Abstract

We report on the time evolution of a charged strongly coupled N = 4 SYM plasma with an axial anomaly subjected to strong electromagnetic fields. The evolution of this plasma corresponds to a fully backreacted asymptotically AdS5 solution to the Einstein-Maxwell-Chern-Simons theory. We explore the evolution of the axial current and production of axial charges. As an application we show that after a sufficiently long time both the entropy and the holographic entanglement entropy of a strip-like topology (both parallel to and transverse to the flow of axial current) grow linearly in time.

Highlights

  • We report on the time evolution of a charged strongly coupled N = 4 SYM plasma with an axial anomaly subjected to strong electromagnetic fields

  • In this work we compute for the first time the dynamical evolution of a charged strongly coupled far from equilibrium plasma with a chiral anomaly subjected to external electromagnetic fields

  • We have displayed the axial current density in the simplest dynamical setup possible to capture the evolution of the current generated due to the axial anomaly during the isotropization of a plasma

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Summary

Holographic description

We employ the characteristic formulation of general relativity first formulated in [59, 60] and implemented in a myriad of subsequent publications for the study of dynamical systems in asymptotically anti-de-Sitter spacetime (some examples [33,34,35,36,37,38,39,40,41,42, 49, 52]). When the Chern-Simons term is not present the integration constant ρ can be interpreted as the axial charge density (see eq (2.38)) This contribution to the total axial charge is a constant throughout the evolution and we are free to set this quantity to zero if we choose. The full equations are included in appendix C Inspecting these equations one finds that eq (2.13a) is no longer a linear ODE, the first equation of the nested list structure has developed a non-linearity by the inclusion of the Chern-Simons term and requires two pieces of initial data, the anisotropy profile at the initial time v0, B(v0, r), and the bulk electric field profile P (v0, r). As proven to be a valid regularization procedure in [58]

Asymptotic analysis
Numerical techniques
Results
Summary and discussion
A Scaling relations
B Residual symmetries
C Equations of motion
Full Text
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