The gravity and affine EoS: Compatibility and observational constraints
This paper investigates the cosmological implications of an affine equation of state within General Relativity and gravity, demonstrating that while both frameworks can unify the universe's transition from decelerated to accelerated expansion, the affine model yields quintessence-like dark energy in General Relativity but phantom-like dark energy in gravity, with parameters constrained by Cosmic Chronometer and Supernovae type Ia data.