Observational constraints on scalar-vector-tensor dark energy with phantom-divide crossing
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-09-25
Updated: 2026-09-25
Terminology
Sources
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- The Cosmological Constant and Dark Energy
- Dynamics of dark energy
- Approaches to Understanding Cosmic Acceleration
- Modified Gravity and Cosmology
- Quintessence: A Review
- Beyond the Cosmological Standard Model
- Cosmological Tests of Modified Gravity
- Beyond $\Lambda$CDM: Problems, solutions, and the road ahead
- A systematic approach to generalisations of General Relativity and their cosmological implications
- Dark energy in Horndeski theories after GW170817: A review
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
- 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
- Extended Dark Energy analysis using DESI DR2 BAO measurements
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