Modified cosmology through Kaniadakis horizon entropy
Andreas Lymperis, Spyros Basilakos, Emmanuel N. Saridakis

TL;DR
This paper explores modified cosmological models derived from applying the first law of thermodynamics to the universe horizon using Kaniadakis entropy, leading to new dark energy behaviors and consistent cosmic evolution.
Contribution
It introduces a novel cosmological framework based on Kaniadakis entropy, resulting in modified Friedmann equations and dark energy dynamics dependent on a new parameter.
Findings
Universe exhibits standard thermal history with transition at redshift ~0.6
Dark energy equation-of-state deviates from ΛCDM and remains in the phantom regime
Cosmology approaches de Sitter phase at late times, consistent with observations
Abstract
We apply the gravity-thermodynamics conjecture, namely the first law of thermodynamics on the Universe horizon, but using the generalized Kaniadakis entropy instead of the standard Bekenstein-Hawking one. The former is a one-parameter generalization of the classical Boltzmann-Gibbs-Shannon entropy, arising from a coherent and self-consistent relativistic statistical theory. We obtain new modified cosmological scenarios, namely modified Friedmann equations, which contain new extra terms that constitute an effective dark energy sector depending on the single model Kaniadakis parameter . We investigate the cosmological evolution, by extracting analytical expressions for the dark energy density and equation-of-state parameters and we show that the Universe exhibits the usual thermal history, with a transition redshift from deceleration to acceleration at around 0.6. Furthermore,…
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