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MODIFIED HOLOGRAPHIC RICCI INTERACTING DARK ENERGY MODELS: DYNAMICAL SYSTEM ANALYSIS AND BAYESIAN COMPARISON

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dc.creatorMARÍA ANTONELLA CID MUÑOZ
dc.date2024
dc.date.accessioned2025-01-10T15:50:50Z
dc.date.available2025-01-10T15:50:50Z
dc.date.issued2024
dc.description.abstractWE PERFORM A DYNAMICAL SYSTEM ANALYSIS AND A BAYESIAN MODEL SELECTION FOR A NEW SET OF INTERACTING SCE- NARIOS IN THE FRAMEWORK OF MODIFIED HOLOGRAPHIC RICCI DARK ENERGY (MHR-IDE) MODELS. THE DYNAMICAL ANALYSIS SHOWS A MODIFIED RADIATION EPOCH AND A LATE-TIME ATTRACTOR CORRE- SPONDING TO AN ACCELERATED PHASE OF HOLOGRAPHIC DARK ENERGY. IN THE BAYESIAN COMPARISON, WE USE A COMBINATION OF BACK- GROUND DATA INCLUDING TYPE IA SUPERNOVAE, COSMIC CHRONOME- TERS, THE LOCAL VALUE OF THE HUBBLE CONSTANT, BARYON ACOUS- TIC OSCILLATIONS, AND COSMIC MICROWAVE BACKGROUND DATA. WE FIND EVIDENCE AGAINST ALL THE MHR-IDE SCENARIOS STUDIED IN COMPARISON WITH THE ?CDM WHEN THE FULL JOINT ANALYSIS IS CONSIDERED.
dc.formatapplication/pdf
dc.identifier.doi10.1140/epjc/s10052-024-12871-x
dc.identifier.issn1434-6052
dc.identifier.issn1434-6044
dc.identifier.urihttps://repositorio.ubiobio.cl/handle/123456789/13926
dc.languagespa
dc.publisherEUROPEAN PHYSICAL JOURNAL C
dc.relation.uri10.1140/epjc/s10052-024-12871-x
dc.rightsPUBLICADA
dc.subjectINFRARED CUTOFF
dc.subjectENTROPY BOUNDS
dc.subjectBLACK-HOLES
dc.titleMODIFIED HOLOGRAPHIC RICCI INTERACTING DARK ENERGY MODELS: DYNAMICAL SYSTEM ANALYSIS AND BAYESIAN COMPARISON
dc.typeARTÍCULO
dspace.entity.typePublication
ubb.EstadoPUBLICADA
ubb.Otra ReparticionDEPARTAMENTO DE FISICA
ubb.SedeCONCEPCIÓN
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