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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 partsof a scalar field. The intial potential system employed is semi classical innature, becoming non-classical at the end of chaotic inflation at the same timecosmological expansion is dominated by the Einstein cosmological constant. Weuse Scherrer's derivation of a sound speed being zero during initialinflationary cosmology, and cange it afterwards as the slope of the scalarfield moves away from a thin wall approximation. All this is to aid in a datareconstruction problem of how to account for the initial origins of CMB due todark matter since effective field theories as presently constructed require acut off value for applicability of their potential structure. This is often atthe cost of, especially in early universe theoretical models, of clearlydefined baryogenesis, and of a well defined mechanism of phase transitions. Thematerial below is now a proposal, in part accepted as a point of discussion asa white paper (appropriately) submitted to the Dark Energy Task Force, in itsmission to advise (through its parent committees) the NSF, NASA and DOE. Thiswas for helping to select both ground-based and space-based techniques foranalyzing data as well as recommending the science requirements for aspace-based dark energy mission.Comment: 38 pages,3 figures. Contains material of a white paper proposal  accepted in June 28,2005, by the DETF committee headed by Dr. Edward Kolb to  review science requirements for a dark energy mission. Combines both a  submitteed white paper to that committee plus the analytical derivation of  the potential suggested in the data reconstruction scheme of this documen

How S-Sʹ Di Quark Pairs Signify an Einstein Constant Dominated Cosmology and Facilitate Reconstruction of Initial Dark Matter Contributions to CMB