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Cosmological observations in scalar-tensor quintessence
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The framework for considering the astronomical and cosmological observations in the context of scalar-tensor quintessence in which the quintessence field also accounts for a time dependence of the gravitational constant is developed. The constraints arising from nucleosynthesis, the variation of the constant, and the post-Newtonian measurements are taken into account. A simple model of supernovae is presented in order to extract the dependence of their light curves with the gravitational constant; this implies a correction when fitting the luminosity distance. The properties of perturbations as well as CMB anisotropies are also investigated.
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Cited by 1 Pith paper
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Bridge the Cosmological Tensions with Thawing Gravity
Thawing Gravity, a scalar-tensor theory with a non-minimally coupled scalar field, fits the full cosmological dataset better than LambdaCDM and yields H0=71.78+/-0.86 and S8=0.793+/-0.012.
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