Initial Stage Decay Processes during Cosmic Decoupling

Cosmic decoupling, as a matter formation process, occurs in three stages, beginning with an interaction between cosmic radiation and quark family #3, followed by quark family #2, and then finally by quark family #1. The first two of these interaction sets fail to successfully produce stable baryon matter particles largely because of excessively large quark particle size and lack of adequate cosmic radiation energy levels needed to satisfy baryon particle energy binding requirements. This paper discusses the particular details of the decay processes that cause quark family #3 to fail in its attempt to produce stable hadron particles. Included are: 1) Meson particle decay, 2) Weak Interaction particle decay, 3) Higgs mechanism-based decay, and 4) Quantum based decay of large quark particles.