Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements
Purba Mukherjee, Arman Shafieloo, Varun Sahni
astro-ph.CO, gr-qc
Submitted: 2026-08-03
Comments: 16 pages, 14 figures. Comments are welcome
Code: https://github.com/lesgourg/class_public
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
- Cosmological Constant - the Weight of the Vacuum
- Cosmological tensions in the era of precision cosmology: Insights from Tensions in Cosmology 2025
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Tensions between the Early and the Late Universe
- The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
- Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- A population of red candidate massive galaxies ~600 Myr after the Big Bang
- Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- New Expansion Rate Anomalies at Characteristic Redshifts Geometrically Determined using DESI-DR2 BAO and DES-SN5YR Observations
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