How soliton-anti soliton di quark pairs signify an Einstein constant dominated cosmology, and lead to new inflationary cosmology physics

TL;DR

This paper explores a model where soliton-anti soliton diquark pairs in scalar fields relate to an Einstein constant dominated universe, proposing new insights into inflationary physics and the origins of cosmic microwave background features.

Contribution

It introduces a novel model linking diquark soliton pairs to cosmological inflation and the Einstein constant, addressing initial universe nucleation and CMB origins.

Findings

Sound speed approaches unity during inflation.

Scalar field potential changes affect nucleation conditions.

Model suggests a link between diquark pairs and dark matter origins.

Abstract

We review the results of a model of how nucleation of a new universe occurs, assuming a di quark identification for soliton-anti soliton constituent parts of a scalar field. Initially, we employ a false vacuum potential system; however ,when cosmological expansion is dominated by the Einstein cosmological constant at the end of chaotic inflation, the initial di quark scalar field is not consistent with respect to a semi classical consistency conditions we analyze as the potential changes to the chaotic inflationary potential utilized by Guth. We use Scherrer's derivation of a sound speed being zero during initial inflationary cosmology, and obtain a sound speed approaching unity as the slope of the scalar field moves away from a thin wall approximation. All this is to aid in a data reconstruction problem of how to account for the initial origins of CMB due to dark matter since effective field theories as presently constructed require a cut off value for applicability of their potential structure. This is often at the cost of, especially in early universe theoretical models, of clearly defined baryogenesis, and of a well defined mechanism of phase transitions.