Einstein's Equations and a Cosmology with Finite Matter
L. Clavelli, Gary R. Goldstein

TL;DR
This paper explores alternative space-time metrics compatible with Einstein's equations within a cosmology featuring a finite total matter mass, proposing a model where matter density originates as a delta function at the big bang and diffuses outward.
Contribution
It introduces a novel cosmological model with finite total matter, differing from standard big bang assumptions, and analyzes compatible space-time metrics.
Findings
Proposes a finite-mass cosmology with matter originating as a delta function.
Identifies space-time metrics compatible with this finite-mass cosmology.
Challenges standard assumptions about the uniformity of the big bang.
Abstract
We discuss various space-time metrics which are compatible with Einstein's equations and a previously suggested cosmology with a finite total mass. In this alternative cosmology the matter density was postulated to be a spatial delta function at the time of the big bang thereafter diffusing outward with constant total mass. This proposal explores a departure from standard assumptions that the big bang occurred everywhere at once or was just one of an infinite number of previous and later transitions.
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.
