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Haug, E.G. and Tatum, E.T. (2026) How a New Type of Cosmological Model Outperforms the Λ-CDM Model in Numerous Categories and Resolves the Hubble Tension. Journal of Applied Mathematics and Physics, 14, 1206-1217.
https://doi.org/10.4236/jamp.2026.143057

has been cited by the following article:

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

  AUTHORS: Espen Gaarder Haug, Eugene Terry Tatum

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

  JOURNAL NAME: Journal of Modern Physics, Vol.17 No.6, June 30, 2026

  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 ( 1+z ) . We also show how H 0 predicted by the Haug-Tatum model is most consistent with the DESI-based H 0 estimates from the ω 0 ω a CDM model that allows for dynamic dark energy.