Constraints on some f(R) gravity models in the Palatini formalism from a time-varying gravitational constant

Details Constraints on some f(R) gravity models in the Palatini formalism from a time-varying gravitational constant Constraints on some f(R) gravity models in the Palatini formalism from a time-varying gravitational constant

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phrvd..79h3536l&link_type=abstract

Physical Review D, vol. 79, Issue 8, id. 083536

Physics

6

Cosmology, Modified Theories Of Gravity, Dark Energy

Scientific paper

In this work, we studied how the relative variation of the gravitational constant |Ḡ˙/Ḡ|0 at the redshift z=0 restricts model parameters in Palatini f(R) gravity. According to results from the observation of big bang nucleosynthesis and the anisotropies in the cosmic microwave background radiation, the ratio that gives the general constraint condition on the f(R) model is taken to be |Ḡ˙/Ḡ|0<10-13yr-1. Associating with the scalar curvature at present, this constraint condition yields concrete relations among model parameters in the generalized ΛCDM model, the logarithmic Lagrangian, and the exponential gravity model. These constraint relations which can be reconcilable with the value |Ḡ˙/Ḡ|0<10-13yr-1 are plotted.

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