  We assume a one-to-one correspondence between comoving coordinates and the
cosmic rest frame in a spherically symmetric inhomogeneous universe. This
strongly restricts the solutions of Einstein's equations: (i) The pressure must
be zero. (ii) The metric does not depend on the radial coordinate, the FLRW
cosmology is excluded (strong homogeneity). (iii) The unique solution
corresponds to the Datt-Ruban solution. Beside the Hubble constant it contains
one free constant of integration which can be chosen in order to represent the
measured Hubble diagram without using a cosmological constant.

General Physics;General Relativity and Quantum Cosmology