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

A. W. Beckwith
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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.

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A. W. Beckwith. 2005-11-15. How soliton-anti soliton di quark pairs signify an Einstein constant dominated cosmology, and lead to new inflationary cosmology physics. https://arxiv.org/abs/gr-qc/0511081

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