New entropy, thermodynamics of apparent horizon and cosmology
S. I. Kruglov

TL;DR
This paper introduces a new nonadditive entropy for the apparent horizon, develops corresponding Friedmann equations, and demonstrates its ability to model dark energy, universe acceleration, and inflation consistent with observational data.
Contribution
It proposes a novel entropy form for the apparent horizon, derives modified cosmological equations, and links holographic dark energy with teleparallel gravity, offering a new approach to cosmology.
Findings
Model parameters match Planck data for current universe.
The model exhibits phantom divide behavior for dark energy.
Equivalent to teleparallel gravity with specific F(T) functions.
Abstract
Here, we consider new nonadditive entropy of the apparent horizon with being the Bekenstein--Hawking entropy. This is an alternative of the R\'{e}nyi and Tsallis entropies, that allows us, by utilising the holographic principle, to develop entropic (holographic) dark energy. When our entropy becomes the Bekenstein--Hawking entropy . The generalized Friedmann equations for Friedmann--Lema\^{i}tre--Robertson--Walker (FLRW) spacetime for the barotropic matter fluid with were obtained. We compute the dark energy pressure , density of energy , the normalized density parameters , and the deceleration parameter of the universe corresponding to our model. From the second modified Friedmann equation a dynamical cosmological constant was obtained. We show that at some model…
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Taxonomy
TopicsCosmology and Gravitation Theories
