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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In quadratic curvature-matter coupled gravity, strange stars described by the MIT bag equation of state can attain a maximum mass of 3.11 solar masses, exceeding the general-relativistic limit and potentially accounting for the lighter companion in GW190814.
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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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Maximum mass limit of strange stars in quadratic curvature-matter coupled gravity
In quadratic curvature-matter coupled gravity, strange stars described by the MIT bag equation of state can attain a maximum mass of 3.11 solar masses, exceeding the general-relativistic limit and potentially accounting for the lighter companion in GW190814.