W. Petry, SPHERICALLY SYMMETRICAL COSMOLOGICAL PERTURBATIONS IN FLAT SPACE-TIMETHEORY OF GRAVITATION, Astrophysics and space science, 235(1), 1996, pp. 41-57
The previously developed equations for the propagation of perturbation
s in a homogeneous, isotropic cosmological model are studied. At the b
eginning of the universe spherically symmetric inhomogeneities can ari
se. In the dust dominated universe the growth of spherically symmetric
perturbations is given in form of infinite series. The increase of th
e inhomogeneity is faster than in general relativity.