Using di quark pairs as a way to obtain dark matter near the beginning of nucleation of a new universe

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dc.creatorBeckwith, A. W.
dc.date2005-03-10
dc.date2005-03-13
dc.date.accessioned2026-07-07T04:31:56Z
dc.date.available2026-07-07T04:31:56Z
dc.descriptionUsing 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.
dc.description15 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
dc.identifierhttps://arxiv.org/abs/math-ph/0503025
dc.identifierhttp://arxiv.org/abs/math-ph/0503025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/58003
dc.subjectMathematical Physics
dc.subject83C45
dc.titleUsing di quark pairs as a way to obtain dark matter near the beginning of nucleation of a new universe
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