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Son, J., Lee, Y., Chung, C., Park, S. and Cho, H. (2025) Strong Progenitor Age Bias in Supernova Cosmology II. Alignment with DESI BAO and Signs of a Non-Accelerating Universe. Monthly Notices of the Royal Astronomical Society, 544, 975-987.
https://doi.org/10.1093/mnras/staf1685

has been cited by the following article:

• TITLE: Physical Properties of the Types of Dark Energy Introduced in Light of the “DESI-Pressure” upon the ΛCDM Universe Model

  AUTHORS: Øyvind G. Grøn

  KEYWORDS: Dark Energy, Cosmological Model, Equation of State, Hubble Tension, Deceleration Parameter

  JOURNAL NAME: Journal of Applied Mathematics and Physics, Vol.14 No.2, February 28, 2026

  ABSTRACT: This paper presents an introduction to the main point in the changes of the ΛCDM-universe model that the cosmologists have proposed in light of the DESI-observational data and other types of observations: New types of dark energy characterized by different equations of state than that of Lorentz invariant vacuum energy, LIVE, with constant density in the ΛCDM-universe model. Gravitational properties and time evolution of these new types of dark energy are discussed and illustrated graphically by employing analytical expressions for dimensionless density factors, resulting from integrating the equation of continuity of the different models. The density factors are employed to calculate the time evolution of the deceleration parameters of universe models with different types of dark energy. It is also shown that the introduction of the w0waCDM-universe models changes the value of Hubble’s constant relative to that of the ΛCDM-universe model, but with a too small magnitude to solve the Hubble tension. It is argued that this is a general feature of all dynamical dark energy models constrained by low redshift data.