Homogeneous spheroidal voids in ΛCDM become only slightly rounder, deviate from linear theory by z≈8, and retain substantial matter density μ>0.5 independent of eccentricity.
Bertschinger,The self-similar evolution of holes in an Einstein-de Sitter universe,ApJS58 (1985) 1
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A semi-analytical approach to cosmic void evolution
Homogeneous spheroidal voids in ΛCDM become only slightly rounder, deviate from linear theory by z≈8, and retain substantial matter density μ>0.5 independent of eccentricity.