Thermodynamic reconstruction in observationally constrained dynamical dark energy models
astro-ph.CO
Submitted: 2026-08-31
Updated: 2026-09-19
Journal ref: Phys. Lett. B 881 (2026) 140879
DOI: 10.1016/j.physletb.2026.140879
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Planck 2018 results. VI. Cosmological parameters
- Challenges for $\Lambda$CDM: An update
- DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
- The Hubble Tension and Early Dark Energy
- Progress in Direct Measurements of the Hubble Constant
- The trouble with $H_0$
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
- DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
- DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
- Early dark energy in the pre- and post-recombination epochs
- Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
- Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
- Robustness of dark energy phenomenology across different parameterizations
- Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
- Tests of Evolving Dark Energy with Geometric Probes of the Late-Time Universe
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