Magnetic fields in heavy ion collisions: flow and charge transport
Gabriele Inghirami (Department of Physics, University of Jyväskylä, Jyvaskyla, 40014, Finland, Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, Helsinki, 00014, Finland); Mark Mace (Department of Physics, University of Jyväskylä, Jyvaskyla, 40014, Finland, Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, Helsinki, 00014, Finland); Yuji Hirono (Asia Pacific Center for Theoretical Physics, Pohang, Gyeongbuk, 37673, Korea, Department of Physics, POSTECH, Pohang, Gyeongbuk, 37673, Korea); Luca Del Zanna (Dipartimento di Fisica e Astronomia, Università di Firenze, Via G. Sansone 1, Sesto Fiorentino, Firenze, 50019, Italy, INAF-Osservatorio Astrofisico di Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy, INFN-Sezione di Firenze, Via G. Sansone 1, Sesto Fiorentino, Firenze, 50019, Italy); Dmitri Kharzeev (Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY, 11794-3800, USA, Department of Physics, Brookhaven National Laboratory, Upton, NY, 11973-5000, USA, RIKEN-BNL Research Center, Brookhaven National Laboratory, Upton, NY, 11973-5000, USA); et al - Show all 6 authors
At the earliest times after a heavy-ion collision, the magnetic field created by the spectator nucleons will generate an extremely strong, albeit rapidly decreasing in time, magnetic field. The impact of this magnetic field may have detectable consequences, and is believed to drive anomalous transport effects like the Chiral Magnetic Effect (CME). We detail an exploratory study on the effects of a dynamical magnetic field on the hydrodynamic medium created in the collisions of two ultrarelativistic heavy-ions, using the framework of numerical ideal MagnetoHydroDynamics (MHD) with the ECHO-QGP code. In this study, we consider a magnetic field captured in a conducting medium, where the conductivity can receive contributions from the electromagnetic conductivity $$\sigma $$ and the chiral magnetic conductivity $$\sigma _{\chi }$$ . We first study the elliptic flow of pions, which we show is relatively unchanged by the introduction of a magnetic field. However, by increasing the magnitude of the magnetic field, we find evidence for an enhancement of the elliptic flow in peripheral collisions. This effect is stronger at RHIC than the LHC, and it is evident already at intermediate collision centralities. Next, we explore the impact of the chiral magnetic conductivity on electric charges produced at the edges of the fireball. This initial $$\sigma _\chi $$ can be understood as a long-wavelength effective description of chiral fermion production. We then demonstrate that this chiral charge, when transported by the MHD medium, produces a charge dipole perpendicular to the reaction plane which extends a few units in rapidity. Assuming charge conservation at the freeze-out surface, we show that the produced charge imbalance can have measurable effects on some experimental observables, like $$v_1$$ or $$\langle \sin \phi \rangle $$ . This demonstrates the ability of a MHD fluid to transport the signature of the initial chiral magnetic fields to late times. We also comment on the limitations of the ideal MHD approximation and detail how further development of a dissipative-resistive model can provide a more realistic description of the QGP.
