Speaker
Description
Relativistic heavy-ion collisions generate strong electromagnetic fields that interact with the conducting quark-gluon plasma (QGP), motivating a description based on relativistic resistive magnetohydrodynamics (RRMHD). We present M-SHIVA 1.0, a finite-volume RRMHD framework designed for heavy-ion collision studies. The coupled 14-equation system is evolved using an HLL shock-capturing scheme with IMEX Runge-Kutta time integration to handle the stiffness associated with high electrical conductivity, while the magnetic-field divergence constraint is controlled using the GLM formulation. The code is validated through Brio-Wu, cylindrical blast, Cartesian rotor, and Milne rotor tests, covering resistive to nearly ideal-MHD regimes. For heavy-ion applications, optical-Glauber profiles are used for the initial QGP energy density, with electromagnetic fields generated by spectator protons. We study the resulting spatial, momentum anisotropy and Joule heating for RHIC- and LHC-like conditions. While finite conductivity significantly affects electromagnetic-field evolution, the irreversible Joule heating remains smaller than the cooling due to longitudinal expansion for the systems considered.