On the necessity of the revisions for the cosmological matter perturbations from the general relativity

Details On the necessity of the revisions for the cosmological matter perturbations from the general relativity On the necessity of the revisions for the cosmological matter perturbations from the general relativity

2011-05-07

arxiv.org/abs/1105.1419v2

Phys.Rev.D83:124040,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

8 pages, LaTeX; the arguments in section 3 are corrected and the results are changed

Scientific paper

10.1103/PhysRevD.83.124040

The differential equations, which are used for matter perturbations, are usually derived from the Newton gravity and the Euler equation in the expanded universe. In this paper, by the explicit calculations of metric perturbation theory in $\Lambda$CDM model, we derive the general relativistic corrections exactly for the equations and show that the differential equations derived from the Newton gravity and the Euler equation are valid in the small scale region from non-relativistic matter dominant era onwards. However the corrections are not negligible in radiation dominant era.

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