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Measurement of Charged-Particle Multiplicities in Gluon and Quark Jets in pp Collisions at s√=1.8   TeV

CDF Collaboration

CLARK, Allan Geoffrey (Collab.), D'ONOFRIO, Monica (Collab.), WU, Xin (Collab.)

Abstract

We report the first largely model independent measurement of charged particle multiplicities in quark and gluon jets, Nq and Ng, produced at the Fermilab Tevatron in pp¯ collisions with a center-of-mass energy of 1.8 TeV and recorded by the Collider Detector at Fermilab. The measurements are made for jets with average energies of 41 and 53 GeV by counting charged particle tracks in cones with opening angles of θc=0.28, 0.36, and 0.47 rad around the jet axis. The corresponding jet hardness Q=Ejetθc varies in the range from 12 to 25 GeV.

At Q=19.2  GeV, the ratio of multiplicities r=Ng/Nq is found to be 1.64±0.17, where statistical and systematic uncertainties are added in quadrature. The results are in agreement with resummed perturbative QCD calculations.

CDF Collaboration, CLARK, Allan Geoffrey (Collab.), D'ONOFRIO, Monica (Collab.), WU, Xin (Collab.). Measurement of Charged-Particle Multiplicities in Gluon and Quark Jets in pp Collisions at s√=1.8   TeV. Physical Review Letters , 2005, vol. 94, no. 17, p. 171802

DOI : 10.1103/PhysRevLett.94.171802

Available at:

http://archive-ouverte.unige.ch/unige:38096

Disclaimer: layout of this document may differ from the published version.

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Measurement of Charged-Particle Multiplicities in Gluon and Quark Jets in p p Collisions at

p s

1:8 TeV

D. Acosta,1T. Affolder,2M. G. Albrow,3D. Ambrose,4D. Amidei,5K. Anikeev,6J. Antos,7G. Apollinari,3T. Arisawa,8 A. Artikov,9W. Ashmanskas,10F. Azfar,11P. Azzi-Bacchetta,12N. Bacchetta,12H. Bachacou,13W. Badgett,3 A. Barbaro-Galtieri,13V. E. Barnes,14B. A. Barnett,15S. Baroiant,16M. Barone,17G. Bauer,6F. Bedeschi,18S. Behari,15

S. Belforte,19W. H. Bell,20G. Bellettini,18J. Bellinger,21D. Benjamin,22A. Beretvas,3A. Bhatti,23M. Binkley,3 D. Bisello,12M. Bishai,3R. E. Blair,10C. Blocker,24K. Bloom,5B. Blumenfeld,15A. Bocci,23A. Bodek,25G. Bolla,14

A. Bolshov,6D. Bortoletto,14J. Boudreau,26C. Bromberg,27E. Brubaker,13J. Budagov,9H. S. Budd,25K. Burkett,3 G. Busetto,12K. L. Byrum,10S. Cabrera,22M. Campbell,5W. Carithers,13D. Carlsmith,21A. Castro,28D. Cauz,19 A. Cerri,13L. Cerrito,29J. Chapman,5C. Chen,4Y. C. Chen,7M. Chertok,16G. Chiarelli,18G. Chlachidze,3F. Chlebana,3

M. L. Chu,7J. Y. Chung,30W.-H. Chung,21Y. S. Chung,25C. I. Ciobanu,29A. G. Clark,31M. Coca,25A. Connolly,13 M. Convery,23J. Conway,32M. Cordelli,17J. Cranshaw,33R. Culbertson,3D. Dagenhart,24S. D’Auria,20P. de Barbaro,25

S. De Cecco,34S. Dell’Agnello,17M. Dell’Orso,18S. Demers,25L. Demortier,23M. Deninno,28D. De Pedis,34 P. F. Derwent,3C. Dionisi,34J. R. Dittmann,3A. Dominguez,13S. Donati,18M. D’Onofrio,31T. Dorigo,12N. Eddy,29

R. Erbacher,3D. Errede,29S. Errede,29R. Eusebi,25S. Farrington,20R. G. Feild,35J. P. Fernandez,14C. Ferretti,5 R. D. Field,1I. Fiori,18B. Flaugher,3L. R. Flores-Castillo,26G. W. Foster,3M. Franklin,36J. Friedman,6I. Furic,6 M. Gallinaro,23M. Garcia-Sciveres,13A. F. Garfinkel,14C. Gay,35D. W. Gerdes,5E. Gerstein,37S. Giagu,34P. Giannetti,18

K. Giolo,14M. Giordani,19P. Giromini,17V. Glagolev,9D. Glenzinski,3M. Gold,38N. Goldschmidt,5J. Goldstein,11 G. Gomez,39M. Goncharov,40I. Gorelov,38A. T. Goshaw,22Y. Gotra,26K. Goulianos,23A. Gresele,28C. Grosso-Pilcher,41

M. Guenther,14J. Guimaraes da Costa,36C. Haber,13S. R. Hahn,3E. Halkiadakis,25R. Handler,21F. Happacher,17 K. Hara,42R. M. Harris,3F. Hartmann,43K. Hatakeyama,23J. Hauser,44J. Heinrich,4M. Hennecke,43M. Herndon,15 C. Hill,2A. Hocker,25K. D. Hoffman,41S. Hou,7B. T. Huffman,11R. Hughes,30J. Huston,27C. Issever,2J. Incandela,2

G. Introzzi,18M. Iori,34A. Ivanov,25Y. Iwata,45B. Iyutin,6E. James,3M. Jones,14T. Kamon,40J. Kang,5 M. Karagoz Unel,46S. Kartal,3H. Kasha,35Y. Kato,47R. D. Kennedy,3R. Kephart,3B. Kilminster,25D. H. Kim,48 H. S. Kim,29M. J. Kim,37S. B. Kim,48S. H. Kim,42T. H. Kim,6Y. K. Kim,41M. Kirby,22L. Kirsch,24S. Klimenko,1 P. Koehn,30K. Kondo,8J. Konigsberg,1A. Korn,6A. Korytov,1J. Kroll,4M. Kruse,22V. Krutelyov,40S. E. Kuhlmann,10

N. Kuznetsova,3A. T. Laasanen,14S. Lami,23S. Lammel,3J. Lancaster,22K. Lannon,30M. Lancaster,49R. Lander,16 A. Lath,32G. Latino,38T. LeCompte,10Y. Le,15J. Lee,25S. W. Lee,40N. Leonardo,6S. Leone,18J. D. Lewis,3K. Li,35

C. S. Lin,3M. Lindgren,44T. M. Liss,29T. Liu,3D. O. Litvintsev,3N. S. Lockyer,4A. Loginov,50M. Loreti,12 D. Lucchesi,12P. Lukens,3L. Lyons,11J. Lys,13R. Madrak,36K. Maeshima,3P. Maksimovic,15L. Malferrari,28 M. Mangano,18G. Manca,11M. Mariotti,12M. Martin,15A. Martin,35V. Martin,46M. Martı´nez,3P. Mazzanti,28 K. S. McFarland,25P. McIntyre,40M. Menguzzato,12A. Menzione,18P. Merkel,3C. Mesropian,23A. Meyer,3T. Miao,3

R. Miller,27J. S. Miller,5S. Miscetti,17G. Mitselmakher,1N. Moggi,28R. Moore,3T. Moulik,14M. Mulhearn,6 A. Mukherjee,3T. Muller,43A. Munar,4P. Murat,3J. Nachtman,3S. Nahn,35I. Nakano,45R. Napora,15F. Niell,5 C. Nelson,3T. Nelson,3C. Neu,30M. S. Neubauer,6C. Newman-Holmes,3T. Nigmanov,26L. Nodulman,10S. H. Oh,22 Y. D. Oh,48T. Ohsugi,45T. Okusawa,47W. Orejudos,13C. Pagliarone,18F. Palmonari,18R. Paoletti,18V. Papadimitriou,33

J. Patrick,3G. Pauletta,19M. Paulini,37T. Pauly,11C. Paus,6D. Pellett,16A. Penzo,19T. J. Phillips,22G. Piacentino,18 J. Piedra,39K. T. Pitts,29R. Plunkett,3A. Pompo,14L. Pondrom,21G. Pope,26T. Pratt,11F. Prokoshin,9A. Pronko,1 J. Proudfoot,10F. Ptohos,17O. Poukhov,9G. Punzi,18J. Rademacker,11A. Rakitine,6F. Ratnikov,32H. Ray,5A. Reichold,11

P. Renton,11M. Rescigno,34F. Rimondi,28L. Ristori,18W. J. Robertson,22T. Rodrigo,39S. Rolli,51L. Rosenson,6 R. Roser,3R. Rossin,12C. Rott,14A. Roy,14A. Ruiz,39D. Ryan,51A. Safonov,16R. St. Denis,20W. K. Sakumoto,25

D. Saltzberg,44C. Sanchez,30A. Sansoni,17L. Santi,19S. Sarkar,34P. Savard,52A. Savoy-Navarro,3P. Schlabach,3 E. E. Schmidt,3M. P. Schmidt,35M. Schmitt,46L. Scodellaro,12A. Scribano,18A. Sedov,14S. Seidel,38Y. Seiya,42 A. Semenov,9F. Semeria,28M. D. Shapiro,13P. F. Shepard,26T. Shibayama,42M. Shimojima,42M. Shochet,41A. Sidoti,12 A. Sill,33P. Sinervo,52A. J. Slaughter,35K. Sliwa,51F. D. Snider,3R. Snihur,49M. Spezziga,33F. Spinella,18M. Spiropulu,2

L. Spiegel,3A. Stefanini,18J. Strologas,38D. Stuart,2A. Sukhanov,1K. Sumorok,6T. Suzuki,42R. Takashima,45 K. Takikawa,42M. Tanaka,10M. Tecchio,5R. J. Tesarek,3P. K. Teng,7K. Terashi,23S. Tether,6J. Thom,3 A. S. Thompson,20E. Thomson,30P. Tipton,25S. Tkaczyk,3D. Toback,40K. Tollefson,27D. Tonelli,18M. To¨nnesmann,27

H. Toyoda,47W. Trischuk,52J. Tseng,6D. Tsybychev,1N. Turini,18F. Ukegawa,42T. Unverhau,20T. Vaiciulis,25

0031-9007=05=94(17)=171802(6)$23.00 171802-1  2005 The American Physical Society

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A. Varganov, E. Vataga, S. Vejcik III, G. Velev, G. Veramendi, R. Vidal, I. Vila, R. Vilar, I. Volobouev, M. von der Mey,44R. G. Wagner,10R. L. Wagner,3W. Wagner,43Z. Wan,32C. Wang,22M. J. Wang,7S. M. Wang,1 B. Ward,20S. Waschke,20D. Waters,49T. Watts,32M. Weber,13W. C. Wester III,3B. Whitehouse,51A. B. Wicklund,10 E. Wicklund,3H. H. Williams,4P. Wilson,3B. L. Winer,30S. Wolbers,3M. Wolter,51S. Worm,32X. Wu,31F. Wu¨rthwein,6 U. K. Yang,41W. Yao,13G. P. Yeh,3K. Yi,15J. Yoh,3T. Yoshida,47I. Yu,48S. Yu,4J. C. Yun,3L. Zanello,34A. Zanetti,19

F. Zetti,13and S. Zucchelli28 (CDF Collaboration)

1University of Florida, Gainesville, Florida 32611, USA

2University of California at Santa Barbara, Santa Barbara, California 93106, USA

3Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA

4University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

5University of Michigan, Ann Arbor, Michigan 48109, USA

6Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

7Institute of Physics, Academia Sinica, Taipei, Taiwan 11529, Republic of China

8Waseda University, Tokyo 169, Japan

9Joint Institute for Nuclear Research, RU-141980 Dubna, Russia

10Argonne National Laboratory, Argonne, Illinois 60439, USA

11University of Oxford, Oxford OX1 3RH, United Kingdom

12Universita di Padova, Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy

13Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

14Purdue University, West Lafayette, Indiana 47907, USA

15The Johns Hopkins University, Baltimore, Maryland 21218, USA

16University of California at Davis, Davis, California 95616, USA

17Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, I-00044 Frascati, Italy

18Istituto Nazionale di Fisica Nucleare, University and Scuola Normale Superiore of Pisa, I-56100 Pisa, Italy

19Istituto Nazionale di Fisica Nucleare, University of Trieste, Italy

20Glasgow University, Glasgow G12 8QQ, United Kingdom

21University of Wisconsin, Madison, Wisconsin 53706, USA

22Duke University, Durham, North Carolina 27708, USA

23Rockefeller University, New York, New York 10021, USA

24Brandeis University, Waltham, Massachusetts 02254, USA

25University of Rochester, Rochester, New York 14627, USA

26University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA

27Michigan State University, East Lansing, Michigan 48824, USA

28Istituto Nazionale di Fisica Nucleare, University of Bologna, I-40127 Bologna, Italy

29University of Illinois, Urbana, Illinois 61801, USA

30The Ohio State University, Columbus, Ohio 43210, USA

31University of Geneva, CH-1211 Geneva 4, Switzerland

32Rutgers University, Piscataway, New Jersey 08855, USA

33Texas Tech University, Lubbock, Texas 79409, USA

34Instituto Nazionale de Fisica Nucleare, Sezione di Roma, University di Roma I, ‘‘La Sapienza,’’ I-00185 Roma, Italy

35Yale University, New Haven, Connecticut 06520, USA

36Harvard University, Cambridge, Massachusetts 02138, USA

37Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA

38University of New Mexico, Albuquerque, New Mexico 87131, USA

39Instituto de Fisica de Cantabria, CSIC-University of Cantabria, 39005 Santander, Spain

40Texas A&M University, College Station, Texas 77843, USA

41Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA

42University of Tsukuba, Tsukuba, Ibaraki 305, Japan

43Institut fu¨r Experimentelle Kernphysik, Universita¨t Karlsruhe, 76128 Karlsruhe, Germany

44University of California at Los Angeles, Los Angeles, California 90024, USA

45Hiroshima University, Higashi-Hiroshima 724, Japan

46Northwestern University, Evanston, Illinois 60208, USA

47Osaka City University, Osaka 588, Japan

48Center for High Energy Physics: Kyungpook National University, Taegu 702-701, Korea; Seoul National University, Seoul 151-742, Korea; and SungKyunKwan University, Suwon 440-746, Korea

49University College London, London WC1E 6BT, United Kingdom

50Institution for Theoretical and Experimental Physics, ITEP, Moscow 117259, Russia

171802-2

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51Tufts University, Medford, Massachusetts 02155, USA

52Institute of Particle Physics, University of Toronto, Toronto M5S 1A7, Canada (Received 2 July 2004; published 5 May 2005)

We report the first largely model independent measurement of charged particle multiplicities in quark and gluon jets,Nq andNg, produced at the Fermilab Tevatron in pp collisions with a center-of-mass energy of 1.8 TeV and recorded by the Collider Detector at Fermilab. The measurements are made for jets with average energies of 41 and 53 GeV by counting charged particle tracks in cones with opening angles ofc0:28, 0.36, and 0.47 rad around the jet axis. The corresponding jet hardnessQEjetcvaries in the range from 12 to 25 GeV. AtQ19:2 GeV, the ratio of multiplicitiesrNg=Nq is found to be 1:640:17, where statistical and systematic uncertainties are added in quadrature. The results are in agreement with resummed perturbative QCD calculations.

DOI: 10.1103/PhysRevLett.94.171802 PACS numbers: 13.87.Fh, 12.38.Qk

We present a new measurement of charged particle multiplicities in quark and gluon jets that is largely inde- pendent of theoretical models of fragmentation. This inde- pendence is achieved by exploiting the difference in quark and gluon jet content of dijet events and jet events inpp collisions. The analysis is carried out in the dijet or jet center-of-mass frame, where the average jet ener- gies areEjet41and 53 GeV. Multiplicities are measured in restricted cones with c0:28, 0.36, and 0.47 rad, where c is the angle between the jet axis and the cone side. The results are compared to predictions based on perturbative QCD calculations carried out in the frame- work of the next-to-leading log approximation (NLLA) [1]

and its extensions [2 –5], supplemented with the hypothesis of local parton-hadron duality (LPHD) [6].

In QCD, quarks and gluons have different probabilities to emit gluons, and it is therefore expected that jets pro- duced by quarks and gluons will show a difference in their average hadron multiplicity. The NLLALPHD ap- proach views jet fragmentation as a predominantly pertur- bative QCD process. The NLLA calculations give the average number of partons, NpartonsY, in a small cone with opening anglecaround the jet direction as a function ofYlnQ=Qeff, whereQEjetcis the jet hardness and Qeffis the lowest allowed transverse momentum of partons with respect to the jet direction. The LPHD hypothesis assumes that hadronization occurs locally at the end of the parton shower development so that the properties of had- rons are closely related to those of the partons. For in- stance, the hadron and parton multiplicities are assumed to be related via a constant factor KLPHD, i.e., Nhadrons KLPHDNpartons, which is independent of the jet energy and of whether the jet originates from a quark or a gluon. In this approach, the ratio of hadron multiplicities in gluon and quark jets,rNg=Nq, is the same as the ratio of partons.

Various calculations for the latter ratio are presented in Fig. 1.

Measurements of multiplicity differences between quark and gluon jets have a long history, most of which comes from ee colliders. The earliest measurements of the ratio r were consistent with 1 [7,8]. Over the ten-year CERN LEP era, the reported values varied from r’1:1 to 1.5 [7]. For purposes of comparison, we show in Fig. 1

recent CLEO [9] and OPAL [10] data points. These are believed to be model independent and the least biased by jet-finding algorithms [7]. The range ofee results mo- tivates an independent measurement of r in a different environment such as pp collisions. The charged particle multiplicities in gluon and quark jets,NgandNq, respec- tively, as well as their ratior, can be extracted by compar- ing the multiplicities in two data samples with very different fractions of gluon jets; thus, we do not have to discriminate between quark and gluon jets when selecting events. Two such samples used in the analysis are dijet and jet events, for which

Njj fgjjNg 1fjjgNq; (1) Njfjg Ng 1fgjNq; (2) whereNjj andNjare the average charged particle multi- plicities per jet in, respectively, dijet and jet events, and fgjj and fjg are fractions of gluon jets in dijet and jet events. To take into account the contamination of jet events by fake photons, Eq. (2) must be modified as follows:

Q, GeV

10 100

r=Ng/Nq

0 1 2 3

Capella et al., 2000 Lupia & Ochs, 1998 Catani et al., 1992 Gaffney & Mueller, 1985

CLEO OPAL

CDF, Ejet= 53 GeV CDF, Ejet= 41 GeV NLLA limit, r=CA/CF=2.25

FIG. 1 (color online). The ratio of charged particle multiplic- ities in gluon and quark jets as a function of jet hardness Q, which is QEjetc for CDF data and QEc:m:2Ejet for eedata [9,10]. CDF results (this Letter) are obtained for cone sizesc0:28, 0.36, and 0.47 rad. The NLLA curves [2 –5] are calculated using Qeff230 MeV [17]. The asymptotic value (Q! 1 [20]) ofr is simply the ratio of the gluon and quark color factors,CA3andCF4=3, respectively.

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Njfg Ng 1fg Nq 1Nfj; (3) whereis the fraction of real photons among the photon candidates, andNfjis the multiplicity in the jet opposite to the fake photon.

The current results are based on events produced inpp collisions with center-of-mass energy

ps

1:8 TeV and recorded by the Collider Detector at Fermilab (CDF) dur- ing the 1993–1995 run period. The integrated luminosity is 957 pb1. The CDF detector is described elsewhere [11]. The CDF coordinate system is defined with respect to the proton beam direction (z >0). The azimuthal angle is measured around thezaxis. The pseudorapidity lntan=2is used in place of the polar angle. The transverse energy is defined asET Esin.

In this measurement, the jets are defined by a cone

algorithm with cone radius R

'2 '2 p 0:7;

full details can be found in [12]. Corrections are applied to the raw jet energy in the cone to compensate for the nonlinearity and nonuniformity of the energy response of the calorimeter, to subtract the energy deposited in the jet cone by sources other than the initial parton (underlying event, multiple interactions, etc.), and to add the energy radiated by the initial parton out of the jet cone (out-of- cone correction). Both jet direction and energy are derived from the calorimeter information alone. The overall uncer- tainty on the jet energy scale is5%. To evaluate possible biases that might originate from the particular choice of jet-finding algorithm, we studied the properties of jets reconstructed by using smaller (R0:4) and larger (R 1:0) cones. Variations are taken as an estimate of the corresponding systematic uncertainty.

The dijet sample is accumulated by using the inclusive jet trigger withET threshold 20 GeV. The trigger is pre- scaled by 1000. Thejet sample is collected using the inclusive photon triggers with thresholds of 23 and 50 GeV onET.

The dijet events are required to have two jets balanced in PT: jP~T1P~T2j=PT1PT2<0:15(2!PT). Only events with both jets in the central region of the detector (j1;2j<

0:9) are retained to ensure efficient track reconstruction.

The events are required to have no more than two well- reconstructed primary vertices. For events with two pri- mary interactions, all tracks are associated with vertices by their proximity. The separation between vertices along the beam line is required to be larger than 12 cm (12!zfor tracks) to allow for unambiguous assignment of tracks. The vertex that has the largest)PT of tracks from cones with R0:7 around the jet directions is taken to be the one associated with the hard collision.

The jet events must pass exactly the same cuts (treating the photon as one of two jets) and satisfy specific photon identification requirements. A cut on the fraction of energy of the photon candidate observed in the hadronic calorimeter,EHA=Etotal<0:125, is applied to suppress the hadronic background. The selected events are required to

have exactly one photon candidate withET>20 GeVand no more than 1 GeV of extra transverse energy in a cone of R0:4around the photon candidate. The last requirement is the photon isolation cut. Events are rejected if they have tracks pointing to the photon candidate cluster. The elec- tromagnetic transverse shower profile measured by the shower maximum detector has to be consistent with that of a single photon.

For our data sample, the jet energy resolution is13%

and the photon energy resolution is 3%. Applying the same energy balance cut to dijet andjet events could lead to a small difference between jets from these samples.

To evaluate this effect we use a tighter cut for jet events:jP~T1P~T2j=PT1PT2<0:125. Variations in the results are found to be small and are conservatively taken as estimates of the associated systematic uncertainty. The results of the analysis also do not show any significant dependence on the number of primary vertices or on the photon isolation cut.

The selected events are then subdivided into two bins according to invariant mass, which is defined as M

E1E22=c4 P~1P~22=c2 q

, where Ei and P~i are the jet or photon energy and momentum and jets are treated as massless objects. The bins have a width chosen to be greater than the dijet mass spread due to the calorimeter resolution, MM ’10%. In the lower bin (72–94 GeV=c2), our sample consists of 3602 dijet and 2526jet events with an average invariant mass of 82 GeV=c2. The other bin (94–120 GeV=c2) has 1768 dijet and 910 jet events with an average invariant mass of 105 GeV=c2. The analysis is carried out in the dijet (orjet) center- of-mass frame, so thatEjetMc2=2. The results are cor- rected for a small difference (<1 GeV) in the average invariant mass of dijet and jet events. This difference is an effect of the jet trigger threshold. The small correction of <1% is taken as an estimate of the corresponding systematic uncertainty.

The fractions of gluon jets in dijet events, fjjg, and pure -jet events, fjg , are determined from HERWIG 5.6 and PYTHIA 6.115 [13] Monte Carlo generators with parton distribution function (PDF) sets [14] CTEQ4M, CTEQ4A2, and CTEQ4A4. Typical values are found to befgjj60%andfgj20%. The systematic uncertainty of 2% on these fractions is estimated from the differ- ences observed with the two Monte Carlo generators and three different PDF sets.

To estimate the fraction of real photons among photon candidates, we use a procedure described in [15].

The fraction is found to be 75%7% and 90%10%

for events with Ejet41 and 53 GeV, respectively. The method is based on measuring the fraction of events with conversions in the material in front of the calorimeter. Fake photons are mostly energetic$0’s or’s from one of the jets in a dijet event. Therefore fakes, being two almost collinear photons, have a higher conversion probability 171802-4

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than does a single prompt photon. The uncertainty in the fraction of real photons, , is taken into account in evaluating the corresponding systematic uncertainty in our measurements.

To measure the multiplicity of charged particles as- sociated with jets in dijet and jet events (Njj and Nj), we count three-dimensionally reconstructed tracks and use vertex cuts on the impact parameter,d, and'z jztrackzvertexj[16]. These cuts exclude tracks originating from secondary interactions in the same bunch crossing, conversions, K0S and - decays, cosmic rays, and other backgrounds. The vertex cuts are varied to study the sys- tematic uncertainties associated with them. After applying all the vertex cuts, there still remains a small number of tracks due toconversions andK0Sor-decays, which is estimated usingHERWIG5.6 and the CDF detector simula- tion package. The corrections are typically 3:5% ( conversions) and 4% (decays) of the measured multi- plicity. The systematic uncertainties assigned to these cor- rections are equal to their magnitudes.

The measured multiplicities are corrected for track re- construction inefficiency. The inefficiency was studied by embedding tracks found in one jet into the opposite jet at the hit level and redoing the full track reconstruction [17].

The size of these corrections on average multiplicities is 6% –8%, depending on the jet energy and cone sizec. The associated systematic uncertainties are estimated by vary- ing the tightness of the criteria used in matching the parameters of the embedded tracks to those of the re- reconstructed tracks.

Tracks coming from the underlying event and multiple interactions in the same bunch crossing (with unresolvedz vertices) are subtracted on average using complementary cones. A pair of complementary cones is defined such that their axis is in the plane normal to the dijet direction and at the same polar angle as the dijet axis. These cones are assumed to collect statistically the same uncorrelated back- ground as the cones around the jets. This correction varies with cone size from 0.2 to 0.5 tracks per cone.

We also apply a correction for losses of very low PT tracks due to bending in the magnetic field of the solenoid.

The efficiency for reconstructing tracks with PT <

200 MeV=cis almost zero. The correction obtained from the HERWIG simulation is typically less than 2%. The systematic uncertainty on this correction is taken to be the correction itself.

The charged particle multiplicity in the jet opposite to the fake photon, Nfj, is estimated based on Monte Carlo studies of fake jet events. It is found that fake pho- tons, on average, carry only 90% of the original jet energy (mainly because fake photons can be accompanied by other particles from the original jet), which results in mismeasurement of the event invariant mass by 5%.

Such events have a true invariant mass higher than it would appear in the analysis and, consequently, the jets have higher multiplicities. We estimate Nfjby considering the ratio'Nfj=Njj usingHERWIGandPYTHIA, and by tak- ing the dijet data sample and shifting the energy of one of the jets down by 10% to mimic a fake photon. The average of all three methods gives'’1:04. The spread in values of '(1:3%) is used to estimate the corresponding sys- tematic uncertainty.

The major sources of systematic uncertainty in the mea- surement of charged particle multiplicity in quark and gluon jets are as follows: background track removal, 7% –10%; jet-finding algorithm, 1% –7%; jet energy mea- surements, 2% –5%; and photon sample purity, 1% – 4%.

The major sources of systematic uncertainty in the mea- surement of the ratio, r, are as follows: jet energy mea- surements, 4% – 9%; photon sample purity, 4% – 6%; track cuts and corrections, 3% –6%; and energy balance, 1% – 5%. The individual systematic uncertainties for results with different jet hardnesses are strongly correlated.

The average multiplicities of charged particles in gluon and quark jets,NgandNq, for two different jet energies and three opening angles, as well as their ratior, are summa- rized in Table I and presented in Figs. 1 and 2. The ratio agrees well with resummed perturbative QCD calculations, 1:4r1:8[2 –5], and is consistent with recent results from OPAL,r’1:5[10]. The ratio is also in good agree- ment with the previous CDF model-dependent measure- ment,r1:70:3[18]. From Fig. 1, one can see that the ratio r tends to increase with energy scale. This trend is statistically significant, because both statistical and sys- tematic uncertainties are strongly correlated. At jet energy Ejet41 GeVand opening anglesc 0:28and 0.47 rad (Q11:5 and 19.2 GeV), we find'rr19:2 GeV r11:5 GeV 0:120:02stat 0:05syst. The aver- age charged particle multiplicities follow the predicted evolution with jet energy and opening angle as a function of QEjetc. To fit our data, we use the recent NLLA expressions [4] with the normalization constant as the only TABLE I. Charged-particle multiplicities in small cones around gluon and quark jet directions and their ratio: Ng,Nq, and r Ng=Nq, respectively. Multiplicities do not include charged particles fromK0S and-decays.

Ejet 41 GeV 52.5 GeV

Cone size,c 0.28 rad 0.36 rad 0.47 rad 0.28 rad 0.36 rad 0.47 rad

QEjetc 11.5 GeV 14.7 GeV 19.2 GeV 14.7 GeV 18.9 GeV 24.7 GeV

Ng 4:980:070:52 6:020:080:55 6:940:080:58 5:940:120:69 7:020:130:72 8:080:140:72

Nq 3:280:110:37 3:700:110:40 4:230:120:47 3:700:170:43 4:220:180:49 4:860:190:57

rNNg

q 1:520:080:13 1:630:090:14 1:640:090:14 1:600:120:19 1:660:130:20 1:660:130:18

(7)

free parameter (the other parameter,Qeff, is set to 230 MeV [17]). The fits for gluon and quark jet data points are independent. One can see that the ee results, except for CLEO data points around 5–7 GeV, fall within the fit bands.

We comparePYTHIA6.115 andHERWIG 5.6 predictions with the results of this analysis. For the range of jet hard- ness, Q, used in our analysis, both HERWIG and PYTHIA

predict the ratio r to be 1.2 –1.4. PYTHIA systematically gives 3%–4% higher multiplicities than does HERWIG. Both Monte Carlo generators are found to reproduce the gluon jet multiplicities fairly well, but they systematically overestimate the multiplicities in quark jets by as much as 30%(2!systdiscrepancy).

In summary, we have measured the multiplicities in gluon and quark jets and their ratio,rNg=Nq, for aver- age jet energiesEjet41and 53 GeV and opening angles c0:28, 0.36, and 0.47 rad. The results are found to agree with the resummed NLLA calculations and are con- sistent with recentee measurements [9,10,19].

We are grateful to Yu. Dokshitzer, I. Dremin, V. Khoze, A. H. Mueller, V. Nechitailo, W. Ochs, R. Peschanski, and B. Webber for a number of very fruitful discussions. We thank the Fermilab staff and the technical staffs of the

participating institutions for their vital contributions. This work was supported by the U.S. Department of Energy and National Science Foundation; the Italian Istituto Nazionale di Fisica Nucleare; the Ministry of Education, Culture, Sports, Science and Technology of Japan; the Natural Sciences and Engineering Research Council of Canada;

the National Science Council of the Republic of China; and the A. P. Sloan Foundation.

[1] Yu. Dokshitzer, V. Khoze, A. Mueller, and S. Troyan, Basics of Perturbative QCD, edited by J. Tran Thanh Van (Editions Frontie`res, Gif-sur-Yvette, 1991).

[2] J. B. Gaffney and A. H. Mueller, Nucl. Phys.B250, 109 (1985).

[3] S. Cataniet al., Nucl. Phys.B377, 445 (1992).

[4] A. Capellaet al., Phys. Rev. D61, 074009 (2000).

[5] S. Lupia and W. Ochs, Phys. Lett. B418, 214 (1998).

[6] Ya. I. Azimov, Yu. Dokshitzer, V. Khoze, and S. Troyan, Z. Phys. C27, 65 (1985);31, 213 (1986).

[7] I. M. Dremin and J. W. Gary, Phys. Rep.349, 301 (2001).

[8] V. Khoze et al., in At the Frontier of Particle Physics:

Handbook of QCD, edited by M. A. Shifman (World Scientific, Singapore, 2001), Vol. 2, p. 1101.

[9] M. S. Alamet al., Phys. Rev. D56, 17 (1997).

[10] G. Abbiendiet al., Eur. Phys. J. C11, 217 (1999).

[11] F. Abeet al., Nucl. Instrum. Methods Phys. Res., Sect. A 271, 387 (1988), and references therein.

[12] F. Abeet al., Phys. Rev. D45, 1448 (1992).

[13] HERWIG: G. Marchesini et al., Comput. Phys. Commun.

67, 465 (1992);PYTHIA: T. Sjo¨strandet al.,ibid.135, 238 (2001).

[14] H. L. Laiet al., Phys. Rev. D55, 1280 (1997).

[15] D. Acostaet al., Phys. Rev. D65, 112003 (2002).

[16] The impact parameter, d, is the shortest transverse dis- tance between the interaction point and the particle tra- jectory. The'zis the difference between thezposition of the track at the point of its closest approach to the beam line and the position of the primary vertex. We use the same cuts ondand'zas in [17,18].

[17] D. Acostaet al., Phys. Rev. D68, 012003 (2003).

[18] T. Affolderet al., Phys. Rev. Lett.87, 211804 (2001).

[19] Mark II Collaboration, P. C. Rowson et al., Phys. Rev.

Lett.54, 2580 (1985); TPC Collaboration, H. Aiharaet al., Phys. Lett. B 184, 299 (1987); CLEO Collaboration, M. S. Alam et al., Phys. Rev. D 46, 4822 (1992); SLD Collaboration, K. Abe et al., Phys. Lett. B 386, 475 (1996); DELPHI Collaboration, P. Abreu et al., Eur.

Phys. J. C6, 19 (1999); Phys. Lett. B 479, 118 (2000);

492, 398(E) (2000); OPAL Collaboration, K. Ackerstaff et al., Eur. Phys. J. C1, 479 (1998); G. Abbiendiet al., Phys. Lett. B550, 33 (2002).

[20] S. J. Brodsky and J. F. Gunion, Phys. Rev. Lett.37, 402 (1976); K. Konishi, A. Ukawa, and G. Veneziano, Nucl.

Phys.B157, 45 (1979).

0 5 10 15 20 25 30 35 40 45

10 102

Q, GeV Charged particle multiplicity, 2Ng and 2Nq

uds-quark jets:

OPAL DELPHI LEP-1 & SLD MARK-2 & TPC CDF, quark jets 3NLLA fit (CDF data), quarks

Gluon jets:

OPAL CLEO CDF, gluon jets

3NLLA fit (CDF data), gluons

FIG. 2 (color online). Average charged particle multiplicities in gluon and quark jets as a function of jet hardnessQ, which is QEjetcfor CDF data andQEc:m:2Ejetforeedata.

For the purpose of comparison to the ee measurements [9,10,19], CDF results on this plot include charged particles fromKS0 and- decays and are multiplied by two. The fits to CDF data are obtained by using the recent NLLA expressions [4]

(see text). The width of the bands corresponds to the uncertainty in the overall normalization.

171802-6

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