Probing the sound speed and clustering of dark energy
astro-ph.CO
Submitted: 2025-11-27
Updated: 2026-06-30
Comments: 14 pages, 8 figures
Journal ref: Sci.Bull. 71 (2026) 4410-4415
DOI: 10.1016/j.scib.2026.08.004
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- Dark Energy Constraints from the Cosmic Age and Supernova
- Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
- Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
- Evolving Dark Energy or Supernovae Systematics?
- The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration
- Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
- Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
- Preference for evolving dark energy in light of the galaxy bispectrum
- Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
- Apparent $w<-1$ and a Lower $S_8$ from Dark Axion and Dark Baryons Interactions
- Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
- Quintom Cosmology: Theoretical implications and observations
- Can dark energy evolve to the Phantom?
- Cosmological Evolution of a Quintom Model of Dark Energy
- Two-field Models of Dark Energy with Equation of State Across -1
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation