On emergent particles and stable neutral plasma balls in SU(2) Yang-Mills thermodynamics
Thierry Grandou, Ralf Hofmann

TL;DR
This paper investigates the properties of stable neutral plasma balls and emergent particles in SU(2) Yang-Mills thermodynamics, revealing their structure, charge, and oscillation frequencies in the deconfining phase.
Contribution
It introduces a detailed model of vortex-loop self-intersections and monopole cores, correcting previous estimates and linking these structures to plasma oscillations in SU(2) Yang-Mills theory.
Findings
The vortex-loop self-intersection region carries one unit of electric charge.
Monopole core vibrations occur at a specific thermodynamic frequency.
Neutral plasma oscillates slower than plasma with a trapped monopole.
Abstract
For a pure SU(2) Yang-Mills theory in 4D we revisit the spatial (3D), ball-like region of radius , in its bulk subject to the pressureless, deconfining phase at where denotes the critical temperature for the onset of the deconfining-preconfining phase transition. Such a region possesses of a finite energy density and represents the self-intersection of a figure-eight shaped center-vortex loop if a BPS monopole of core radius , isolated from its antimonopole by repulsion externally invoked through a transient shift of (anti)caloron holonomy (pair creation), is trapped therein. The entire soliton (vortex line plus region of self-intersection of mass containing the monopole) can be considered an excitation of the pressureless and energyless ground state of the confining phase. Correcting an earlier estimate of , we show that the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsQuantum Chromodynamics and Particle Interactions · High-Energy Particle Collisions Research · Ionosphere and magnetosphere dynamics
