The non-linear evolution of a stratified perturbation in a three dimensional expanding Universe is considered. A general Lagrangian scheme (Q model) is introduced and numerical investigations are performed. The asymptotic contraction of the core of the agglomeration is studied. A power-law scaling is detected and an heuristic interpretation of the numerical findings is provided. An asymptotic equation for the multi-stream velocity flow is derived and it is shown to agree quantitatively with the dynamics of the Q model. The relation to the adhesion model is discussed
Basing our discussion on the Lagrangian description of hydrodynamics, we studied the evolution of de...
One of the most interesting challenges of present cosmology concerns the understanding of structure ...
We present a new method to calculate formation of cosmological structure in the Newtonian limit. The...
The non-linear evolution of a stratified perturbation in a three dimensional expanding Universe is c...
The non-linear evolution of a planar perturbation in a three dimensional expanding Universe is cons...
A description of the dynamics of a collisionless, self-gravitating fluid is developed and applied to...
The non-linear evolution of one-dimensional perturbations in a three-dimensional expanding Universe ...
We develop a systematic method to obtain the solution of the collisionless Boltzmann equation which ...
We review the formalism and applications of non-linear perturbation theory (PT) to understanding the...
The growth of density perturbations in an expanding universe in the non-linear regime is investigate...
We develop a path-integral formalism to study the formation of large-scale structures in the univers...
We study an approach to the formation of large-scale structure in the universe based on the descript...
We propose a phenomenological generalization of the models of large-scale structure formation in the...
We introduce the theory of non-linear cosmological perturbations using the correspondence limit of t...
We analyze the performance of a perturbation theory for nonlinear cosmological dynamics, based on th...
Basing our discussion on the Lagrangian description of hydrodynamics, we studied the evolution of de...
One of the most interesting challenges of present cosmology concerns the understanding of structure ...
We present a new method to calculate formation of cosmological structure in the Newtonian limit. The...
The non-linear evolution of a stratified perturbation in a three dimensional expanding Universe is c...
The non-linear evolution of a planar perturbation in a three dimensional expanding Universe is cons...
A description of the dynamics of a collisionless, self-gravitating fluid is developed and applied to...
The non-linear evolution of one-dimensional perturbations in a three-dimensional expanding Universe ...
We develop a systematic method to obtain the solution of the collisionless Boltzmann equation which ...
We review the formalism and applications of non-linear perturbation theory (PT) to understanding the...
The growth of density perturbations in an expanding universe in the non-linear regime is investigate...
We develop a path-integral formalism to study the formation of large-scale structures in the univers...
We study an approach to the formation of large-scale structure in the universe based on the descript...
We propose a phenomenological generalization of the models of large-scale structure formation in the...
We introduce the theory of non-linear cosmological perturbations using the correspondence limit of t...
We analyze the performance of a perturbation theory for nonlinear cosmological dynamics, based on th...
Basing our discussion on the Lagrangian description of hydrodynamics, we studied the evolution of de...
One of the most interesting challenges of present cosmology concerns the understanding of structure ...
We present a new method to calculate formation of cosmological structure in the Newtonian limit. The...