The shear dynamics in Bianchi I cosmological model on the brane

Details The shear dynamics in Bianchi I cosmological model on the brane The shear dynamics in Bianchi I cosmological model on the brane

2001-03-26

arxiv.org/abs/gr-qc/0103093v2

Class.Quant.Grav. 18 (2001) 2311-2316

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, no figures; some comments and references added; submitted to Class. Quant. Gravity

Scientific paper

10.1088/0264-9381/18/12/306

The shear dynamics in Bianchi I cosmological model on the brane with a perfect fluid (the equation of state is $p=(\gamma-1) \mu$) is studied. It is shown that for $1 < \gamma < 2$ the shear parameter has maximum at some moment during a transition period from nonstandard to standard cosmology. An exact formula for the matter density $\mu$ in the epoch of maximum shear parameter as a function of the equation of state is obtained.

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