ABSTRACT The KBC void is a local underdensity with the observed relative density contrast δ ≡ 1 − ρ/ρ0 = 0. 46 ± 0. 06 between 40 and 300 Mpc around the Local Group. If mass is conserved in the Universe, such a void could explain the 5. 3σ Hubble tension. However, the MXXL simulation shows that the KBC void causes 6. 04σ tension with standard cosmology (ΛCDM). Combined with the Hubble tension, ΛCDM is ruled out at 7. 09σ confidence. Consequently, the density and velocity distribution on Gpc scales suggest a long-range modification to gravity. In this context, we consider a cosmological MOND model supplemented with 11 \, eV/c^2 sterile neutrinos. We explain why this νHDM model has a nearly standard expansion history, primordial abundances of light elements, and cosmic microwave background (CMB) anisotropies. In MOND, structure growth is self-regulated by external fields from surrounding structures. We constrain our model parameters with the KBC void density profile, the local Hubble and deceleration parameters derived jointly from supernovae at redshifts 0. 023−0. 15, time delays in strong lensing systems, and the Local Group velocity relative to the CMB. Our best-fitting model simultaneously explains these observables at the 1. 14{\ per\ cent} confidence level (2. 53σ tension) if the void is embedded in a time-independent external field of 0. 055 \, a䃐. Thus, we show for the first time that the KBC void can naturally resolve the Hubble tension in Milgromian dynamics. Given the many successful a priori MOND predictions on galaxy scales that are difficult to reconcile with ΛCDM, Milgromian dynamics supplemented by 11 \, eV/c^2 sterile neutrinos may provide a more holistic explanation for astronomical observations across all scales.
Haslbauer et al. (Thu,) studied this question.