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Feng, Yejun; Wang, Yishu; Palmer, A.; Li, Ling; Silevitch, D. M.; Calder, Stuart; Rosenbaum, T. F.

doi:10.1103/physrevb.95.125102

Cited by 1 publication

(2 citation statements)

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“…In our model we compute the spectra of the emitted particles by using the Cooper-Frye prescription [43], so we should modify this recipe in such a way to take into account a contribution due to the electromagnetic fields. Unfortunately, the underlying assumption of the ideal MHD approach that the electric field in the comoving frame of the fluid is always zero, with an infinitely small relaxation time, makes modifying the distribution function in the denominator of the Cooper-Frye equation in a consistent way very difficult [62,63]. It will be possible to overcome this limitation with resistive MHD.…”

Section: Charge Production and The Cmementioning

confidence: 99%

“…Unfortunately, the underlying assumption of the ideal MHD approach that the electric field in the comoving frame of the fluid is always zero, with an infinitely small relaxation time, makes modifying the distribution function in the denominator of the Cooper-Frye equation in a consistent way very difficult [62,63]. It will be possible to overcome this limitation with resistive MHD.…”

Section: Charge Production and The Cmementioning

confidence: 99%

See 1 more Smart Citation

Magnetic fields in heavy ion collisions: flow and charge transport

et al. 2020

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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 σ and the chiral magnetic conductivity σχ. 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 σχ 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 v1 or sin φ . 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.

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Section: Charge Production and The Cmementioning

confidence: 99%

Section: Charge Production and The Cmementioning

confidence: 99%