Study of dynamical dark energy using DESI DR2 BAO, CMB, and Type Ia Supernovae data
Abstract
Dark Energy Spectroscopic Instrument (DESI) Collaboration reported an evidence for dynamical dark energy model using baryon acoustic oscillation (BAO) measurements from DESI Data Release 2 (DR2), cosmic microwave background (CMB), and three Type Ia Supernovae (SNe) data (Pantheon+, Union3, and DES-SN5YR) recently. The significances are from 2.8∼4.2σ depending on which SNe sample is used, and the highest significance is obtained based on the DES-SN5YR data. But more recently, Dark Energy Survey (DES) Collaboration recalibrated the DES-SN5YR data, and a significance of only 3.2σ is obtained based on the calibrated data, which is called DES-Dovekie. In this work, we perform a comprehensive analysis of five representative dynamical dark energy parametrization models, including Chevallier-Polarski-Linder (CPL), Barboza-Alcaniz (BA), exponential (EXP), logarithmic (LOG), and Jassal-Bagla-Padmanabhan (JBP), using DESI DR2 BAO, Planck CMB, ACT DR6, and SNe data from Pantheon+, Union3, and DES-Dovekie. Similarly, a significance of around 3σ is obtained based on the DES-Dovekie data. And the significances are 2.1∼3.7σ for different SNe samples and different parametrization models, indicating an evolutionary dark energy dynamics. Furthermore, a phantom-like behavior in the past and has transitioned into quintessence-like behavior today for the dynamical dark energy is preferred.
Related
- Testing ΛCDM versus Dynamical Dark Energy in 1 Yr: A DESI Spectroscopic Follow-up Program for Rubin Supernovae
- A new window on dynamical dark energy: combining DESI-DR2 BAO with future gravitational wave observations
- Is DESI Seeing Dynamical Dark Energy, or a Cosmic Glitch in Gravity?
- Reassessing Evidence for Dark-Sector Interactions with Dynamical Dark Energy and DESI DR2
- Searching for Type Ia Supernovae in the Dark Energy Spectroscopic Instrument
BibTeX
@misc{wang2026study,
title = {{Study of dynamical dark energy using DESI DR2 BAO, CMB, and Type Ia Supernovae data}},
author = {Pin Wang and Ping Wang and Jielei Zhang},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.10567},
eprint = {2609.10567},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.10567},
}
RIS
TY - UNPB
TI - Study of dynamical dark energy using DESI DR2 BAO, CMB, and Type Ia Supernovae data
AU - Pin Wang
AU - Ping Wang
AU - Jielei Zhang
PY - 2026
DA - 2026/09/01
PB - arXiv
DO - 10.48550/arxiv.2609.10567
UR - https://arxiv.org/abs/2609.10567
AB - Dark Energy Spectroscopic Instrument (DESI) Collaboration reported an evidence for dynamical dark energy model using baryon acoustic oscillation (BAO) measurements from DESI Data Release 2 (DR2), cosmic microwave background (CMB), and three Type Ia Supernovae (SNe) data (Pantheon+, Union3, and DES-SN5YR) recently. The significances are from 2.8∼4.2σ depending on which SNe sample is used, and the highest significance is obtained based on the DES-SN5YR data. But more recently, Dark Energy Survey (DES) Collaboration recalibrated the DES-SN5YR data, and a significance of only 3.2σ is obtained based on the calibrated data, which is called DES-Dovekie. In this work, we perform a comprehensive analysis of five representative dynamical dark energy parametrization models, including Chevallier-Polarski-Linder (CPL), Barboza-Alcaniz (BA), exponential (EXP), logarithmic (LOG), and Jassal-Bagla-Padmanabhan (JBP), using DESI DR2 BAO, Planck CMB, ACT DR6, and SNe data from Pantheon+, Union3, and DES-Dovekie. Similarly, a significance of around 3σ is obtained based on the DES-Dovekie data. And the significances are 2.1∼3.7σ for different SNe samples and different parametrization models, indicating an evolutionary dark energy dynamics. Furthermore, a phantom-like behavior in the past and has transitioned into quintessence-like behavior today for the dynamical dark energy is preferred.
ER -