Cosmic walls and filaments formation in modified Chaplygin gas cosmology
  We want to study the perturbation growth of an initial seed of an ellipsoidal
shape in Top-Hat collapse model of structure formation in the Modified
Chaplygin gas cosmology. Considering reasonable values of the constants and the
parameters of the model under study, it is shown that a very small deviation
from spherical symmetry (ellipsoidal geometry) in the initial seed leads to a
final highly non-spherical structure which can be considered as a candidate for
justifying already known cosmological structures as cosmic walls and filaments.
