Bose-Einstein distribution in RH = ct black hole horizon–driven, non–adiabatic cosmology

Haug [1] has recently demonstrated that the lithium problem appears to be solvable within RH = ct cosmology. For the model to be viable, it must also be consistent with the Bose–Einstein distribution. Here, we briefly demonstrate that the theory predicts g = 2, perfectly in line with the radiation-dominated phase of the universe. Furthermore, we show how the kinematic constraint RH = ct enforces H = 1/t and a∝t, while the gravitationally sustained radiation bath enforces ρrad \propto Tˆ4 \propto tˆ(−2). The resulting cosmology is horizon-driven, non-adiabatic, and entropy-balanced.