When Dark Energy Turns On: Constraints on a Critical Emergence Model
摘要
We investigate a specific emergent dark energy scenario, known as critically emergent dark energy (CEDE), in which dark energy is effectively absent in the early Universe and becomes dynamically relevant only after a critical cosmic epoch through a phase transition. We constrain this model using recent cosmological observations, including cosmic microwave background (CMB) data from \emph{Planck} 2018, baryon acoustic oscillation (BAO) measurements from SDSS and DESI DR2, and two independent Type Ia supernova compilations, PantheonPlus and Union3. Our results show that within the CEDE framework a dark energy phase transition is not ruled out. In particular, CMB-only, CMB+SDSS, and CMB+DESI datasets provide evidence for a nonzero transition scale factor and, according to standard statistical indicators such as and Bayesian evidence, can favor CEDE over the CDM model. At the same time, we find that CEDE does not fully resolve the Hubble constant tension. Overall, our analysis indicates that dark energy models featuring a phase transition remain a viable and phenomenologically interesting extension of the standard cosmological framework. Upcoming high-precision cosmological surveys will be essential to further assess whether such emergent dark energy scenarios represent a genuine departure from CDM or an effective description of current data.
引用
@article{arxiv.2603.13137,
title = {When Dark Energy Turns On: Constraints on a Critical Emergence Model},
author = {Mahdi Najafi and Mahdi Habibollahi and Masoume Reyhani and Eleonora Di Valentino and Supriya Pan and Javad T. Firouzjaee and Weiqiang Yang},
journal= {arXiv preprint arXiv:2603.13137},
year = {2026}
}