Observational constrains on the DGP brane-world model with a Gauss-Bonnet term in the bulk
Jian-Hua He, Bin Wang, Eleftherios Papantonopoulos

TL;DR
This paper evaluates the DGP brane-world model with a Gauss-Bonnet term using supernova, BAO, and H(z) data, finding it a viable explanation for cosmic acceleration.
Contribution
It provides the first comprehensive observational constraints on the DGP model with a Gauss-Bonnet term in the bulk.
Findings
Gauss-Bonnet-Induced Gravity model fits observational data well
Model can explain the universe's accelerated expansion
Parameters are consistent with current cosmological observations
Abstract
Using the data coming from the new 182 Gold type Ia supernova samples, the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey and the H(z) data, we have performed a statistical joint analysis of the DGP brane-world model with a high curvature Gauss-Bonnet term in the bulk. Consistent parameters estimations show that the Gauss-Bonnet-Induced Gravity model is a viable candidate to explain the observed acceleration of our universe.
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