Relativity and Cosmology

    

Scale Dependence and the Relational Properties of Mass

Authors: Christopher R. Brown

Homogeneity is inconsistent with general covariance, yet remains necessary given the practical limitations of solving Einstein's field equations. We resolve this contradiction using a scale-dependent density profile. In this view, empty points have no ontological standing and the geometry of spacetime exists only as an abstract network of physical relationships. Gravitational boundaries are considered to be coordinate artifacts rather than physical partitions. Our solution naturally derives the Hubble constant and the CMB temperature with no adjustable parameters. A single coupling constant $kapprox .833 kg/m^2$ connects the surface area of the horizon(s) to the density distribution. The result is a stable, static and infinite cosmological model capable of explaining a wide range of phenomena.

Comments: 8 Pages.

Download: PDF

Submission history

[v1] 2025-05-14 17:24:33

Unique-IP document downloads: 94 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