Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent
gr-qc, astro-ph.CO
Submitted: 2026-07-27
Updated: 2026-10-12
Comments: 22 pages, 2 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- 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
- How Theory-Informed Priors Affect DESI Evidence for Evolving Dark Energy
- Evolving Dark Energy or Supernovae Systematics?
- Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
- Phantom-Crossing Dark Energy and the m Tug-of-War
- Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply
- Can dark energy evolve to the Phantom?
- Quintom Cosmology: Theoretical implications and observations
- Quintom cosmology and modified gravity after DESI 2024
- Quintessential dark energy crossing the phantom divide
- Interacting Dark Sectors in light of DESI DR2
- Phantom crossing or dark interaction?
- Crossing the phantom divide in scalar-tensor and vector-tensor theories
- Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
- Effective Field Theory, Black Holes, and the Cosmological Constant
- A Model of Holographic Dark Energy
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