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The Time-Dependent Lambda Parameter in Haug-Tatum R H =ct Cosmology Appears Consistent with Recent DESI Findings

DOI: 10.4236/jmp.2026.176031, PP. 714-723

Keywords: Cosmological Constant, DESI, Hubble Parameter, Time-Dependent Lambda, Model, Dynamic Dark Energy, Cosmological Redshift, Cosmological Entropy, Black Hole Cosmology

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Abstract:

Based on the Haug-Tatum R H t =ct cosmology model redshift formula, z= R H 0 R H t ?1= H t H 0 ?1 , we demonstrate that the time-dependent Lambda parameter as a function of z must be Λ t = Λ 0 ( 1+z ) 4 . This equation is also consistent with the Haug and Tatum formula, Λ t =3 H t 2 c 2 =3 ( ? T t 2 c ) 2 and the observation-based relation, T t = T 0 (

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