Thermodynamic constraints on fΛ(t) and hB(t) in a first-law-derived cosmological model are shown to reduce to ρ ≥ 0 and w ≥ -1, so the claimed consistency with the observed cosmological constant is an artifact of setting the integration constant C = Λ/3.
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Cosmological scenario based on the first and second laws of thermodynamics: Thermodynamic constraints on a generalized cosmological model
Thermodynamic constraints on fΛ(t) and hB(t) in a first-law-derived cosmological model are shown to reduce to ρ ≥ 0 and w ≥ -1, so the claimed consistency with the observed cosmological constant is an artifact of setting the integration constant C = Λ/3.