Distinguishes Wilson holonomy from spectral monodromy in spin-orbit rings and maps the Hamiltonian to effective U(1) plus non-Abelian connections for two explicit ring models.
Modeling space plasma dynamics with anisotropic Kappa distributions
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abstract
Space plasmas are collisionpoor and kinetic effects prevail leading to wave fluctuations, which transfer the energy to small scales: wave-particle interactions replace collisions and enhance dispersive effects heating particles and producing suprathermal populations observed at any heliospheric distance in the solar wind. At large distances collisions are not efficient, and the selfgenerated instabilities constrain the solar wind anisotropy including the thermal core and the suprathermal components. The generalized power-laws of Kappa-type are the best fitting model for the observed distributions of particles, and a convenient mathematical tool for modeling their dynamics. But the anisotropic Kappa models are not correlated with the observations leading, in general, to inconsistent effects. This review work aims to reconcile some of the existing Kappa models with the observations.
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2026 1verdicts
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Wilson Holonomy and Spectral Monodromy in Spin-Orbit Rings: Effective Gauge Connections and Loop Observables
Distinguishes Wilson holonomy from spectral monodromy in spin-orbit rings and maps the Hamiltonian to effective U(1) plus non-Abelian connections for two explicit ring models.