Please use this identifier to cite or link to this item: https://www.um.edu.mt/library/oar/handle/123456789/121229
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dc.contributor.authorBernardo, Reginald Christian-
dc.contributor.authorGrandón, Daniela-
dc.contributor.authorSaid, Jackson-
dc.contributor.authorCárdenas, Víctor H.-
dc.date.accessioned2024-04-24T09:16:19Z-
dc.date.available2024-04-24T09:16:19Z-
dc.date.issued2023-
dc.identifier.citationBernardo, R. C., Grandón, D., Said, J. L., & Cárdenas, V. H. (2023). Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation. Physics of the Dark Universe, 40, 101213.en_GB
dc.identifier.issn22126864-
dc.identifier.urihttps://www.um.edu.mt/library/oar/handle/123456789/121229-
dc.description.abstractWe look at dark energy from a biology inspired viewpoint by means of the Approximate Bayesian Computation (ABC) and late time cosmological observations. We find that dynamical dark energy comes out on top, or in the ABC language naturally selected, over the standard CDM cosmological scenario. We confirm this conclusion is robust to whether baryon acoustic oscillations and Hubble constant priors are considered. Our results show that the algorithm prefers low values of the Hubble constant, consistent or at least a few standard deviation away from the cosmic microwave background estimate, regardless of the priors taken initially in each model. This supports the result of the traditional MCMC analysis and could be viewed as strengthening evidence for dynamical dark energy being a more favorable model of late time cosmology.en_GB
dc.language.isoenen_GB
dc.publisherElsevier BVen_GB
dc.rightsinfo:eu-repo/semantics/restrictedAccessen_GB
dc.subjectBayesian statistical decision theoryen_GB
dc.subjectGravitationen_GB
dc.subjectGravityen_GB
dc.subjectDark energy (Astronomy)en_GB
dc.subjectCosmology -- Mathematical modelsen_GB
dc.subjectStatistical physicsen_GB
dc.titleDark energy by natural evolution : constraining dark energy using approximate bayesian computationen_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.2023.101213-
dc.publication.titlePhysics of the Dark Universeen_GB
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