Cosmological Evidence for Dark Axion-Dark Baryon Interactions from Apparent Phantom Crossing
Justin Khoury, Meng-Xiang Lin, Mark Trodden
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-07-17
Comments: Add more references. 13 pages, 6 figures, 3 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Apparent $w<-1$ and a Lower $S_8$ from Dark Axion and Dark Baryons Interactions
- 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
- Early Dark Energy Can Resolve The Hubble Tension
- Acoustic Dark Energy: Potential Conversion of the Hubble Tension
- Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
- The Hubble Tension and Early Dark Energy
- The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration
- Union3.1: Reducing Systematics in Supernova Cosmology with Self-consistent Measurements of Host Galaxy Properties for 2000 Type Ia Supernovae
- Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
- Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
- Dark Energy Constraints from the Cosmic Age and Supernova
- Cosmological Evolution of a Quintom Model of Dark Energy
- Can the dark energy equation-of-state parameter w be less than -1?
- The phantom menaced: constraints on low-energy effective ghosts
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