Authors: Ernst Schmutzer
In this paper the behaviour of a matter torus under the influence of the expanding cosmos model (according to our theory PUFT) is investigated. This task can numerically be treated for the full life time of the cosmos model (from the Urstart to the Finish). As we know from our literature cited, the graphic course of the cosmological scalaric field after the Urstart exhibits an increase , followed by a return down to the Finish. This curious behaviour of the cosmological scalaric field leads to the suspicion that the shape of the torus during the life time of the cosmos may be: sphere at the Urstart, transformation of the sphere to a ring with decreasing thickness, return to a sphere at the Finish. It seems that such a theoretically predicted physical effect could perhaps exist in Nature. The torus was chosen as a test object, since the numerical calculations can be done without approximation procedures. We took this rather simple example to show this cosmological effect for further applications in astrophysics.
Comments: 11 Pages.
[v1] 2017-09-09 10:15:41
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