Deus ex H0 -- Is evidence for dynamical dark energy conditioned on early cosmology?
Nils Schöneberg, Rodrigo Calderón, Julien Lesgourgues
Abstract
Some free-form reconstructions of the dark energy equation of state suggest that dynamical dark energy is the only explanation for the observed data. In this letter we argue that early Universe solutions to the Hubble tension (around or before recombination) generically cause the evidence for this claim to strongly reduce, establishing a tight connection between the early and late cosmology. In particular, the level of evidence for dynamical dark energy depends on the parameters H0 rd and Ωm and early universe solutions typically push towards higher values of H0 rd and lower values of Ωm, where such evidence is reduced.
Create a lesson
Related papers
Follow-up of SN 2025wny VI: The Rate and Detectable Population of Strongly Lensed SLSNe-I in ZTF
Jacob O. Hjortlund, Edvard Mörtsell, Ariel Goobar et al.
Cosmological anatomy of interacting dark energy
Miguel A. Sabogal, Sunny Vagnozzi, Eleonora Di Valentino
Void probability function in the Quijote simulations
Snehasish Bhattacharjee
Constraints of Big Bang Nucleosynthesis and Cosmological Observations on varying Higgs VEV
Hongrui Feng, Yudong Luo, Toshitaka Kajino et al.
Infrared Universality of Scalar Induced Gravitational Waves Beyond Second Order
Chen Yuan
Resolving 3 Exotic Hyperbolic-Umbilic Lensing Configurations in the "Cosmic Mantis": An Exploration of RXJ0437.1+0043 with JWST
Catherine Cerny, David J. Lagattuta, Keren Sharon et al.