Astrophysics

    

A Model of a Gravitational Flux Tube Between Two Stars

Authors: Kurt Becker

Astronomers are observing fast radio bursts. Some of these may be due to viewing flux tubes between stars. The narrow cones of space-time between two distant stars have a very special geometry. This geometry results in bending geodesics towards the line-of-centers between these two stars which results in increasing gravity between these two stars. This paper may provide a mathematical model to explain the empirical equation of Modified Newtonian Dynamics. The hypothesis of gravitational flux tubes between stars also predicts a great increase in brightness when stars are viewed less than one milli arc-sec from the line-of-center between our Sun and that star. Pointing a telescope within one milli-arc sec is currently impossible to achieve. It can only be accidentally passed through and since the Earth rotates, viewing will only last for milli seconds.

Comments: 23 Pages.

Download: PDF

Submission history

[v1] 2021-08-26 16:24:56
[v2] 2021-09-11 13:03:07
[v3] 2022-05-31 17:59:38

Unique-IP document downloads: 229 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.

comments powered by Disqus