Metric of Kasner

The metric of Kasner is a particular form of metric introduced by the physicist Kasner in 1921 to study the anisotropic models of universe.

The metric one is given by the following equation:

g_ {ij} = ds^2 = - dt^2 + t^ {2 p_1} dx^2 + t^ {2 p_2} dy^2 + t^ {2 p_3} dz^2

The parameters of metric, (p_1, p_2, p_3) check the following conditions:

p_1 + p_2 + p_3 = {p_1} ^2 + {p_2} ^2 + {p_3} ^2 = 1

Immediate properties

The condition on the value of the parameters implies that one of them is negative (except in the commonplace case where one of them is equal to 1 and the two others to zero). Indeed: (p_1 + p_2 + p_3) ^2 = {p_1} ^2 + {p_2} ^2 + {p_3} ^2 + 2 p_1 p_2 + 2 p_1 p_3 + 2 p_2 p_3 from where: p_1 p_2 + p_1 p_3 + p_2 p_3 = 0 , condition which cannot be carried out if all the p_i are positive. It is shown that (for example): - \ frac {1} {3} < p_1 < 0 .

The elementary element of volume in this metric has as a measurement \ sqrt {- G} = T . The universe describes by this metric is thus expanding. However, owing to the fact that at least of the p_i is negative, this expansion is transformed into contraction in one of the directions.

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