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
Unique-IP document downloads: 37 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.