Brane-world cosmology and varying $G$
Leonardo Amarilla, Hector Vucetich

TL;DR
This paper explores a brane-world cosmological model with a bulk scalar field where the Newton coupling G varies over time, and uses observational bounds to constrain the model's parameters.
Contribution
It introduces a brane-world model linking brane tension to G, leading to natural G variation and constrains it using nucleosynthesis and CMB data.
Findings
G variation is tightly constrained by nucleosynthesis.
CMB data provides the strongest bounds on model parameters.
Model links brane tension directly to Newton's G.
Abstract
We consider a brane-world cosmological model coupled to a bulk scalar field. Since the brane tension turns out to be proportional to Newton coupling , in such a model a time variation of naturally occurs. By resorting to available bounds on the variation of , the parameters of the model are constrained. The constraints coming from nucleosynthesis and CMB result to be the severest ones.
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