Numerical magneto-hydrodynamics for relativistic nuclear collisions
Gabriele Inghirami, Luca Del Zanna, Andrea Beraudo, Mohsen Haddadi, Moghaddam, Francesco Becattini, Marcus Bleicher

TL;DR
This paper introduces an enhanced numerical code for relativistic magnetohydrodynamics that models electromagnetic effects in nuclear collisions, providing new insights into magnetic field evolution and its impact on quark-gluon plasma dynamics.
Contribution
The paper presents the first implementation of electromagnetic fields in the ECHO-QGP code for relativistic heavy-ion collisions, enabling self-consistent RMHD simulations of the quark-gluon plasma.
Findings
Magnetic fields in non-central collisions are estimated to be significant.
In ideal RMHD, magnetic fields do not substantially alter elliptic flow.
Further studies are needed to include dissipative effects and initial condition variations.
Abstract
We present an improved version of the ECHO-QGP numerical code, which self-consistently includes for the first time the effects of electromagnetic fields within the framework of relativistic magnetohydrodynamics (RMHD). We discuss results of its application in relativistic heavy-ion collisions in the limit of infinite electrical conductivity of the plasma. After reviewing the relevant covariant formalisms, we illustrate the implementation of the evolution equations in the code and show the results of several tests aimed at assessing the accuracy and robustness of the implementation. After providing some estimates of the magnetic fields arising in non-central high-energy nuclear collisions, we perform full RMHD simulations of the evolution of the Quark-Gluon Plasma in the presence of electromagnetic fields and discuss the results. In our ideal RMHD setup we find that the…
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