1984
DOI: 10.1111/j.1749-6632.1984.tb23387.x
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The Evolution of Voids in the Expanding Universe

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“…On a larger scale still inhomogeneous spacetimes have been used to model clusters of galaxies [Kantowski, 1969a], variations in the Hubble flow due to the supercluster [Mavrides, 1977], the evolution of cosmic voids [Sato, 1984, Hausman et al, 1983, Bonnor and Chamorro, 1990and 1991, the observed distribution of galaxies and simple hierarchical models of the universe [Bonnor, 1972, Wesson, 1978, Wesson, 1979, Ribeiro, 1992a.…”
Section: Modelling Local Non-linearitiesmentioning
confidence: 99%
“…On a larger scale still inhomogeneous spacetimes have been used to model clusters of galaxies [Kantowski, 1969a], variations in the Hubble flow due to the supercluster [Mavrides, 1977], the evolution of cosmic voids [Sato, 1984, Hausman et al, 1983, Bonnor and Chamorro, 1990and 1991, the observed distribution of galaxies and simple hierarchical models of the universe [Bonnor, 1972, Wesson, 1978, Wesson, 1979, Ribeiro, 1992a.…”
Section: Modelling Local Non-linearitiesmentioning
confidence: 99%