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

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 w.r.t a semi classical consistency condition 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.