A possible solution to the Hubble constant discrepancy — Cosmology where the local volume expansion is driven by the domain average density. (arXiv:1904.09689v1 [gr-qc])

A possible solution to the Hubble constant discrepancy — Cosmology where the local volume expansion is driven by the domain average density. (arXiv:1904.09689v1 [gr-qc])
<a href="http://arxiv.org/find/gr-qc/1/au:+Kasai_M/0/1/0/all/0/1">Masumi Kasai</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Futamase_T/0/1/0/all/0/1">Toshifumi Futamase</a>

The Hubble constant problem is the discrepancy between different measurements
of the Hubble constant in different scales. We show that this problem can be
resolved within the general relativistic framework of the perturbation theory
in the inhomogeneous universe, with the help of spatial averaging procedure
over a finite local domain in the $t=mbox{const.}$ hypersurface.

The Hubble constant problem is the discrepancy between different measurements
of the Hubble constant in different scales. We show that this problem can be
resolved within the general relativistic framework of the perturbation theory
in the inhomogeneous universe, with the help of spatial averaging procedure
over a finite local domain in the $t=mbox{const.}$ hypersurface.

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