Gravitational Clustering to All Perturbative Orders

Details Gravitational Clustering to All Perturbative Orders Gravitational Clustering to All Perturbative Orders

1998-11-08

arxiv.org/abs/astro-ph/9811119v1

Braz.J.Phys.31:42-44,2001

Astronomy and Astrophysics

Astrophysics

3 pages, revtex

Scientific paper

We derive the time evolution of the density contrast to all orders of perturbation theory, by solving the Einstein equation for scale-invariant fluctuations. These fluctuations are represented by an infinite series in inverse powers of the radial parameter. In addition to the standard growing modes, we find infinitely many more new growing modes for open and closed universes.

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