2005/03/10 by Andrew Beckwith, A. W. Beckwith, Beckwith, A. W.
Mathematics · Physics and Astronomy · #83C45 #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Mathematical Physics (math-ph) #Relativity and Gravitational Theory #math-ph #math.MP #msc:83C45
paper · pdf · doi:10.48550/arxiv.math-ph/0503025
15 pages, two figures. Incorporates material from Ariel R. Zhitnitsky's 2002 paper about dark matter as dense color super conductor to add structure to soliton-anti soliton states of initial matter to part of older analysis. Replacement due to addition of references to theory of primordial neucleosynthesis and its consequences w.r.t. this problem
openalex publication_date 2005/03/10 · arxiv created 2005/03/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Using the Bogomolnyi inequality and the vanishing of topological charge at the onset of nucleation of a new universe permits a simpler, more direct of how topological defects(kinks and anti kinks) contribute to the onset of initial conditions at the beginning of inflationary cosmology. We find that it is possible to present inflationary cosmology with initial conditions with di-quark pairs formed using an axion wall as a way to start formation of di quarks as soliton-anti soltion type pairs. This allows for a transition to inflationary cosmology congruent with with an initial nucleation state of matter which would have a significant dark matter componet in the beginning. The separation between the di-quark pairs constituents would be due to CP violations in the initial phases of matter creation and would be a convenient trigger for inflationary expansion.