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New entropy, thermodynamics of apparent horizon and cosmology
Here, we consider new nonadditive entropy of the apparent horizon $S_K=S_{BH}/(1+γS_{BH})$ with $S_{BH}$ being the Bekenstein--Hawking entropy. This is an alternative of the Rényi and Tsallis entropies, that allows us, by utilising the holographic principle, to develop a new model of entropic (holog
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