General Relativistic Dynamics of Irrotational Dust: Cosmological Implications
Astrophysics
2009-10-22 v1
Abstract
The non--linear dynamics of cosmological perturbations of an irrotational collisionless fluid is analyzed within General Relativity. Relativistic and Newtonian solutions are compared, stressing the different role of boundary conditions in the two theories. Cosmological implications of relativistic effects, already present at second order in perturbation theory, are studied and the dynamical role of the magnetic part of the Weyl tensor is elucidated.
Keywords
Cite
@article{arxiv.astro-ph/9310036,
title = {General Relativistic Dynamics of Irrotational Dust: Cosmological Implications},
author = {Sabino Matarrese and Ornella Pantano and Diego Saez},
journal= {arXiv preprint arXiv:astro-ph/9310036},
year = {2009}
}
Comments
12 pages , DFPD 93/A/67