Probing dark energy with braneworld cosmology in the light of recent cosmological data
Miguel A. Garcia-Aspeitia, Juan Maga\~na, Alberto Hernandez-Almada and, V. Motta

TL;DR
This paper tests a braneworld cosmology model with dark energy against recent observational data, finding no significant deviations from standard cosmology but setting new bounds on model parameters.
Contribution
It provides observational constraints on a Randall-Sundrum braneworld model with dark energy using multiple cosmological datasets.
Findings
EoS consistent with cosmological constant at 3σ
BAO data favors quintessence dark energy
No significant evidence for extra dimension effects within current uncertainties
Abstract
We investigate a brane model based on Randall-Sundrum scenarios with a generic dark energy component. The latter drives the accelerated expansion at late times of the Universe. In this scheme, extra terms are added into Einstein Field equations that are propagated to the Friedmann equations. To constrain the dark energy equation of state (EoS) and the brane tension we use observational data with different energy levels (Supernovae type Ia, , baryon acoustic oscillations, and cosmic microwave background radiation distance, and a joint analysis) in a background cosmology. Beside EoS being consistent with a cosmological constant at the confidence level for each dataset, the baryon acoustic oscillations probe favors an EoS consistent with a quintessence dark energy. Although we found different lower limit bounds on the brane tension for each data sets, being the most…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
