Abstract
The initial state of the cosmos is analytically modeled as a radiation filled spherical cavity that expands from a singularity to later act as a clock and energy source in support of a 3-stage, radiation to a quark-hadron based, decoupling process. The model thereby avoids a need for Inflation and the presence of matter at start-up and during the radiation dominated phase, but nevertheless remains strongly consistent with attributes of the Guth Inflationary model. At decoupling, only quark family #1 with up-down attributes has adequate energy to successfully complete decoupling. Earlier in a 3-stage process, attempts at hadronization by quark families #2 and #3 fail due to large quark size and binding energy requirements that exceed the available radiation energy supply. These attempts decay rapidly to take a quark family #1 form. Decoupling is further modeled as half-spin based radiation resonance forms that are linked, via particle time dilation, to matter based micro-black-holes.
Highlights
A recently published paper on quark family attributes allows one to see more clearly their impact on cosmic evolution and decoupling.[1] The following chart (Table 1) where J is total angular momentum, B is baryon number, Q is electric charge, and I3 is Isospin summarizes a list of relevant observed quark attributes from that paper which will be used here to analyze the role of quarks at various stages of cosmic development
The foregoing presentation begins with an analysis of observed quark attributes to determine what impact they might have on cosmic evolution and decoupling
It is shown thereby that cosmic decoupling can only occur when cosmic radiation frequency corresponds to approximately 2.27 ̽ 1023 Hz
Summary
A recently published paper on quark family attributes allows one to see more clearly their impact on cosmic evolution and decoupling. Note that an isolated neutron particle set only has a life span of 889 seconds [2] due to Beta decay By comparison, both the Charm-Strange family and especially the Top-Bottom family have significantly shorter life spans [3, 4, 5, 6] and can be viewed as failed attempts to successfully hadronize during a 3-stage cosmic decoupling process. In this regard, see the lepton life spans listed below in a second associated chart (Table 2) that summarizes the spin-1⁄2 lepton family particle attributes that are part of the atomic particle set that includes the above defined quark families. See the lepton life spans listed below in a second associated chart (Table 2) that summarizes the spin-1⁄2 lepton family particle attributes that are part of the atomic particle set that includes the above defined quark families. [7] The lepton life span data listed here gives a close approximation of the Charm-Strange and Top-Bottom quark family group attributes during hadronization attempts
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