Hubble tension in k-essence: Evidence for robust tension alleviation
Isaac Opio, Didam Duniya, Bishop Mongwane, Hassan Abdalla
BIUST · BIUST · Cape Town · NWU and Omdurman
astro-ph.CO
Submitted: 2026-07-03
Comments: 18 pages, 5 figures (Abstract here is adjusted to comply with arXiv limit.)
Code: https://github.com/PantheonPlusSH0ES/DataRelease
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- 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
- The Megamaser Cosmology Project. II. The Angular-Diameter Distance to UGC 3789
- H0LiCOW I. $H_0$ Lenses in COSMOGRAIL's Wellspring: Program Overview
- In the Realm of the Hubble tension $-$ a Review of Solutions
- Hubble Tension: The Evidence of New Physics
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- The Hubble tension: A decade review
- Testing the cosmological principle with the Pantheon+ sample and the region-fitting method
- The Expansion of the Universe is Faster than Expected
- Tensions between the Early and the Late Universe
- JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0
- The Perfect Host: JWST Cepheid Observations in a Background-Free SN Ia Host Confirm No Bias in Hubble-Constant Measurements
- Dissecting the Hubble tension: Insights from a diverse set of Sound Horizon-free H0 measurements
- The Hubble Hunter's Guide
- Early Dark Energy Can Resolve The Hubble Tension
- Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
- Scaling solutions as Early Dark Energy resolutions to the Hubble tension
- Alleviating $H_0$ and $S_8$ Tensions Simultaneously in K-essence Cosmology
- Comprehensive Study of $k$-essence Model: Dynamical System Analysis and Observational Constraints from Latest Type Ia Supernova and BAO Observations
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