
Citation: Shovkovy, I. A.
Electromagnetic response in an
expanding quark-gluon plasma.
Preprints 2022,5, 442–450. https://
doi.org/10.3390/particles5040034
Publisher’s Note: MDPI stays neutral
with regard to jurisdictional claims in
published maps and institutional affil-
iations.
Copyright: © 2022 by the author.
Licensee MDPI, Basel, Switzerland.
This article is an open access article
distributed under the terms and
conditions of the Creative Commons
Attribution (CC BY) license (https://
creativecommons.org/licenses/by/
4.0/).
Article
Electromagnetic response in an expanding quark-gluon plasma
Igor A. Shovkovy 1,2
1College of Integrative Sciences and Arts, Arizona State University, Mesa, Arizona 85212, USA;
igor.shovkovy@asu.edu
2Department of Physics, Arizona State University, Tempe, Arizona 85287, USA
Abstract:
The validity of conventional Ohm’s law is tested in the context of a rapidly evolving quark-
gluon plasma produced in heavy-ion collisions. Here we discuss the electromagnetic response using
an analytical solution in kinetic theory. As conjectured previously, after switching on an electric field
in a nonexpanding plasma, the time-dependent current is given by
J(t) = (
1
−e−t/τ0)σ0E
, where
τ0
is the transport relaxation time and
σ0
is the steady-state electrical conductivity. Such an incomplete
electromagnetic response reduces the efficiency of the magnetic flux trapping in the quark-gluon plasma
and may prevent the observation of the chiral magnetic effect. Here we extend the study to the case
of a rapidly expanding plasma. We find that the decreasing temperature and the increasing transport
relaxation time have opposite effects on the electromagnetic response. While the former suppresses the
time-dependent conductivity, the latter enhances it.
Keywords: quark-gluon plasma; heavy-ion collisions; kinetic theory; transport; electrical conductivity
1. Introduction
The relativistic heavy-ion collision experiments in Brookhaven and CERN produce the
hottest state of matter ever created in experiments [
1
,
2
]. It is so hot that not only nuclei but
also their constituent protons and neutrons melt away. The corresponding state of matter is
the quark-gluon plasma (QGP) [
3
,
4
]. Over the last two decades, we learned much about its
physical properties. The QGP produced by relativistic heavy-ion collisions has a rather high
temperature of several hundred megaelectronvolts. While composed of deconfined quarks and
gluons, it remains surprisingly strongly interacting. The strong interaction is responsible for a
quick equilibration of the plasma, its high opacity to passing relativistic jets [
5
,
6
], low viscosity
[
7
], and a well-pronounced hydrodynamic flow [
8
]. Theoretical studies also predict that the
QGP may reveal unusual features connected with the chiral magnetic and chiral separation
effects [9–12] that have roots in the quantum chiral anomaly [13,14].
The presence of background magnetic fields is one of the prerequisites for the chiral
anomalous effects [
9
–
12
]. Strong magnetic fields are indeed natural to expect in relativistic
heavy-ion collisions. Since the colliding ions carry positive charges, they produce large electric
currents while moving past each other at speeds close to the speed of light in opposite directions.
According to theoretical estimates, the corresponding currents induce magnetic fields with the
strengths of the order of |eB| ∼ m2
π[15–18].
The detailed description of QGP is intricate because the magnetic fields in heavy-ion
collisions are so short-lived. Moreover, while the fields spike to large values at the moment
of the closest approach of colliding ions, they may become negligible when the proper QGP
forms and becomes equilibrated [
19
]. If it is the case, the chiral effects would not have enough
time to build up. Then, in turn, their observable signatures will be suppressed or non-existent.
One may suggest that the magnetic flux can be trapped and sustained by the QGP because
the latter has a substantial electrical conductivity [
20
–
23
]. If true, the field strength would
decrease relatively slowly with time and, thus, remain sufficiently large to yield discernible
effects due to the chiral anomaly. For a while, this scenario seemed plausible although, perhaps,
arXiv:2210.00691v2 [nucl-th] 22 Oct 2022