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dc.contributor.authorOrtiz Baños, María
dc.contributor.authorBouhmadi López, Mariam ORCID
dc.contributor.authorLazcoz Sáez, Ruth ORCID
dc.contributor.authorSalzano, Vincenzo
dc.date.accessioned2021-04-21T07:31:53Z
dc.date.available2021-04-21T07:31:53Z
dc.date.issued2021-03-17
dc.identifier.citationEuropean Physical Journal C 81(3) : (2021) // Article ID 237es_ES
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.urihttp://hdl.handle.net/10810/51120
dc.description.abstractIn this work, we further study a metric modified theory of gravity which contains a non-minimal coupling to matter, more precisely, we assume two functions of the scalar curvature, f1 and f2, where the first one generalises the Hilbert-Einstein action, while the second couples to the matter Lagrangian. On the one hand, assuming a Lambda CDM background, we calculate analytical solutions for the functions f1 and f2. We consider two setups: on the first one, we fix f2 and compute f1 and on the second one, we fix f1 and compute f2. Moreover, we do the analysis for two different energy density contents, a matter dominated universe and a general perfect fluid with a constant equation of state fuelling the universe expansion. On the other hand, we complete our study by performing a cosmographic analysis for f1 and f2. We conclude that the gravitational coupling to matter can drive the accelerated expansion of the universees_ES
dc.description.sponsorshipM. B.-L., M. O. B. and R. L. were supported by the Spanish Ministry of Economy and Competitiveness through research projects No. FIS2017-85076-P (MINECO/AEI/FEDER, UE) and also by the Basque Government through research project No. GIC17/116-IT956-16. M.O.B. acknowledges financial support from the FPI grant BES-2015-071489. The work of M.B.L. is also supported by the Basque Foundation of Science IKERBASQUE. This article is based upon work from COST Action CA15117 (CANTATA), supported by COST (European Cooperation in Science and Technology)es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.relationinfo:eu-repo/grantAgreement/MICINN/FIS2017-85076-Pes_ES
dc.relationinfo:eu-repo/grantAgreement/MICINN/BES-2015-071489es_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectmetric modified theory of gravityes_ES
dc.subjectHilbert-Einsteines_ES
dc.subjectmatter Lagrangianes_ES
dc.subjectLambda CDMes_ES
dc.subjectcosmographic analysises_ES
dc.subjectuniverse expansiones_ES
dc.subjectgravitational coupling to matteres_ES
dc.titleLambda CDM Suitably Embedded in f(R) with a Non-Minimal Coupling to Matteres_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderThis article is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0)es_ES
dc.rights.holderAtribución 3.0 España*
dc.relation.publisherversionhttps://link-springer-com.ehu.idm.oclc.org/article/10.1140%2Fepjc%2Fs10052-021-09004-zes_ES
dc.identifier.doi10.1140/epjc/s10052-021-09004-z
dc.departamentoesFísicaes_ES
dc.departamentoeuFisikaes_ES


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This article is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0)
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