatedurlhttp://www.aip.org
dc.identifier.relatedurlhttp://arxiv.org/abs/0812.3048
dc.identifier.urihttps://hdl.handle.net/20.500.14352/53241
dc.journal.titlePhysics and Mathematics of Gravitation
dc.language.isoeng
dc.page.final255
dc.page.initial252
dc.publisherAmer Inst Physics
dc.relation.projectIDFPA 2004-02602
dc.relation.projectID2005-02327
dc.relation.projectIDCAM/UCM 910309
dc.relation.projectIDPR34/07-15875
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordCosmology
dc.subject.keywordModified Theories of Gravity
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleCosmological density perturbations in modified gravity theories
dc.typebook part
dcterms.references1. S. Perlmutter et a/.[Supemova Cosmology Project Collaboration], Astrophys. J. 517, 565, (1999). 2. E. J. Copeland, M. Sami and S. Tsujikawa, Int. J. Mod. Phys. D, 15, 1753 (2006). 3. L. Pogosian and A. Silvestri, Phys. Rev. D 77 023503, (2008). 4. D. J. Eisenstein et al. Astrophys. J. 633: 560-574, (2005). 5. D. N. Spergel et al. [WMAP Collaboration], Astrophys. J. Suppl. 170 377, (2007). 6. E. Linder Phys.Rev D 72 : 043529, (2005). 7. A. de la Cruz-Dombriz, A. Dobado and A. L. Maroto, Phys. Rev D 77 123515 (2008). 8. S. M. Carroll et al.. New J. Phys. 8 323, (2006) ; P Zhang, Phys. Rev. D 73 123504, (2006). 9. S. Tsujikawa, Phys. Rev. D 76 023514, (2007). 10. L. Amendola, R. Gannouji, D. Polarski and S. Tsujikawa, Phys. Rev D 75 083504 (2007).
dspace.entity.typePublication
relation.isAuthorOfPublication16523fad-99a9-422c-9a8e-c949ccffadec
relation.isAuthorOfPublicatione14691a1-d3b0-47b7-96d5-24d645534471
relation.isAuthorOfPublication.latestForDiscovery16523fad-99a9-422c-9a8e-c949ccffadec

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