Electromagnetic fields from the extended Kharzeev-McLerran-Warringa model in relativistic heavy-ion collisions
Yi Chen, Xin-Li Sheng, Guo-Liang Ma

TL;DR
This paper extends the Kharzeev-McLerran-Warringa model to include longitudinal position dependence, medium effects, and realistic QGP evolution, providing more accurate estimates of electromagnetic fields in relativistic heavy-ion collisions.
Contribution
It introduces generalized formulas for electromagnetic fields in vacuum and QGP medium, incorporating position dependence, charge distributions, retardation, and time-dependent conductivity, improving modeling accuracy.
Findings
Magnetic field evolution is slower and more realistic with the extended model.
Medium effects prolong magnetic field duration, aligning with experimental polarization data.
The model is useful for studying electromagnetic phenomena at various collision energies.
Abstract
Based on the Kharzeev-McLerran-Warringa (KMW) model that estimates strong electromagnetic (EM) fields generated in relativistic heavy-ion collisions, we generalize the formulas of EM fields in the vacuum by incorporating the longitudinal position dependence, the generalized charge distributions and retardation correction. We further generalize the formulas of EM fields in the pure quark-gluon plasma (QGP) medium by incorporating a constant Ohm electric conductivity and also during the realistic early-time stages QGP evolution by using a time-dependent electric conductivity. Using the extended KMW model, we observe a slower time evolution and a more reasonable impact parameter dependence of the magnetic field strength than those from the original KMW model in the vacuum. The inclusion of medium effects by using the lattice data helps to further prolong the time evolution of magnetic…
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