A General Relativistic Rotating Evolutionary Universe - Part II

TL;DR

This paper extends previous work by introducing generalized Gaussian metrics to model a rotating universe within general relativity, modifying standard cosmological metrics and making testable predictions.

Contribution

It develops a new class of metrics to incorporate universal rotation, expanding the mathematical framework of cosmological models.

Findings

Rotation of the universe can be modeled with generalized Gaussian metrics.

The modified metrics alter the standard Robertson-Walker form.

Experimental predictions are proposed based on the new models.

Abstract

As a sequel to (Berman, 2008a), we show that the rotation of the Universe can be dealt by generalised Gaussian metrics, defined in this paper. Robertson-Walker's metric has been employed with proper-time, in its standard applications; the generalised Gaussian metric imply in the use of a non-constant temporal metric coefficient modifying Robertson-Walker's standard form. Experimental predictions are made