Large scale structure constraints for a class of f(R) theories of gravity

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dc.contributor.authorAbebe, Amare
dc.contributor.authorCruz Dombriz, Álvaro de la
dc.contributor.authorDunsby, Peter K. S.
dc.date.accessioned2023-06-19T13:28:28Z
dc.date.available2023-06-19T13:28:28Z
dc.date.issued2013-08-26
dc.description© 2013 American Physical Society. We would like to thank David Bacon for a comprehensive reading of the manuscript and for his useful comments. We are also indebted to Marc Manera and Ashley Ross for providing us the most updated literature about the SDSS-III project. We warmly thank as well José Beltrán for useful comments about BAO calculations. A. A. acknowledges financial support from NRF (South Africa). A. d. l. C. D. acknowledges financial support from Marie Curie–Beatriu de Pinós Contract No. BP-B00195 Generalitat de Catalunya, ACGC University of Cape Town and MINECO (Spain) Projects No. FIS2011-23000, No. FPA2011-27853-C02-01 and Consolider-Ingenio MULTIDARK Grant No. CSD2009-00064. P. K. S. D. thanks the NRF for financial support and Queen Mary, University of London for support during the final stages of this work. A. d. l. C. D. thanks the KITPC, Chinese Academy of Sciences, for its hospitality during the final stages of this work.
dc.description.abstractOver the past few years much attention has been given to the study of modified gravity theories in order to find a more natural explanation for the late time acceleration of the Universe. Nevertheless, a comparison of the matter power spectrum predictions made by these theories with available data has not yet been subjected to a detailed analysis. In the context of f(R) theories of gravity we study the predicted power spectra using both a dynamical systems approach for the background and solving for the matter perturbations without using the quasistatic approximation, comparing the theoretical results with several Sloan Digital Sky Survey data. The importance of studying the first order perturbed equations by assuming the correct background evolution and the relevance of the initial conditions are also stressed. We determine the statistical significance in relation to the observational data and demonstrate their conflict with existing observations.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipNRF (South Africa)
dc.description.sponsorshipMarie Curie-Beatriu de Pinos Contract
dc.description.sponsorshipGeneralitat de Catalunya
dc.description.sponsorshipACGC University of Cape Town
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO), España
dc.description.sponsorshipNRF
dc.description.sponsorshipQueen Mary, University of London
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/28584
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dc.identifier.doi10.1103/PhysRevD.88.044050
dc.identifier.issn1550-7998
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.88.044050
dc.identifier.relatedurlhttp://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/33807
dc.issue.number4
dc.journal.titlePhysical review D
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.projectIDBP-B00195
dc.relation.projectIDFIS2011-23000
dc.relation.projectIDFPA2011-27853-C02-01
dc.relation.projectIDCSD2009-00064
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordBaryon acoustic-Oscillations
dc.subject.keywordR-N-Gravity
dc.subject.keywordNonlinear gravitational lagrangians
dc.subject.keywordMicrowave background anisotropies
dc.subject.keywordGauge-Invariant perturbations
dc.subject.keywordHigh-Redshift supernovae
dc.subject.keywordProbe wmap observations
dc.subject.keywordHubble-Space-Telescope
dc.subject.keywordDigital sky survey
dc.subject.keywordCosmological perturbations
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleLarge scale structure constraints for a class of f(R) theories of gravity
dc.typejournal article
dc.volume.number88
dspace.entity.typePublication
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