The isotropy and the homogeneity of the universe were postulated in the form of the `` cosmological principle '' by Einstein, then by Friedmann and Lemaître. They were introduced on primarily philosophical bases (the ground does not occupy a place privileged in the universe). The recent observations came to give a justification a posteriori .
One can thus consider with a good approximation which the universe is maximalement symmetrical. One can show (weinberg1972, chapter 13) that for this type of geometry, the metric one is written in polar co-ordinates:
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(1.2) |
One often expresses .
If the following co-ordinates are introduced:
then one can rewrite the metric one in the form:
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(1.3) |
In this frame of reference, an object whose co-ordinates
remain constant in the course of time is motionless, made abstraction
of the general expansion of the universe which is included/understood
in the factor
.
The most remarkable property of this metric is that it introduces naturally, through the scale factor, the dynamics of the universe. The universe can be expanding or contraction.