Confronting anomalous kaon correlations measured in Pb-Pb collisions atpsNN 276 TeV Joseph I. Kapusta1Scott Pratt2and Mayank Singh1

2025-04-27 0 0 502.31KB 12 页 10玖币
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Confronting anomalous kaon correlations measured in Pb-Pb collisions at sN N = 2.76
TeV
Joseph I. Kapusta,1Scott Pratt,2and Mayank Singh1
1School of Physics & Astronomy, University of Minnesota, Minneapolis, MN 55455, USA
2Department of Physics and Astronomy and Facility for Rare Isotope Beams
Michigan State University, East Lansing, MI 48824 USA
Measurements of the dynamical correlations between neutral and charged kaons in central Pb-Pb
collisions at sNN = 2.76 TeV by the ALICE Collaboration display anomalous behavior relative
to conventional heavy-ion collision simulators such as AMPT, EPOS, and HIJING. We consider
other conventional statistical models, none of which can reproduce the magnitude and centrality
dependence of the correlations. The data can be reproduced by coherent emission from domains
which grow in number and volume with increasing centrality. We show that the energy released by
condensation of strange quarks may be sufficient to explain the anomaly.
I. INTRODUCTION
High energy heavy-ion collision experiments help us ex-
plore the deconfined state of QCD matter. The Quark-
Gluon Plasma (QGP) created in these experiments ex-
pands and cools to form hadrons on timescales on the
order of ten fm/c. We infer the properties of the QGP
from the yields and correlations of these hadrons.
The ALICE Collaboration has measured the correla-
tion function νdyn(K0
S, K±) as a function of multiplic-
ity and transverse momentum in Pb-Pb collisions at
sNN = 2.76 TeV [1]. These measurements stand in
contrast to the predictions made using standard heavy-
ion simulators [2], including AMPT, EPOS, and HIJING.
The purpose of this paper is to construct a simple model,
based on the condensation of strange quark and anti-
quark pairs, in an attempt to reproduce the data, and
to explore the degree to which other, less exotic, physics
might explain the ALICE results. The proposed disor-
dered chiral condensate (DCC) [3] state is expected to
give anomalaous values of νdyn(K0
S, K±) which could ex-
plain the data, though we show in this work that an
ordinary strange condensate will give a similar result.
The νdyn(A,B) measures the degree to which the obser-
vation of particles of types Aand Bare more correlated
with themselves than with each other,
νdyn(A, B) = RAA +RBB 2RAB,
RAB =hNANBi−hNAiδAB
hNAihNBi1,(1)
where the symbols ··i refer to averages over events.
The second term, proportional to δAB , subtracts the con-
tribution of a particle with itself. If particles were uncor-
related with one another, one would have RAA =RBB =
RAB = 0, and νdyn would vanish. That is the reason
for referring to this correlation function as dynamical. If
νdyn(A, B)>0, it implies that the observation of an Aor
Btype particle more strongly biases a second particle to-
ward being the same type. For the ALICE measurement
the two types of particles were charged kaons, either K+
or K, and neutral kaons, i.e. K0
Smesons. Positive val-
ues of νdyn(K0
S, K±) can result from decays, such as the
φmeson, which decays into either two charged kaons or
two neutral kaons. Other sources can be charge conser-
vation, or anomalously strong Bose enhancement from
condensation or coherent emission.
Background sources of correlation, such as decays and
charge conservation, largely correlate two particles with
one another. In such cases νdyn scales inversely with
the multiplicity. For this reason, ALICE multiplied νdyn
by a factor 1, which is inversely proportional to the
multiplicity
1=NK±NK0
S
NK±+NK0
S
,(2)
where NK±and NK0
Srefer to the average number of
charged and K0
Smesons observed per event. If one cor-
rects for multiplicity, and if the number of charged and
neutral kaons were equal, 1would become one sixth
the total number of kaons.
We present a phenomenological model with coherent
emission in Sec. II. We find that the data can be repro-
duced if a sufficient fraction of the kaons were to origi-
nate from coherent sources of sufficient size. Section III
considers simple systems to illustrate the effects of de-
cays, charge conservation, and Bose symmetrization. We
find that generating large correlations requires that many
kaons are in the same quantum state, as occurs in Bose
condensation. Section IV shows results of a purely ther-
mal model with charge conservation. The resulting corre-
lation from this model also comes well short of the data.
Section V calculates the energy available from strange
quark condensation in several versions of the linear sigma
model. Conclusions from this study, along with prospects
and suggestions for future study, are given in Sec. VI.
II. ISOSPIN FLUCTUATIONS FROM
CONDENSATES
The observable which isolates isospin fluctuations is
νdyn as discussed earlier. The ALICE Collaboration
measured the number of short-lived kaons K0
Sand the
number of positively and negatively charged kaons K+
arXiv:2210.03257v1 [hep-ph] 6 Oct 2022
2
and Kto construct νdyn(K0
S, K±) [1]. Table I shows
some of the experimental data. The numbers marked
with an asterix were interpolated from 966.0 in the
10-20% bin. From the data there is a best fit rela-
tion where dNch/dη = 1.317N1.19
part. Conversely Ntot
K
0.113 dNch/dη as one would expect from an isothermal
freeze-out model. In either case the 60-80% bin appears
anomalous and has been excluded from these fits. The
quantity αwas defined as
α=1
NK0
S
+1
NK±
.(3)
For a first analysis we assume that kaons of all four kinds
are produced in equal numbers despite the fact that K0
S
was measured in a slightly different range in momentum
space than the charged kaons.
Centrality νdyn νdyn1/α NK0
S3/2αNK±3/α dNch/dη Npart
0-5 % 0.006827 ±0.00068 0.213 ±0.021 31.20 46.80 93.60 1601.0 382.8
5-10 % 0.006927 ±0.00069 0.169 ±0.017 24.40 36.60 73.20 1294.0 329.7
10-15 % 0.006993 ±0.0007 0.141 ±0.014 20.16 30.24 60.48 1075.0* 281.1
15-20 % 0.007226 ±0.0007 0.113 ±0.011 15.64 23.46 46.92 857.0* 238.6
20-40 % 0.008307 ±0.0008 0.080 ±0.010 9.630 14.45 28.89 537.50 157.2
40-60 % 0.016430 ±0.00167 0.066 ±0.007 4.02 6.03 12.06 205.0 68.56
60-80 % 0.025130 ±0.0022 0.053 ±0.005 2.11 3.17 6.33 55.50 22.52
TABLE I. Summary of the relevant νdyn experimental data from Table 2 of Ref. [1]. The charged particle pseudo-rapidity
densities are taken from [4] and the number of participants from [5].
ALICE found that the correlations are spread across
pseudo-rapidity but are restricted in transverse momen-
tum. This indicates that the coherent kaons likely orig-
inate in different domains which extend to at least 1.5
units in pseudo-rapidity and are moving at different ve-
locities depending on their transverse position in the pro-
duced matter. In the language of DCC, the data favors
the domains picture [6] as opposed to the “Baked Alaska”
picture where there is a single DCC at the center with
the expanding fireball on the outside [7].
A simple formula for νdyn was derived in Ref. [8]. It is
νdyn = 4βKβK
3Nd1
Ntot
K(4)
where βKis the fraction of all kaons coming from con-
densates, Ndis the number of domains, and Ntot
Kis the
total number of kaons regardless of their charge or source.
This formula is based on several assumptions. (1) There
are two sources for each domain. One is a coherent source
which, by definition, has a distribution of the fraction f
of neutral kaons which is equal to one (which is the case
for strange DCC [9]) while the other (random) source is
a Gaussian with a width determined by the number of
kaons. (2) Domains are independent of each other. (3)
The number of domains is greater than two.
The fraction of kaons from condensates can be esti-
mated as
βK=ζVd
mKNtot
K
(5)
where ζis the energy density of condensation which is
converted to kaons and Vdis the total volume of all such
domains.
In the DCC picture domain size should be limited by
causality, and that is related to the lifetime of the system.
In order to estimate the latter, we use results from Pb-
Pb collisions at sNN = 2.76 TeV as simulated by the
relativistic 2nd order viscous hydrodynamic code MU-
SIC, with IP-Glasma initial conditions and initial proper
time τ0= 0.4 fm/c [10]. For a given event, the fluid cell
with the highest initial temperature was followed until
it expanded and cooled to some temperature of inter-
est, and the proper time duration (not including τ0) was
recorded. Averaged over events in a given multiplicity
window yielded a numerical value τav. The results are
shown in the Table II, with τav in units of fm/c. If the
expansion is primarily one dimensional then one would
expect Nd/Vdto scale as 1av. Being an intensive quan-
tity, Nd/Vdshould be independent of the total charged
particle multiplicity dNch/dη. On the other hand, both
Vdand Ndshould be proportional to dNch/dη. Taken
together it means that νdyn will depend on centrality.
The experimental data for νdyn(K±, K0
S)is plotted as
a function of dNch/dη in Fig. 1(a) and as a function of
time in Fig. 1(b). In both cases the data exhibits greater
than linear growth.
To reproduce the data, we assume that the number
of domains scales with the total kaon multiplicity which
3
Centrality T= 160 MeV T= 150 MeV T= 140 MeV
0-5 % 11.56 13.27 14.93
5-10 % 10.84 12.48 14.39
10-15 % 10.22 11.78 13.84
15-20 % 9.81 11.52 12.98
20-25 % 9.31 10.72 12.10
25-30 % 9.05 10.15 11.89
30-35 % 8.47 9.69 11.11
35-40 % 7.88 8.81 10.53
40-45 % 7.24 8.61 9.83
45-50 % 6.88 7.51 8.94
TABLE II. Proper time elapsed in fm/c beginning at the start
of hydrodynamic flow and ending at the indicated tempera-
ture using the hydrodynamic code MUSIC with IP Glasma
initial conditions [10]. Chemical equilibration happens at
about 160 MeV.
scales with dNch/dη so that
Nd=aNtot
K,
Vd=v0Ntot
Kτav
10τ0,(6)
where the factor of 10 is inserted simply as a matter of
numerical convenience. Then
βK=bτav
10τ0(7)
where
b=ζv0
mK
(8)
which results in
νdyn = 4bτav
10τ0b
3aτav
10τ011
Ntot
K
,
νdyn
α=2
3bτav
10τ0b
3aτav
10τ01.(9)
A fit to the five highest multiplicity bins yields b=
0.1044 ±0.0380 and b2/a = 0.2187 ±0.0458 as shown in
Fig. 2. We assume that chemical freeze-out occurs at
T= 160 MeV. The fit only determines the product of ζ
with v0. Using as a reference ζ= 25 MeV/fm3we have
v0= 2.07 25 MeV/fm3
ζfm3.(10)
Table III shows the results with the reference ζ= 25
MeV/fm3. We use the extrapolated value of τav for the
20-40% bin to be 8.62 fm/c and for the 40-60% bin to be
6.60 fm/c so that we can fill in the table. If, for example,
ζ= 50 MeV/fm3instead, the number of sources Nddoes
not change but the volume Vdis halved.
FIG. 1. The correlation νdyn(K±, K0
S)from the ALICE
Collaboration is plotted against the charged multiplicity, also
measured by ALICE (a) and against the duration of the col-
lision in the deconfined phase, as estimated by hydrodynamic
calculations (b). Times are shown for three choices of de-
confinement temperatures: 140, 150 and 160 MeV. The cor-
relation increases roughly linearly with the multiplicity, and
stronger than linear with the collision duration.
Centrality NdVd(fm3)βK
0-5 % 9.32 1120 0.302
5-10 % 7.29 821 0.283
10-15 % 6.02 640 0.267
15-20 % 4.67 476 0.256
20-40 % 2.88 258 0.225
40-60 % 1.20 82 0.172
TABLE III. The number of domains Ndand the total volume
Vdoccupied by them. The two parameter fit was made to the
five highest multiplicity bins. This assumes ζ= 25 MeV/fm3.
摘要:

ConfrontinganomalouskaoncorrelationsmeasuredinPb-PbcollisionsatpsNN=2:76TeVJosephI.Kapusta,1ScottPratt,2andMayankSingh11SchoolofPhysics&Astronomy,UniversityofMinnesota,Minneapolis,MN55455,USA2DepartmentofPhysicsandAstronomyandFacilityforRareIsotopeBeamsMichiganStateUniversity,EastLansing,MI48824USAM...

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