The Rényi entropy and entropic cosmology

Entropic cosmology with the Rényi entropy of the apparent horizon $S_R=(1/α)\ln(1+αS_{BH})$, where $S_{BH}$ is the Bekenstein--Hawking entropy, is studied. By virtue of the thermodynamics-gravity correspondence a model of dark energy is investigated. The generalised Friedmann equations for the Friedmann--Lemaître--Robertson--Walker spatially flat universe with the barotropic matter fluid are obtained. We compute the dark energy density $ρ_D$, pressure $p_D$ and the deceleration parameter $q$ of the universe. At some model parameters the normalized density parameter of the matter $Ω_{m0}\approx 0.315$ and the deceleration parameter $q_0\approx -0.535$ for the current epoch, which are in the agreement with the Planck data, are found. Making use of the thermodynamics-gravity correspondence, we describe the late time of the universe acceleration. The entropic cosmology considered is equivalent to cosmology based on the teleparallel gravity with the definite function $F(T)$. The Hubble parameters are in approximate agreement (within $5$ percents) with the observational Hubble data for redshifts $0.07\leq z \leq 1.75$ at the entropy parameter $α\approx 0.305~GH_0^2$.

Source: arXiv:2605.00054v1 - http://arxiv.org/abs/2605.00054v1 PDF: https://arxiv.org/pdf/2605.00054v1 Original Link: http://arxiv.org/abs/2605.00054v1