Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
gr-qc, astro-ph.CO
Submitted: 2026-09-15
Updated: 2026-09-15
Comments: Matches published version
Journal ref: Phys. Lett. B 881 (2026) 140877
DOI: 10.1016/j.physletb.2026.140877
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Mapping Luminosity-Redshift Relationship to LTB Cosmology
- An inhomogeneous alternative to dark energy?
- Chandra X-ray Spectroscopic Imaging of Sgr A* and the Central Parsec of the Galaxy
- A point mass in an isotropic universe: III. The region $R\leq 2m$
- A point mass in an isotropic universe. Existence, uniqueness and basic properties
- Quasi-Local Gravitational Energy
- On singularities, horizons, invariants, and the results of Antoci, Liebscher and Mihich (GRG 38, 15 (2006) and earlier)
- Anisotropies in the Cosmic Microwave Background: An Analytic Approach
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Phantom Energy and Cosmic Doomsday
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