Cotton gravity in Codazzi parametrization produces horizon entropy equal to the Bekenstein-Hawking term plus a Codazzi-tensor correction whose sign diagnoses the type of cosmic matter.
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Fractional entropy on the apparent horizon yields stable modified cosmology that fits late-time data best at α near 2, shifting H0 upward as α decreases.
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Thermodynamic formulation of Cotton gravity in the Codazzi parametrization
Cotton gravity in Codazzi parametrization produces horizon entropy equal to the Bekenstein-Hawking term plus a Codazzi-tensor correction whose sign diagnoses the type of cosmic matter.
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Thermodynamic behavior of cosmological models with fractional entropy
Fractional entropy on the apparent horizon yields stable modified cosmology that fits late-time data best at α near 2, shifting H0 upward as α decreases.