Reconstructing cosmic expansion in $f(R, G)$ gravity using a log-periodic deceleration model

TL;DR

This paper reconstructs the late-time cosmic expansion using a specific $f(R,G)$ gravity model with a log-periodic deceleration parameter, constrained by multiple observational datasets, and finds results consistent with current cosmological observations.

Contribution

It introduces a novel $f(R,G)$ gravity model with a log-periodic deceleration parameter and constrains it using comprehensive observational data, demonstrating its viability for describing cosmic acceleration.

Findings

Hubble constant estimated between 71.7 and 72.8 km/s/Mpc.

Transition redshift from deceleration to acceleration around 0.744 to 0.879.

Model satisfies energy conditions NEC and DEC, with SEC violated at late times.

Abstract

We study the late-time cosmology in $f(R, G)=R+\alpha R^{2}+\beta e^{\gamma G}$, using a logarithmic parametrization of the deceleration parameter $q(z)=q_{0}+q_{1}sin[log(1+z)]$. The Hubble parameter $H(z)$ is reconstructed and model parameters are constrained via MCMC analysis using CC ($31$), BAO ($26$) and Pantheon+SHOES ($1701$) datasets. Our results yield a Hubble constant in the range $H_0 = 71.7$--$72.8$ km/s/Mpc, consistent with late-time observations. The present deceleration parameter is found to be $q_{0}=-0.484$ to $-0.517$, while the evolution parameter $q_{1}\approx 1$, indicating increasing acceleration. The transition redshift shifts from $z_{tr}=0.879$ (CC) to $0.744$ (CC+BAO+Pantheon+SHOES), supporting a dynamic acceleration phase. The model reproduces early radiation behavior with $\omega (z>>1) \approx 0.33$ and predicts present-day values $\omega_{0} \approx -0.49$. Energy conditions NEC and DEC are satisfied, while SEC is violated at late times. The statefinder parameters $\{r_0, s_0\} = (0.866, 0.046)$ lie near the $\Lambda$CDM point. Estimated age of the Universe ranges from $13.01$ to $13.59$ Gyr. Thermodynamic analysis confirms consistency with the generalized second law. Overall, the model offers a viable and observationally consistent description of cosmic acceleration.