Authors: Kurt L. Becker
Abstract This paper attempts to give a theoretical foundation for the Modified Newtonian Dynamics equations developed by M. Milgrom Ref.1. It will show that there is a cross sectional limit, below which 1/r2 asymptotically changes to 1/r. When the cross section of a distant star falls below the cross section of a particle transmitting the gravitational force, such as a graviton, as viewed from a baryon, such as a proton, then the inverse square law is no longer valid. Gravitational attraction then depends on the distance travelled by the particle and will result in the force of gravity varying as 1/r. It is only the relative geometries which limit the inverse square law. The sizes of the suns and particles involved will only result in different limits and will not change the basic outcome of 1/r.
Comments: 8 Pages. This paper attempts to give a theoretical foundation for the MOND equations.
[v1] 2019-01-19 14:53:31
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.