Generalized emergent dark energy: observational Hubble data constraints and stability analysis

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dc.contributor.authorHernandez-Almada, A.
dc.contributor.authorLeon, Genly
dc.contributor.authorMagana, Juan
dc.contributor.authorGarcia-Aspeitia, Miguel A.
dc.contributor.authorMotta, V
dc.date.accessioned2025-01-23T19:47:48Z
dc.date.available2025-01-23T19:47:48Z
dc.date.issued2020
dc.description.abstractRecently, a phenomenologically emergent dark energy (PEDE) model was presented with a dark energy density evolving as (Omega) over tilde (DE)(z) = Omega(DE,0)[1 - tanh(log(10)(1 + z))], i.e. with no degree of freedom. Later on, a generalized model was proposed by adding one degree of freedom to the PEDE model, encoded in the parameter Delta. Motivated by these proposals, we constrain the parameter space (h, Omega((0))(m)) and (h, Omega((0))(m), Delta) for PEDE and generalized emergent dark energy (GEDE), respectively, by employing the most recent observational (non-)homogeneous and differential age Hubble data. Additionally, we reconstruct the deceleration and jerk parameters and estimate yield values at z = 0 of q(0) = -0.784(-0.027)(+0.028) and j(0) = 1.241(-0.149)(+0.164) for PEDE and q(0) = -0.730(-0.067)(+0.059) and j(0) = 1.293(-0.187)(+0.194) for GEDE using the homogeneous sample. We report values on the deceleration-acceleration transition redshift with those reported in the literature within 2 sigma CL. Furthermore, we perform a stability analysis of the PEDE and GEDE models to study the global evolution of the Universe around their critical points. Although the PEDE and GEDE dynamics are similar to the standard model, our stability analysis indicates that in both models there is an accelerated phase at early epochs of the Universe evolution.
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/staa2052
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/staa2052
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/100411
dc.identifier.wosidWOS:000574924500024
dc.issue.numero2
dc.language.isoen
dc.pagina.final1602
dc.pagina.inicio1590
dc.revistaMonthly notices of the royal astronomical society
dc.rightsacceso restringido
dc.subjectcosmological parameters
dc.subjectdark energy
dc.subjectcosmology: observations
dc.subjectcosmology: theory
dc.titleGeneralized emergent dark energy: observational Hubble data constraints and stability analysis
dc.typeartículo
dc.volumen497
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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