Authors: Bernard Riley
By application of the 10D/4D correspondence, the radii of nearby stars have been shown to map onto the masses of stable atomic nuclei. The correspondence is now used to calculate the mass m and radius r of the subatomic object that corresponds to a typical 1.4 solar mass neutron star. The mass m is found to be 4.0 TeV. Using natural units, r/m is precisely 2.
Comments: 8 Pages.
[v1] 2017-07-12 03:52:25
Unique-IP document downloads: 33 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.