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Spacetime dynamics of chiral magnetic currents in a hot non-Abelian plasma

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arxiv 2308.14825 v2 pith:5FY3I6VM submitted 2023-08-28 hep-ph hep-thnucl-th

Spacetime dynamics of chiral magnetic currents in a hot non-Abelian plasma

classification hep-ph hep-thnucl-th
keywords chiralcorrelationsdynamicsfluctuationsnon-abelianplasmaspatialtopological
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The correlations of electric currents in hot non-Abelian plasma are responsible for the experimental manifestations of the chiral magnetic effect (CME) in heavy-ion collisions. We evaluate these correlations using holography, and show that they are driven by large-scale topological fluctuations. In a non-Abelian plasma with chiral fermions, local axial charge can be generated either by topological fluctuations (creating domains with nonzero Chern-Simons number) or by thermal fluctuations. Within holography, we investigate the dynamical creation of the axial charge and isolate the imprint of the topological dynamics on the spatial correlations of electric current. In particular, we show that the spatial extent of the current correlation is quite large ($\sim 1\ {\rm fm}$) and grows with time, which is consistent with sphaleronlike dynamics. We provide numerical estimates for this spatial size that can be used as an input in phenomenological analyses.

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    A driven holographic Weyl semimetal supports a stable nonequilibrium steady state, becomes superharmonic and then chaotic at stronger driving, and exhibits strong-coupling chiral pumping in a magnetic field.