Model-Independent Indication for a Localized Anomaly in the Late-Time Expansion History
Shibendu Gupta Choudhury, Purba Mukherjee, Eleonora Di Valentino, Anjan A Sen
astro-ph.CO, gr-qc
Submitted: 2026-07-14
Comments: 15 pages, 5 figures, comments are welcome
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- From Data to Software to Science with the Rubin Observatory LSST
- Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation
- Distance measures in cosmology
- Union3.1: Reducing Systematics in Supernova Cosmology with Self-consistent Measurements of Host Galaxy Properties for 2000 Type Ia Supernovae
- Persistent and serious challenge to the $\Lambda$CDM throne: Evidence for dynamical dark energy rising from combinations of different types of datasets
- Reconstructing dark energy with fewer assumptions
- One-parameter dynamical dark energy: Hints for oscillations
- Evolving Dark Energy Is Vacuum Energy After All
- Updated constraints on interacting dark energy: A comprehensive analysis using multiple CMB probes, DESI DR2, and supernovae observations
- Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond- CDM Interpretations, and Tensions
- Robust Preference for Dark Sector Interactions
- When Dark Energy Turns On: Constraints on a Critical Emergence Model
- Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing
- Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models
- Dynamical Dark Energy Meets Varying Electron Mass: Implications for Phantom Crossing and the Hubble Constant
- When One-Parameter Dark Energy Makes Neutrinos Physical Again
- Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO
- Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies
- Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2
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