This method simulates quark-gluon plasma behaviors in heavy-ion collisions, suggesting advancements in understanding high-energy physics.
We present bhac-qgp, a new numerical code to simulate the evolution of matter created in heavy-ion collisions in the presence of electromagnetic fields. It is derived from the Black Hole Accretion Code (BHAC), which has been designed to model astrophysical processes in a general-relativistic magnetohydrodynamical description. As the original Black Hole Accretion Code, BHAC QGP benefits from the use of adaptive mesh refinement, which allows us to dynamically adjust the resolution where necessary and makes use of time-dependent Milne coordinates and the ultrarelativistic equation of state, ๐=๐/3. We demonstrate that bhac-qgp accurately passes a number of systematic and rigorous tests.
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Mayer et al. (2025) studied this question.
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