Can cosmic voids ease the Hubble tension? Local expansion in w 0w a CDM
Tommaso Moretti, Noemi Frusciante, Giovanni Verza
astro-ph.CO, gr-qc
Submitted: 2026-07-22
Comments: 22 pages, 11 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- 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
- Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
- Planck 2018 results. VI. Cosmological parameters
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- In the Realm of the Hubble tension $-$ a Review of Solutions
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
- Evolving Dark Energy or Supernovae Systematics?
- A Local Hubble Bubble from SNe Ia?
- Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2
- Evidence for a ~300 Mpc Scale Under-density in the Local Galaxy Distribution
- The Local Hole revealed by galaxy counts and redshifts
- Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
- Confronting Lemaitre-Tolman-Bondi models with Observational Cosmology
- Rendering Dark Energy Void
- Testing the Copernican principle by constraining spatial homogeneity
- Probing spatial homogeneity with LTB models: a detailed discussion
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