Electromagnetic response in an expanding quark-gluon plasma

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Citation: Shovkovy, I. A.
Electromagnetic response in an
expanding quark-gluon plasma.
Preprints 2022,5, 442–450. https://
doi.org/10.3390/particles5040034
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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
et/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 [912] 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[1518].
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
443
only marginally so [
19
,
24
]. On the other hand, it was even suggested that the electromagnetic
response is too weak for applicability of the classical treatment [
25
]. A recent study in Ref. [
26
]
subjected the underlying mechanism to another scrutiny. It claimed that the incomplete
electromagnetic response in heavy-ion collisions, termed colloquially as the "violation of the
conventional Ohm’s law," would reduce trapping of the magnetic flux and, thus, strongly
suppress possible observables due to the chiral anomalous effects. A similar conclusion follows
also from other considerations in Ref. [27].
In retrospect, it should not be surprising that the conventional Ohm’s law is violated on
time scales shorter than the transport relaxation time. However, one needs to clarify why the
electrical conductivity should be suppressed compared to the conventional Ohm’s law in the
steady state. Recall that the electrical conductivity quantifies the electromagnetic response to
an electric field, which is a dissipative process. The dissipation comes from the momentum
relaxation of charges scattering on one another. On times shorter than the relaxation time, the
probability of scattering is negligible, no momentum relaxation occurs, and no dissipation is
expected. In other words, the transport is effectively ballistic. Nevertheless, on short times
scales, the electromagnetic response is indeed incomplete. Below we reconfirm the result by
using analytical solutions within the framework of kinetic theory. We also extend the study to
the case of QGP with a rapid expansion.
The paper is organized as follows. In Sec. 2, we discuss the electromagnetic response in
the simplest model of a plasma without expansion. The effects of expansion are studied in
Sec. 3, where we address the effects of changing temperature, electric field, and collision rate.
Discussion of the main results and the summary of findings are given in Sec. 4
2. Electromagnetic response in a plasma without expansion
Kinetic theory is a convenient tool for describing the electromagnetic response in a plasma.
Within such a framework, a state of QGP is described by distribution functions for every
particle type. For simplicity, we will restrict our consideration below to a single species of
charged particles. Conceptually, such a model will capture the main qualitative features
of the electromagnetic response. Also, the generalization to the case of multiple species is
straightforward.
To study the electromagnetic response, we will perturb the plasma by applying a back-
ground electric field
~
E
, which turns on suddenly at
t=
0. Without loss of generality, we will
assume that the electric field points in the
x
direction. Such a field will induce a nonzero electric
current in the plasma,
Jx(t) = 4eZd3p
(2π)3vxf(px,t), (1)
where
f(px
,
t)
is a time-dependent distribution function in the perturbed plasma. By definition,
the particle velocity is given by
vx∂ep/px
, where
ep=qp2
x+p2
+m2
. Note that the extra
overall factor 4 accounts for the contributions from both particles and antiparticles, as well as
from the two spin degrees of freedom.
The out-of-equilibrium distribution function
f(px
,
t)
satisfies the following kinetic equa-
tion: f(px,t)
t+eExf(px,t)
px
=f(px,t)f0(px)
τ0
, (2)
where
Ex
is the
x
-component of the electric field,
τ0
is the transport relaxation time, and
f0(px) =
1
/(ep2
x+p2
+m2/T0+
1
)
is the Fermi-Dirac distribution function of the plasma in
equilibrium at temperature
T0
. It is appropriate to mention that, in heavy-ion collisions, the
distribution function may differ considerably from the Fermi-Dirac one, especially during
the early stages of plasma evolution. Thus, one might be tempted to complicate the analysis
摘要:

Citation:Shovkovy,I.A.Electromagneticresponseinanexpandingquark-gluonplasma.Preprints2022,5,442–450.https://doi.org/10.3390/particles5040034Publisher'sNote:MDPIstaysneutralwithregardtojurisdictionalclaimsinpublishedmapsandinstitutionalafl-iations.Copyright:©2022bytheauthor.LicenseeMDPI,Basel,Switze...

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