The Universe expansion and Energy problems
Moukaddem Nazih

TL;DR
This paper develops a physical model of universe expansion using a time-dependent Riemannian space, unifying various physics principles and constants, and providing insights into the universe's age, size, and energy.
Contribution
It introduces a novel model that unifies classical and modern physics by incorporating time-dependent constants and adapting general relativity to describe universe expansion.
Findings
The universe's size and age are determined within the model.
Only total energy, electromagnetic constant, and speed of light are universal constants.
Other fundamental constants are time-dependent and related to these constants.
Abstract
In this paper we construct a physical modelization of the universe expansion. The universe then reduces to a Riemannian space , where for 0, and is a time - dependent Riemannian metric which reflects and characterizes the dynamical matter - energy distribution on according to the Mach - Einstein principle. Our model allows us to resolve several major problems of Physics. It is consistent in the sense that all Newtonian and classical physical laws are valid as particular cases in classical situations. Moreover, our model permits to recover some confirmed principles and postulates such as the famous Einstein's relationship and to specify some approximate results of modern Physics. After showing, rigorously, the deficiency of the second part of the special relativity second postulate and after specifying…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Advanced Mathematical Theories and Applications
