Theoretical analysis reveals an accessible magnetic monopole mass of 10^8 GeV via topological defects, suggesting viable detection in particle colliders and cosmic rays.
This paper derives the magnetic monopole as a topological defect of the string-magnetic mode χstring^M and calculates its mass as a function of the coarse-graining scale L_c, yielding an experimentally accessible window distinct from GUT predictions. The winding number w_M = 1/2π∮ ∇CG^M · dl ∈ Z is shown to be a topological invariant of the first-space meta-field. When w_M ≠ 0, the coarse-graining operator ĈL_c(M) cannot smooth the knot, producing a residual δ-function magnetic charge. The mass formula mₘₒₙₒ(L_c) = αmag MPl(lstring/L_c)^2 gives mₘₒₙₒ ~ 10^8 GeV for L_c ~ 10⁻²⁰ m, within reach of cosmic-ray and heavy-ion collision searches. Two detection channels are proposed: transient magnetic charge signals in Pb-Pb collisions at √{sNN} = 5.5 TeV, and galactic magnetic field deflection anomalies in ultra-high-energy cosmic rays.
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kimik3,单洁,X. Ma, Independent Researcher, Institute for First-Space Ontology and Emergent Physics Email: maexiang@163.com; 15552786932@139.com; maexiang2026@Outlook.com (2026) studied this question.
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