Perturbative Approximations to the Evolution of Plane Symmetric Cosmological Structures
The two main perturbative schemes for the non-linear evolution of large-scale structures are the Lagrangian and the Eulerian ones. The former has been set as a much more powerful technique, due to its property of yielding the exact solution in the plane-symmetric case. We have applied the Eulerian scheme to this plane symmetric case and have
Raposo, A. P. et al.
Fecha de publicación:
12
1998