Publicación:
BAYESIAN COMPARISON OF INTERACTING SCENARIOS

dc.creatorMARÍA ANTONELLA CID MUÑOZ
dc.date2019
dc.date.accessioned2025-01-10T15:00:02Z
dc.date.available2025-01-10T15:00:02Z
dc.date.issued2019
dc.description.abstractWE PERFORM A BAYESIAN MODEL SELECTION ANALYSIS FOR DIFFERENT CLASSES OF PHENOMENOLOGICAL COUPLED SCENARIOS OF DARK MATTER AND DARK ENERGY WITH LINEAR AND NON-LINEAR INTERACTING TERMS. WE USE A COMBINATION OF SOME OF THE LATEST COSMOLOGICAL DATA SUCH AS TYPE IA SUPERNOVAE (SNE IA), COSMIC CHRONOMETERS (CC), COSMIC MICROWAVE BACKGROUND (CMB) AND TWO SETS OF BARYON ACOUSTIC OSCILLATIONS MEASUREMENTS, NAMELY, 2-DIMENSIONAL ANGULAR MEASUREMENTS (BAO2) AND 3-DIMENSIONAL ANGLE-AVERAGED MEASUREMENTS (BAO3). WE FIND WEAK AND MODERATE EVIDENCE AGAINST TWO-THIRDS OF THE INTERACTING SCENARIOS CONSIDERED WITH RESPECT TO ?CDM WHEN THE FULL JOINT ANALYSIS IS CONSIDERED. ABOUT ONE-THIRD OF THE MODELS PROVIDE A DESCRIPTION TO THE DATA AS GOOD AS THE ONE PROVIDED BY THE STANDARD MODEL. OUR RESULTS ALSO INDICATE THAT EITHER SNE IA, CC OR BAO2 DATA BY THEMSELVES ARE NOT ABLE TO DISTINGUISH AMONG INTERACTING MODELS OR ?CDM BUT THE STANDARD BAO3 MEASUREMENTS AND THE COMBINATION WITH THE CMB DATA ARE INDEED ABLE TO DISCRIMINATE AMONG THEM. WE FIND THAT EVIDENCE DISFAVORING INTERACTING MODELS IS WEAKER WHEN WE USE BAO2 (DATA CLAIMED TO BE ALMOST MODEL-INDEPENDENT) INSTEAD OF THE STANDARD BAO3 MEASUREMENTS. THESE RESULTS HELP SELECT CLASSES OF VIABLE AND NON-VIABLE INTERACTING MODELS IN LIGHT OF CURRENT DATA.
dc.formatapplication/pdf
dc.identifier.doi10.1088/1475-7516/2019/03/030
dc.identifier.issn1475-7516
dc.identifier.issn1475-7516
dc.identifier.urihttps://repositorio.ubiobio.cl/handle/123456789/9940
dc.languagespa
dc.publisherJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
dc.relation.uri10.1088/1475-7516/2019/03/030
dc.rightsPUBLICADA
dc.titleBAYESIAN COMPARISON OF INTERACTING SCENARIOS
dc.title.alternativeCOMPARACIÓN BAYESIANA DE ESCENARIOS DE INTERACCIÓN
dc.typeARTÍCULO
dspace.entity.typePublication
ubb.EstadoPUBLICADA
ubb.Otra ReparticionDEPARTAMENTO DE FISICA
ubb.SedeCONCEPCIÓN
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