Evolution of magnetic fields from the 3+1 dimensional self-similar and Gubser flows in ideal relativistic magnetohydrodynamics
M. Shokri, N. Sadooghi

TL;DR
This paper investigates the evolution of magnetic fields in 3+1 dimensional self-similar and Gubser flows within ideal relativistic magnetohydrodynamics, revealing different decay behaviors and the potential relevance to quark-gluon plasma in heavy ion collisions.
Contribution
It derives new solutions for magnetic field evolution in 3+1D self-similar and Gubser flows using symmetry and conformal transformations, extending previous 1+1D analyses.
Findings
Magnetic fields decay from 1/t to 1/t^3 over time.
Gubser flow results suggest more realistic magnetic field decay in quark-gluon plasma.
Transverse and longitudinal magnetic field components are characterized.
Abstract
Motivated by the recently found realization of the dimensional Bjorken flow in ideal and nonideal relativistic magnetohydrodynamics (MHD), we use appropriate symmetry arguments, and determine the evolution of magnetic fields arising from the dimensional self-similar and Gubser flows in an infinitely conductive relativistic fluid (ideal MHD). In the case of the dimensional self-similar flow, we arrive at a family of solutions, that are related through a differential equation arising from the corresponding Euler equation. To find the magnetic field evolution from the Gubser flow, we solve the MHD equations of a stationary fluid in a conformally flat spacetime. The results are then Weyl transformed back into the Minkowski spacetime. In this case, the temporal evolution of the resulting magnetic field is shown to exhibit a transition between an early…
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