Constraints on Redshift-Binned Dark Energy using DESI BAO Data
Ye-Huang Pang, Xue Zhang, Qing-Guo Huang

TL;DR
This study constrains the redshift-dependent dark energy equation of state using DESI BAO, Planck, ACT, and supernova data, exploring models with early dark energy to address the H0 tension, but finds no conclusive transition pattern.
Contribution
It introduces a redshift-binned dark energy model constrained by multiple datasets, including EDE, to investigate dark energy evolution and the H0 tension.
Findings
W1>-1 at 1.9-3.3 sigma depending on data
W3< -1 within 1.5 sigma in various datasets
Dark energy transition from phantom to quintessence remains inconclusive
Abstract
We parameterize the equation of state of late-time dark energy as , with three redshift bins, characterized by a constant equation of state in each bin. Then, we constrain the parameters of the CDM model using datasets from DESI BAO data, Planck CMB power spectrum, ACT DR6 lensing power spectrum, and type Ia supernova distance-redshift data of Pantheon Plus/DES Y5/Union3. The significances for is , and , and is consistent with within level, while , and for in these three data combinations with different choices of type Ia supernova datasets, respectively. Additionally, to alleviate tension, we incorporate the early dark energy (EDE) model in the early-time universe and add the SH0ES absolute magnitude prior (or prior) to…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Adaptive optics and wavefront sensing · Geophysics and Gravity Measurements
