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dc.contributor.authorBriffa, Rebecca-
dc.contributor.authorEscamilla-Rivera, Celia-
dc.contributor.authorSaid, Jackson-
dc.contributor.authorMifsud, Jurgen-
dc.date.accessioned2024-04-22T08:43:00Z-
dc.date.available2024-04-22T08:43:00Z-
dc.date.issued2023-
dc.identifier.citationBriffa, R., Escamilla-Rivera, C., Said, J. L., & Mifsud, J. (2023). f (T, B) gravity in the late Universe in the context of local measurements. Physics of the Dark Universe, 39, 101153.en_GB
dc.identifier.issn22126864-
dc.identifier.urihttps://www.um.edu.mt/library/oar/handle/123456789/121125-
dc.description.abstractWe explore the viability of three models in gravity using data from recent surveys based on cosmic chronometers, the Pantheon data set, and baryonic acoustic oscillation data. We also assess the consistency of these models and data set combinations with two important priors on the Hubble constant coming from the SH0ES Team and measurements using the tip of the red giant branch respectively. These give the highest and lowest values of the Hubble constant coming from cosmology independent studies. In general, our analysis does provide a more consistent fit for the late time data being analysed. However, each model does include an additional model parameter in comparison with the concordance model. We close the analysis with a comparative analysis in which each model, data set and Hubble constant prior combination are cross-analysed against each other.en_GB
dc.language.isoenen_GB
dc.publisherElsevier BVen_GB
dc.rightsinfo:eu-repo/semantics/restrictedAccessen_GB
dc.subjectGravitation -- Researchen_GB
dc.subjectDark energy (Astronomy)en_GB
dc.subjectAstrophysics -- Observationsen_GB
dc.subjectCosmologyen_GB
dc.subjectGravityen_GB
dc.titlef (T , B) gravity in the late universe in the context of local measurementsen_GB
dc.typearticleen_GB
dc.rights.holderThe copyright of this work belongs to the author(s)/publisher. The rights of this work are as defined by the appropriate Copyright Legislation or as modified by any successive legislation. Users may access this work and can make use of the information contained in accordance with the Copyright Legislation provided that the author must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the prior permission of the copyright holder.en_GB
dc.description.reviewedpeer-revieweden_GB
dc.identifier.doi10.1016/j.dark.2022.101153-
dc.publication.titlePhysics of the Dark Universeen_GB
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