Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?

Documents similaires

• Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data?
  par: Pérez, Javier de Cruz, et autres
  Publié: (2026)
• Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?
  par: Park, Chan-Gyung, et autres
  Publié: (2025)
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
  par: Park, Chan-Gyung, et autres
  Publié: (2024)
• Updated observational constraints on $ϕ$CDM dynamical dark energy cosmological models
  par: Park, Chan-Gyung, et autres
  Publié: (2025)
• Updated observational constraints on spatially-flat and non-flat $Λ$CDM and XCDM cosmological models
  par: Perez, Javier de Cruz, et autres
  Publié: (2024)