Causality and dissipation in relativistic polarizeable fluids
David Montenegro, Giorgio Torrieri

TL;DR
This paper investigates how causality breaks down in relativistic polarizable fluids and proposes a modified framework with dissipation to restore causality, highlighting implications for ferromagnetic materials and spontaneous magnetization.
Contribution
It introduces a relaxation term linking vorticity and polarization to restore causality in relativistic polarizable fluids, providing a new causal Lagrangian near the perfect fluid limit.
Findings
A relaxation term is necessary to restore causality.
A minimum dissipation level is required for causality.
Infrared acausal modes indicate spontaneous magnetization in ferromagnetic materials.
Abstract
We analyze the breakdown of causality for the perfect fluid limit in a medium with polarizeability. We show that to restore causality a relaxation term linking vorticity and polarization, analogous to the Israel-Stewart term linking viscous forces and gradients,is required. This term provides a minimum amount of dissipation a locally thermalized relativistic medium with polarizeability must have, independently of its underlying degrees of freedom. For ferromagnetic materials an infrared acausal mode remains, which we interpret as a Banks-Casher mode signaling spontaneous magnetization. With these ingredients, we propose a candidate for a fully causal Lagrangian of a relativistic polarizeable system near the perfect fluid limit.
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