Thermodynamic Cosmology from the CMB Temperature and the Planck Temperature and The Relation to Quantum Cosmology

In this paper, we demonstrate that, in RH = ct cosmology, a wide range of cosmological parameters and properties can be expressed simply as functions of the CMB temperature relative to the Planck temperature, as well as the Hawking temperature relative to the CMB temperature. This approach offers a novel framework for studying the thermodynamics of the cosmos within black hole cosmology. Notably, it enhances the precision of predictions and introduces a minimum acceleration associated with a mass gap, which may provide a plausible explanation for galaxy rotation curves.