arXiv:hep-ex/9601010v1 1 Feb 1996
Factorial and Cumulant Moments in
e+e−→ Hadrons at the Z0Resonance
The SLD Collaboration
K. Abe,(29)I. Abt,(14)C.J. Ahn,(26)T. Akagi,(27)N.J. Allen,(4)W.W. Ash,(27)†
D. Aston,(27)K.G. Baird,(24)C. Baltay,(33)H.R. Band,(32)M.B. Barakat,(33)
G. Baranko,(10)O. Bardon,(16)T. Barklow,(27)A.O. Bazarko,(11)R. Ben-David,(33)
A.C. Benvenuti,(2)G.M. Bilei,(22)D. Bisello,(21)G. Blaylock,(7)J.R. Bogart,(27)
T. Bolton,(11)G.R. Bower,(27)J.E. Brau,(20)M. Breidenbach,(27)W.M. Bugg,(28)
D. Burke,(27)T.H. Burnett,(31)P.N. Burrows,(16)W. Busza,(16)A. Calcaterra,(13)
D.O. Caldwell,(6)D. Calloway,(27)B. Camanzi,(12)M. Carpinelli,(23)R. Cassell,(27)
R. Castaldi,(23)(a)A. Castro,(21)M. Cavalli-Sforza,(7)A. Chou,(27)E. Church,(31)
H.O. Cohn,(28)J.A. Coller,(3)V. Cook,(31)R. Cotton,(4)R.F. Cowan,(16)
D.G. Coyne,(7)G. Crawford,(27)A. D’Oliveira,(8)C.J.S. Damerell,(25)M. Daoudi,(27)
R. De Sangro,(13)P. De Simone,(13)R. Dell’Orso,(23)M. Dima,(9)P.Y.C. Du,(28)
R. Dubois,(27)B.I. Eisenstein,(14)R. Elia,(27)E. Etzion,(4)D. Falciai,(22)C. Fan,(10)
M.J. Fero,(16)R. Frey,(20)K. Furuno,(20)T. Gillman,(25)G. Gladding,(14)
S. Gonzalez,(16)G.D. Hallewell,(27)E.L. Hart,(28)A. Hasan,(4)Y. Hasegawa,(29)
K. Hasuko,(29)S. Hedges,(3)S.S. Hertzbach,(17)M.D. Hildreth,(27)J. Huber,(20)
M.E. Huffer,(27)E.W. Hughes,(27)H. Hwang,(20)Y. Iwasaki,(29)D.J. Jackson,(25)
P. Jacques,(24)J. Jaros,(27)A.S. Johnson,(3)J.R. Johnson,(32)R.A. Johnson,(8)
T. Junk,(27)R. Kajikawa,(19)M. Kalelkar,(24)H. J. Kang,(26)I. Karliner,(14)
H. Kawahara,(27)H.W. Kendall,(16)Y. Kim,(26)M.E. King,(27)R. King,(27)
R.R. Kofler,(17)N.M. Krishna,(10)R.S. Kroeger,(18)J.F. Labs,(27)M. Langston,(20)
A. Lath,(16)J.A. Lauber,(10)D.W.G.S. Leith,(27)M.X. Liu,(33)X. Liu,(7)M. Loreti,(21)
A. Lu,(6)H.L. Lynch,(27)J. Ma,(31)G. Mancinelli,(22)S. Manly,(33)G. Mantovani,(22)
T.W. Markiewicz,(27)T. Maruyama,(27)R. Massetti,(22)H. Masuda,(27)
E. Mazzucato,(12)A.K. McKemey,(4)B.T. Meadows,(8)R. Messner,(27)
P.M. Mockett,(31)K.C. Moffeit,(27)B. Mours,(27)D. Muller,(27)T. Nagamine,(27)
S. Narita,(29)U. Nauenberg,(10)H. Neal,(27)M. Nussbaum,(8)Y. Ohnishi,(19)
L.S. Osborne,(16)R.S. Panvini,(30)H. Park,(20)T.J. Pavel,(27)I. Peruzzi,(13)(b)
M. Piccolo,(13)L. Piemontese,(12)E. Pieroni,(23)K.T. Pitts,(20)R.J. Plano,(24)
R. Prepost,(32)C.Y. Prescott,(27)G.D. Punkar,(27)J. Quigley,(16)B.N. Ratcliff,(27)
T.W. Reeves,(30)J. Reidy,(18)P.E. Rensing,(27)L.S. Rochester,(27)P.C. Rowson,(11)
J.J. Russell,(27)O.H. Saxton,(27)S.F. Schaffner,(27)T. Schalk,(7)R.H. Schindler,(27)
B.A. Schumm,(15)A. Seiden,(7)S. Sen,(33)V.V. Serbo,(32)M.H. Shaevitz,(11)
J.T. Shank,(3)G. Shapiro,(15)S.L. Shapiro,(27)D.J. Sherden,(27)K.D. Shmakov,(28)
C. Simopoulos,(27)N.B. Sinev,(20)S.R. Smith,(27)J.A. Snyder,(33)P. Stamer,(24)
H. Steiner,(15)R. Steiner,(1)M.G. Strauss,(17)D. Su,(27)F. Suekane,(29)
A. Sugiyama,(19)S. Suzuki,(19)M. Swartz,(27)A. Szumilo,(31)T. Takahashi,(27)
F.E. Taylor,(16)E. Torrence,(16)A.I. Trandafir,(17)J.D. Turk,(33)T. Usher,(27)
J. Va’vra,(27)C. Vannini,(23)E. Vella,(27)J.P. Venuti,(30)R. Verdier,(16)
P.G. Verdini,(23)S.R. Wagner,(27)A.P. Waite,(27)S.J. Watts,(4)A.W. Weidemann,(28)
E.R. Weiss,(31)J.S. Whitaker,(3)S.L. White,(28)F.J. Wickens,(25)D.A. Williams,(7)
D.C. Williams,(16)S.H. Williams,(27)S. Willocq,(33)R.J. Wilson,(9)
W.J. Wisniewski,(27)M. Woods,(27)G.B. Word,(24)J. Wyss,(21)R.K. Yamamoto,(16)
J.M. Yamartino,(16)X. Yang,(20)S.J. Yellin,(6)C.C. Young,(27)H. Yuta,(29)
G. Zapalac,(32)R.W. Zdarko,(27)C. Zeitlin,(20)Z. Zhang,(16)and J. Zhou,(20)
(1)Adelphi University, Garden City, New York 11530
(2)INFN Sezione di Bologna, I-40126 Bologna, Italy
(3)Boston University, Boston, Massachusetts 02215
(4)Brunel University, Uxbridge, Middlesex UB8 3PH, United Kingdom
(5)California Institute of Technology, Pasadena, California 91125
(6)University of California at Santa Barbara, Santa Barbara, California 93106
(7)University of California at Santa Cruz, Santa Cruz, California 95064
(8)University of Cincinnati, Cincinnati, Ohio 45221
(9)Colorado State University, Fort Collins, Colorado 80523
(10)University of Colorado, Boulder, Colorado 80309
(11)Columbia University, New York, New York 10027
(12)INFN Sezione di Ferrara and Universit` a di Ferrara, I-44100 Ferrara, Italy
(13)INFN Lab. Nazionali di Frascati, I-00044 Frascati, Italy
(14)University of Illinois, Urbana, Illinois 61801
(15)Lawrence Berkeley Laboratory, University of California, Berkeley, California
(16)Massachusetts Institute of Technology, Cambridge, Massachusetts 02139
(17)University of Massachusetts, Amherst, Massachusetts 01003
(18)University of Mississippi, University, Mississippi 38677
(19)Nagoya University, Chikusa-ku, Nagoya 464 Japan
(20)University of Oregon, Eugene, Oregon 97403
(21)INFN Sezione di Padova and Universit` a di Padova, I-35100 Padova, Italy
(22)INFN Sezione di Perugia and Universit` a di Perugia, I-06100 Perugia, Italy
(23)INFN Sezione di Pisa and Universit` a di Pisa, I-56100 Pisa, Italy
(24)Rutgers University, Piscataway, New Jersey 08855
(25)Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX United
(26)Sogang University, Seoul, Korea
(27)Stanford Linear Accelerator Center, Stanford University, Stanford, California
(28)University of Tennessee, Knoxville, Tennessee 37996
(29)Tohoku University, Sendai 980 Japan
(30)Vanderbilt University, Nashville, Tennessee 37235
(31)University of Washington, Seattle, Washington 98195
(32)University of Wisconsin, Madison, Wisconsin 53706
(33)Yale University, New Haven, Connecticut 06511
(a)Also at the Universit` a di Genova
(b)Also at the Universit` a di Perugia
We present the first experimental study of the ratio of cumulant to factorial mo-
ments of the charged-particle multiplicity distribution in high-energy particle interac-
tions, using hadronic Z0decays collected by the SLD experiment at SLAC. We find that
this ratio, as a function of the moment-rank q, decreases sharply to a negative mini-
mum at q = 5, which is followed by quasi-oscillations. These features are insensitive
to experimental systematic effects and are in qualitative agreement with expectations
from next-to-next-to-leading-order perturbative QCD.
One of the most fundamental observables in high-energy particle interactions is the mul-
tiplicity of particles produced in the final state. A large body of experimentally mea-
sured multiplicity distributions has been accumulated in a variety of hard processes.
The Poisson distribution (PD) does not describe the shapes of multiplicity distribu-
tions measured in e+e−, pp, and p¯ p collisions, implying non-random particle-production
mechanisms, but elucidation of the relationship between the measured shapes and the
underlying dynamics has proven to be problematic.
At present the theory of strong interactions, Quantum Chromodynamics (QCD) ,
cannot be used to calculate distributions of final-state hadrons since the mechanism
of hadron formation has not been understood quantitatively. However, perturbative
QCD can be applied to calculate some properties of the cascade of gluons radiated by
the partons produced in a hard scattering process. If there is a simple relationship
between the distributions of partons and detected final state particles, as follows for
example from the ansatz of local parton-hadron duality (LPHD) , then such calcu-
lations may be expected to reproduce some features of experimental data. An early
calculation  in the leading double-logarithmic approximation (DLA) was successful
in describing the energy dependence of the average multiplicity, as well as the energy
independence of the “KNO distribution”  of n/<n>, the multiplicity scaled by its av-
erage value. However, the width predicted by this calculation is much larger than that
of experimentally observed multiplicity distributions . It has been suggested that
the inclusion of higher-order terms in perturbative QCD calculations should reduce the
predicted width of the multiplicity distribution [6, 7], although no such calculation has
yet been achieved. However, the ratio of cumulant to factorial moments has recently
been proposed  as a sensitive measure of the shape of multiplicity distributions and
has been found to be calculable in higher-order perturbative QCD.
Factorial moments have been used to characterize cascade phenomena in various
scientific fields . The factorial moment of rank q is defined 
Fq≡<n(n − 1)...(n − q + 1)>
where n is the particle multiplicity of an event and <n> is the average multiplicity in
the event sample. The cumulant moments Kqare related to the Fqby 
(q − 1)!
m!(q − m − 1)!Kq−mFm, (2)
and F0=F1=K1≡ 1. While the DLA QCD calculation predicts  that the ratio Hq≡
Kq/Fqdecreases as q−2, the inclusion of higher orders yields more striking behavior.
A calculation in the next-to-leading logarithm approximation (NLA) predicts  a
minimum in Hq at q ≈ 5 and a positive constant value for q ≫ 5, while the next-
to-next-to-leading logarithm approximation (NNLA) predicts  that this minimum
is negative and is followed by quasi-oscillations about zero. These predictions are
illustrated in Fig. 1.
In a previous study  Hqwere calculated using published multiplicity distribu-
tions from e+e−and p¯ p collisions, and features qualitatively similar to those predicted
by the NNLA calculation were observed. This was a significant result, supporting not
only QCD at the parton level, but also the notion of LPHD. However, no account was
taken of experimental systematic effects or of the correlations, both statistical and sys-
tematic, between values of Hqat different ranks q. In addition, some Hqvalues derived
from data from similar experiments were apparently inconsistent. Furthermore, it was
shown subsequently  that the observed features could be induced by the effective
truncation of the multiplicity distribution inherent in a measurement using a finite
In this letter we present the first experimental determination of the ratio of cumulant
to factorial moments of the charged-particle multiplicity distribution in high-energy
particle interactions, using hadronic decays of Z0bosons produced in e+e−annihila-
tions. We study systematic effects in detail, in particular the influence of truncation of
the distribution, and investigate the correlations between moments of different rank.
We compare our measurements with the predictions of perturbative QCD, and also
with two widely used distributions predicted by phenomenological models of particle
2 Charged Multiplicity Analysis
Hadronic decays of Z0bosons produced by the SLAC Linear Collider (SLC) were
collected with the SLC Large Detector (SLD) . The trigger and initial selection
of hadronic events are described in . The analysis used charged tracks measured
in the central drift chamber (CDC)  and vertex detector (VXD) . A set of
cuts was applied to the data to select well-measured tracks and events well contained
within the detector acceptance. Charged tracks were required to have: a distance of
closest approach transverse to the beam axis within 5 cm, and within 10 cm along
the axis from the measured interaction point; a polar angle, θ, with respect to the
beam axis within |cosθ| < 0.8; and a momentum transverse to the beam axis greater
than 0.15 GeV/c. Events were required to have: a minimum of five such tracks; a
thrust-axis  direction within |cosθT| < 0.71; and a total visible energy of at least
20 GeV, which was calculated from the selected tracks assigned the charged pion mass.
A total of 86,679 events from the 1993 to 1995 SLC/SLD runs survived these cuts and
were included in this analysis. The efficiency for selecting hadronic events satisfying
the |cosθT| cut was estimated to be above 96%. The background in the selected event
sample was estimated to be (0.3 ± 0.1)%, dominated by Z0→ τ+τ−decays, and was
subtracted statistically from the observed multiplicity distribution.
The experimentally observed charged-particle multiplicity distribution was cor-
rected for effects introduced by the detector, such as geometrical acceptance, track-
reconstruction efficiency, and additional tracks from photon conversions and particle
interactions in the detector materials, as well as for initial-state photon radiation and
the effect of the cuts listed above. The charged multiplicity of an event was defined
to include all promptly produced charged particles, as well as those produced in the
decay of particles with lifetime < 3 · 10−10s. A two-stage correction was calculated
using Monte Carlo simulated hadronic Z0decays produced by the JETSET 6.3 
event generator, subjected to a detailed simulation of the SLD and reconstructed in
the same way as the data. Each MC event passing the event-selection cuts yielded a
number of generated tracks ngand a number of observed tracks no, which were used
to form the matrix
where N(ng,no) is the number of MC events with nggenerated tracks and noobserved
tracks, and NMC
a sum of three Gaussians was fitted to M(ng,no) and this parametrization was used
in the correction. The effects of the event-selection cuts and of initial-state radiation
were corrected using factors
obs(no) is the number of MC events with noobserved tracks. For each no,
where Ptrue(ng) is the normalized simulated multiplicity distribution generated without
initial-state radiation and Psel(ng) is the normalized distribution for those events in
the fully-simulated sample that passed the selection cuts.
Both corrections were applied to the experimentally observed multiplicity distribu-
tion Pexp(no) to yield the corrected distribution:
Pcor(n) = CF(n) ·
M(n,no) · Pexp(no), (5)
which is shown with statistical errors only in Fig. 2a. The factorial moments Fq, cumu-
lant moments Kq, and their ratios Hqwere calculated from this distribution according
to Eqs. 1 and 2. The resulting Hqup to rank q = 17 are shown in Fig. 3 and listed
in Table 1. As q increases, the value of Hq falls rapidly (inset of Fig. 3), reaches a
negative minimum at q = 5, and then oscillates about zero with a positive maximum
at q = 9 and a second negative minimum at q = 13. The statistical and systematic
errors are strongly correlated between ranks as we now discuss.
3 Statistical and Systematic Errors
Statistical errors and correlations were studied by analyzing simulated multiplicity dis-
tributions. The Hqwere calculated from 10 Monte Carlo samples of the same size as
the data sample and 20 multiplicity distributions generated according to the measured
distribution. For each Hq the standard deviation in these 30 samples was taken as
the statistical error, and is listed in Table 1. In each case the Hqexhibited the same
behavior as those calculated from the data, although the value of H5and the appar-
ent phase of the quasi-oscillation for q ≥ 8 were found to be sensitive to statistical
fluctuations. We investigated the possibility that the observed features might result
from a statistical fluctuation by generating 10,000 multiplicity distributions according
to Poisson and negative-binomial distributions (see below) with the same mean value
as our corrected multiplicity distribution. In no case did any sample exhibit either a
minimum near q= 5 or quasi-oscillations at higher q.
Experimental systematic effects were also investigated. An important issue is the
simulation of the track-reconstruction efficiency of the detector. The Hqwere found
to be sensitive to the global efficiency, which was tuned in the simulation so that our
average corrected multiplicity equalled the value measured in hadronic Z0decays .
The Hq resulting from a variation in the global efficiency of ±1.7%, corresponding
to the error on the measured average multiplicity, are shown in Fig. 4. There is an
asymmetric effect on the value of H5and on the apparent phase of the quasi-oscillation.
For each q the difference between the Hqwith increased and decreased efficiency was
assigned as a symmetric systematic uncertainty.
It is important to consider the dependence of the track reconstruction efficiency on
multiplicity. Our simulated efficiency is 91.5% for tracks crossing at least 40 of the 80
layers of the CDC, and is independent of ngwithin ±0.5%. Varying the efficiency for
ng> 20 by ±0.5% caused a change of ±4% in H5, and negligible changes for q > 5.
This change was assigned as a systematic uncertainty.
Variation of the form of the parametrization of the correction matrix M was found
to affect mainly the amplitude of the quasi-oscillation for q ≥ 8. Application of the
unparametrized version of the matrix M(ng,no) produced the largest such effect, which
is shown in Fig. 4. This change was conservatively assigned as a symmetric systematic
uncertainty to account for possible mismodelling of the off-diagonal elements of the
matrix. The effect on the Hqof variation of the parameters of the three-Gaussian fits
to M within their errors increases with increasing q, becoming the dominant uncertainty
for q ≥16.
The effects on the Hqof wide variations in the criteria for track and event selection
were found to be small compared with those due to the above sources. The effect
of including values of the multiplicity distribution at n=2 and n=4, taken from the
JETSET model, in the calculation of the moments is also small. Varying the estimated
level of non-hadronic background, which appears predominantly in the low-multiplicity
bins, by ±100% produces a negligible change in the Hq.
The uncertainties from the above systematic sources were added in quadrature to
derive a systematic error on each Hq, which is listed in Table 1. All of our studies
showed a clear first minimum in Hqat q = 5 followed by quasi-oscillations for q ≥8.
The value of H5has a total uncertainty of ±13% that is strongly correlated with similar
errors on H6and H7and with an uncertainty in the phase of the quasi-oscillation of
∓0.2 units of rank. There is an uncertainty on the amplitude of the quasi-oscillation
of ±15% that is essentially independent of the other errors. From these studies we
conclude that the steep decrease in Hqfor q<5, the negative minimum at q = 5, and
the quasi-oscillation about zero for q≥8 are well-established features of the data.
4 Comparison of the Hqwith QCD Predictions
We have compared these results with the qualitative predictions of perturbative QCD
discussed in Section 1. Figure 1 shows that the DLA QCD calculation predicts no neg-
ative values of Hqand is inconsistent with the data. The NLA and NNLA calculations
predict  a steep decrease in Hqto a minimum at
data. For q > 5, the NLA calculation predicts that Hq increases toward a constant
value, which is not consistent with the data, whereas the NNLA calculation predicts
quasi-oscillations in Hqin agreement with the data.
The moment ratios are thus seen to be a sensitive discriminator between QCD
calculations at different orders of purturbation theory. We conclude that the Hqcalcu-
lated for gluons in the next-to-next-to-leading logarithm approximation of perturbative
QCD describe the shape of the observed multiplicity distribution, whereas the available
calculations at lower order do not.
Z) measured in Z0decays  qmin≈ 5. These features are seen in the
Table 1: Ratio of cumulant to factorial moments, Hq. The errors are strongly correlated
between ranks as discussed in the text.
5 Comparison with phenomenological models
Measured multiplicity distributions have been compared extensively with the predic-
tions of phenomenological models. We consider two such predicted distributions. The
negative binomial distribution (NBD)
Pn(?n?,k) = Cn
?n? + k
?n? + k
where ?n? and k are free parameters, is predicted  by models in which the hard
interaction produces several objects, sometimes identified with the partons in a QCD
cascade, each of which decays into a number of particles. The log-normal distribution
where µ, σ, and c are free parameters, is predicted  by models in which the particles
result from a scale-invariant stochastic branching process, which might be related to
−(ln(n′+ c) − µ)2
the parton branchings in a QCD cascade.
Considering statistical errors only, we performed least-squares fits of the NBD and
LND to our corrected multiplicity distribution. These fitted distributions and their
normalized residuals are shown in Figs. 2a and 2b, respectively. Both provide rea-
sonable descriptions of the data, with χ2/ndf of 68.0/24 and 30.5/23, respectively.
Although the NBD has a high χ2and shows structure in the residuals in the core
of the distribution, it is difficult to exclude without a thorough understanding of the
uncorrelated component of the systematic errors. These results are in agreement with
those from a previous analysis .
The PD and the phenomenological distributions differ markedly in their moment
structure: for the PD, Hq= 0 for all q; for the fitted NBD, Hqis positive and falls as
q−25; for the fitted LND, Hqfalls with increasing q to a negative minimum at q = 6
and then oscillates about zero. It was recently argued  that the truncation of the
large-n tail of the multiplicity distribution due to finite data-sample size could lead
to quasi-oscillations in Hq similar to those observed in the data. We calculated Hq
values from the fitted distributions over the multiplicity range observed in the data,
6 ≤ n ≤ 54, and the results are displayed in Fig. 5. The truncated PD and NBD
are found to produce features similar to those in the data, but with much smaller
amplitudes. The amplitudes are not sensitive to the exact value of the truncation
point and we conclude that the moment ratios predicted by the PD and NDB are
inconsistent with the data. The LND predictions are insensitive to the truncation
point and show the same qualitative features as the data. However, the first minimum
is smaller in amplitude and is at q = 6. The quasi-oscillation for q ≥ 8 has similar
amplitude and period, and is displaced by about one unit from the data. The moment
ratios Hqare thus seen to provide a sensitive test of phenomenological models.
In conclusion, we have conducted the first experimental study of the ratio Hqof cu-
mulant to factorial moments of the charged-particle multiplicity distribution in high-
energy particle interactions, using hadronic Z0decays. We find that Hq decreases
sharply with increasing rank q to a negative minimum at q = 5, followed by quasi-
oscillations; we show these features to be insensitive to statistical and experimental
The predictions of perturbative QCD in the next-to-next-to-leading-logarithm ap-
proximation are in agreement with the features observed in the data, supporting both
the validity of QCD at the parton level and the notion that the observable final state
reflects the underlying parton structure. Calculations in the leading double-logarithm
and next-to-leading-logarithm approximations are not sufficient to describe the data.
The Poisson and negative binomial distributions do not predict these features. The
log-normal distribution predicts features similar to those of the data, but does not
describe the data in detail. We conclude that the moment ratios Hqof the charged-
particle multiplicity distribution provide a sensitive test both of perturbative QCD and
of phenomenological models.
We thank the personnel of the SLAC accelerator department and the technical staffs of
our collaborating institutions for their efforts, which resulted in the successful operation
of the SLC and the SLD. We thank I. Dremin for useful discussions.
This work was supported by U.S. Department of Energy contracts: DE-FG02-
91ER40676 (BU), DE-FG03-92ER40701 (CIT), DE-FG03-91ER40618 (UCSB), DE-
FG03-92ER40689 (UCSC), DE-FG03-93ER40788 (CSU), DE-FG02-91ER40672 (Col-
orado), DE-FG02-91ER40677(Illinois), DE-AC03-76SF00098 (LBL), DE-FG02-92ER40715
(Massachusetts), DE-AC02-76ER03069 (MIT), DE-FG06-85ER40224 (Oregon), DE-
AC03-76SF00515 (SLAC), DE-FG05-91ER40627 (Tennessee), DE-AC02-76ER00881
(Wisconsin), DE-FG02-92ER40704 (Yale); U.S. National Science Foundation grants:
PHY-91-13428 (UCSC), PHY-89-21320(Columbia), PHY-92-04239 (Cincinnati), PHY-
88-17930 (Rutgers), PHY-88-19316 (Vanderbilt), PHY-92-03212 (Washington); the UK
Science and Engineering Research Council (Brunel and RAL); the Istituto Nazionale
di Fisica Nucleare of Italy (Bologna, Ferrara, Frascati, Pisa, Padova, Perugia); and the
Japan-US Cooperative Research Project on High Energy Physics (Nagoya, Tohoku).
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1. Functional form of perturbative QCD predictions of the ratio Hqof cumulant to
factorial moments in the leading double-logarithm (solid line), next-to-leading-
logarithm (dotted line) and next-to-next-to-leading-logarithm (dashed line) ap-
proximations. The vertical scale and relative normalizations are arbitrary.
2. a) The corrected charged-particle multiplicity distribution. The open circles at
n= 2, 4 are the predictions of the JETSET Monte Carlo. The solid and dashed
lines represent fitted negative-binomial and log-normal distributions, respectively.
The normalized residuals are shown in b). The fits yielded parameter values of
k = 24.9 and ?n? = 20.7 for the NBD and µ = 3.52, σ = 0.175 and c = 13.4 for
the LND. The errors are statistical only.
3. Ratio of cumulant to factorial moments, Hq, as a function of the moment rank
q. The error bars are statistical and are strongly correlated between ranks.
4. Examples of systematic effects on Hq. The data points show the Hqwith sta-
tistical errors derived using the standard correction. The dotted (dashed) line
connects Hqvalues derived with an increase (decrease) of 1.7% in the simulated
track reconstruction efficiency. The solid line connects Hqvalues derived using
the unparametrized correction matrix.
5. Comparison of the Hqmeasured in the data (dots with statistical errors) with the
predictions of truncated Poisson (dotted line joining the values at different q),
negative binomial (dashed line) and log-normal (dot-dashed line) distributions.
Moment Rank q
Hq (arbitrary units)
Charged Multiplicity n
20 40 600
Moment Rank q
Moment Rank q
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Moment Rank q