Renormalization group corrections to CDM model and observational consequences for H 0 tension
astro-ph.CO, gr-qc, hep-th
Submitted: 2025-09-28
Updated: 2026-09-11
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
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Elastic, dielectric and piezoelectric anomalies and Raman spectroscopy of 0.5Ba(Ti0.8Zr0.2)O3-0.5(Ba0.7Ca0.3)TiO3
- Interacting dark energy with time varying equation of state and the $H_0$ tension
- A novel approach to cosmological non-linearities as an effective fluid
- The matter with(in) CPL
- The Hubble Tension and Early Dark Energy
- Early Dark Energy Can Resolve The Hubble Tension
- On the non-local heat kernel expansion
- Form factors and decoupling of matter fields in four-dimensional gravity
- Nonlocality of quantum matter corrections and cosmological constant running
- Running G and \Lambda at low energies from physics at M_X: possible cosmological and astrophysical implications
- Cosmic perturbations with running G and Lambda
- Renormalization group scale-setting in astrophysical systems
- Scale-dependent gravity and covariant scale-setting
- Dynamics of the Laplace-Runge-Lenz vector in the quantum-corrected Newton gravity
- Effective Action of Vacuum: Semiclassical Approach
- Scale-dependent cosmology from effective quantum gravity in the invariant framework
- Cobaya: Code for Bayesian Analysis of hierarchical physical models
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