Evolution of matter perturbations in the context of cosmic slowing down
gr-qc, astro-ph.CO
Submitted: 2026-08-05
Updated: 2026-08-05
Comments: 22 pages, 5 tables, 15 figures, to appear in MPLA
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck and the local Universe: quantifying the tension
- Does the Hubble constant tension call for new physics?
- Planck 2015 results. XIII. Cosmological parameters
- Planck 2018 results. VI. Cosmological parameters
- A 2.4% Determination of the Local Value of the Hubble Constant
- Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
- A Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck
- Conjoined constraints on modified gravity from the expansion history and cosmic growth
- Cosmology Intertwined III: $f \sigma_8$ and $S_8$
- Early Dark Energy Can Resolve The Hubble Tension
- Can scale-dependent cosmology alleviate the $H_0$ tension?
- Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data
- Evolution of the $f\sigma_8$ tension with the Planck15/$\Lambda$CDM determination and implications for modified gravity theories
- Hints of Modified Gravity in Cosmos and in the Lab?
- Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
- Growth of structures and redshift-space distortion data in scale-dependent gravity
- Challenges for $\Lambda$CDM: An update
- Anomalies in Physical Cosmology
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Model independent cosmographic constraints from DESI 2024
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