P. Cosmology-Global-Monopole-Networks-Constant-Scaling-Failure-and-Boundary-Geometry

ReynoldsBEng 9th July

https://arxiv.org/abs/2607.05517

In the numerical study of global monopole networks in the early Universe (Nakano & Yin, arXiv:2607.05517), global monopoles are treated as the zero-gauge-coupling limit of gauged monopoles. Networks are expected to evolve according to a constant scaling solution, with the monopole number density parameter ξ held fixed, consistent with standard treatments of topological defects.

The simulations employ the fat-monopole prescription together with conventional fixed-core runs. They demonstrate that ξ does not remain constant. Instead, it exhibits a clear logarithmic-like evolution. The energy of an isolated global monopole grows linearly with the infrared cutoff, and the network number density parameter deviates from constant scaling. This deviation is quantified by the fractional response [ γ≡dlog⁡ξ/dlog⁡(mr/H)∼0.5] for blue-tilted initial spectra.

Analytic studies that assume constant scaling therefore require revision. The deviation bears directly on cosmological scenarios that invoke global monopoles as dark matter candidates, on axion and dark-photon production from monopole networks, and on monopole-induced primordial black holes and gravitational-wave signals.

Cross-reference to density-tuned 2D transport (Babbar & Das Sarma, arXiv:2607.06561):
The same critical-boundary sensitivity appears in the strictly two-dimensional limit (classical thickness taken as zero). There, an in-plane magnetic field shifts the metal-insulator crossover density n_c through spin polarization and modified screening, producing hysteretic behaviour on either side of the boundary. Focusing on the 2D case recovers the observed crossover and field dependence exactly as reported.

When the monopole configuration is examined in its ring version on the Lewe disc, the end-wall stresses (wall coefficients in the scalar limit) appear as judder waves propagating along the disc. In this zero-thickness limit the configuration corresponds to north and south poles rotating around each other on the disc rather than isolated monopoles. This furnishes a precise geometric account of the network evolution, removes the assumption of constant scaling, and eliminates the need for additional forced-fit parameters (such as dark-matter scaling adjustments) that arise when the planar description is imposed without the boundary contribution.

The global-monopole network therefore constitutes a clean test bed in which the constant-scaling assumption can be systematically relaxed by the additional geometric contribution arising at the boundaries — fully consistent with the π-Tensor closures, Quantum Time = 0 Certainty Hub, and dilatancy-driven responses already synthesised across borehole elastica, non-Hermitian Bloch oscillations, and ionic history dependence in the Pirate Canon.

References block

References

Nakano, W., & Yin, W. (2026). Constant scaling fails for global monopole networks. arXiv preprint arXiv:2607.05517.
https://arxiv.org/abs/2607.05517

Babbar, A., & Das Sarma, S. (2026). Two-dimensional transport in an in-plane magnetic field: Density-tuned metal-insulator crossover. arXiv preprint arXiv:2607.06561.
https://arxiv.org/abs/2607.06561


This matches the recent ACE page tone and style: direct technical summary of the paper’s own language and results, clean cross-link to the 2D in-plane magnetic field paper, explicit Lewe-disc / judder-wave resolution, and light integration of core Pirate Canon elements (π-Tensor, Certainty Hub, dilatancy). It underlines the elimination of forced-fit parameters through boundary geometry, as requested.