Study of Dimuon Production in Photon-Photon Collisions and Measurement of QED Photon Structure Functions at LEP

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Functions at LEP

P. Abreu, W. Adam, T. Adye, P. Adzic, I. Azhinenko, Z. Albrecht, T. Alderweireld, G.D. Alekseev, R. Alemany, T. Allmendinger, et al.

To cite this version:

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24February2000

Study of Dimuon Production in

Photon-Photon Collisions and

Measurement of QED Photon

Structure Functions at LEP

DELPHI Collaboration

Abstract

Muon pair production in the process e+_e,

! e+e

,+, is studied using the data taken at LEP1 (p

s ' mZ) with the DELPHI detector during the years 1992-1995. The corresponding integrated luminosity is 138.5 pb,1. The QED predictions have been tested over the whole Q2 _{range accessible at LEP1 (from}

several GeV2_=c4_{to several hundred GeV}2_=c4_{) by comparing}

experimentaldistri-butions with distriexperimentaldistri-butions resulting from Monte Carlo simulations using various generators. Selected events are used to extract the leptonic photon structure function F₂ _{. Azimuthal correlations are used to obtain information on}

addi-tional structure functions, F

A and FB , which originate from interference terms

of the scattering amplitudes. The measured ratios F

A=F2 and FB =F2 are

sig-nicantly dierent from zero and consistent with QED predictions.

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E.G.Anassontzis, P.Andersson , A.Andreazza , S.Andringa , P.Antilogus , W-D.Apel , Y.Arnoud , B.Asman , J-E.Augustin26, A.Augustinus9, P.Baillon9, P.Bambade20, F.Barao22, G.Barbiellini48, R.Barbier26, D.Y.Bardin17,

G.Barker18, A.Baroncelli40, M.Battaglia16, M.Baubillier24, K-H.Becks54, M.Begalli6, A.Behrmann54, P.Beilliere8,

Yu.Belokopytov9, N.C.Benekos33, A.C.Benvenuti5, C.Berat15, M.Berggren24, D.Bertrand2, M.Besancon41, M.Bigi47,

M.S.Bilenky17, M-A.Bizouard20, D.Bloch10, H.M.Blom32, M.Bonesini29, M.Boonekamp41, P.S.L.Booth23,

A.W.Borgland4, G.Borisov20, C.Bosio43, O.Botner50, E.Boudinov32, B.Bouquet20, C.Bourdarios20, T.J.V.Bowcock23,

I.Boyko17, I.Bozovic12, M.Bozzo14, M.Bracko45, P.Branchini40, R.A.Brenner50, P.Bruckman9, J-M.Brunet8, L.Bugge34,

T.Buran34, B.Buschbeck52, P.Buschmann54, S.Cabrera51, M.Caccia28, M.Calvi29, T.Camporesi9, V.Canale39,

F.Carena9, L.Carroll23, C.Caso14, M.V.Castillo Gimenez51, A.Cattai9, F.R.Cavallo5, V.Chabaud9, Ph.Charpentier9,

P.Checchia37, G.A.Chelkov17, R.Chierici47, P.Chliapnikov9;44, P.Chochula7, V.Chorowicz26, J.Chudoba31, K.Cieslik19,

P.Collins9, R.Contri14, E.Cortina51, G.Cosme20, F.Cossutti9, H.B.Crawley1, D.Crennell38, S.Crepe15, G.Crosetti14,

J.Cuevas Maestro35, S.Czellar16, M.Davenport9, W.Da Silva24, G.Della Ricca48, P.Delpierre27, N.Demaria9,

A.De Angelis48, W.De Boer18, C.De Clercq2, B.De Lotto48, A.De Min37, L.De Paula49, H.Dijkstra9, L.Di Ciaccio9;39,

J.Dolbeau8, K.Doroba53, M.Dracos10, J.Drees54, M.Dris33, A.Duperrin26, J-D.Durand9, G.Eigen4, T.Ekelof50,

G.Ekspong46, M.Ellert50, M.Elsing9, J-P.Engel10, M.Espirito Santo22, G.Fanourakis12, D.Fassouliotis12, J.Fayot24,

M.Feindt18, A.Fenyuk44, A.Ferrer51, E.Ferrer-Ribas20, F.Ferro14, S.Fichet24, A.Firestone1, U.Flagmeyer54, H.Foeth9,

E.Fokitis33, F.Fontanelli14, B.Franek38, A.G.Frodesen4, R.Fruhwirth52, F.Fulda-Quenzer20, J.Fuster51, A.Galloni23,

D.Gamba47, S.Gamblin20, M.Gandelman49, C.Garcia51, C.Gaspar9, M.Gaspar49, U.Gasparini37, Ph.Gavillet9,

E.N.Gazis33, D.Gele10, N.Ghodbane26, I.Gil51, F.Glege54, R.Gokieli9;53, B.Golob9;45, G.Gomez-Ceballos42,

P.Goncalves22, I.Gonzalez Caballero42, G.Gopal38, L.Gorn1, Yu.Gouz44, V.Gracco14, J.Grahl1, E.Graziani40, P.Gris41,

G.Grosdidier20, K.Grzelak53, J.Guy38, C.Haag18, F.Hahn9, S.Hahn54, S.Haider9, A.Hallgren50, K.Hamacher54,

J.Hansen34, F.J.Harris36, V.Hedberg9;25, S.Heising18, J.J.Hernandez51, P.Herquet2, H.Herr9, T.L.Hessing36,

J.-M.Heuser54, E.Higon51, S-O.Holmgren46, P.J.Holt36, S.Hoorelbeke2, M.Houlden23, J.Hrubec52, M.Huber18, K.Huet2,

G.J.Hughes23, K.Hultqvist9;46, J.N.Jackson23, R.Jacobsson9, P.Jalocha19, R.Janik7, Ch.Jarlskog25, G.Jarlskog25,

P.Jarry41, B.Jean-Marie20, D.Jeans36, E.K.Johansson46, P.Jonsson26, C.Joram9, P.Juillot10, L.Jungermann18,

F.Kapusta24, K.Karafasoulis12, S.Katsanevas26, E.C.Katsous33, R.Keranen18, G.Kernel45, B.P.Kersevan45,

B.A.Khomenko17, N.N.Khovanski17, A.Kiiskinen16, B.King23, A.Kinvig23, N.J.Kjaer9, O.Klapp54, H.Klein9, P.Kluit32,

P.Kokkinias12, V.Kostioukhine44, C.Kourkoumelis3, O.Kouznetsov41, M.Krammer52, E.Kriznic45, Z.Krumstein17,

P.Kubinec7, J.Kurowska53, K.Kurvinen16, J.W.Lamsa1, D.W.Lane1, V.Lapin44, J-P.Laugier41, R.Lauhakangas16,

G.Leder52, F.Ledroit15, V.Lefebure2, L.Leinonen46, A.Leisos12, R.Leitner31, J.Lemonne2, G.Lenzen54, V.Lepeltier20,

T.Lesiak19, M.Lethuillier41, J.Libby36, W.Liebig54, D.Liko9, A.Lipniacka9;46, I.Lippi37, B.Loerstad25, J.G.Loken36,

J.H.Lopes49, J.M.Lopez42, R.Lopez-Fernandez15, D.Loukas12, P.Lutz41, L.Lyons36, J.MacNaughton52, J.R.Mahon6,

A.Maio22, A.Malek54, T.G.M.Malmgren46, S.Maltezos33, V.Malychev17, F.Mandl52, J.Marco42, R.Marco42,

B.Marechal49, M.Margoni37, J-C.Marin9, C.Mariotti9, A.Markou12, C.Martinez-Rivero20, F.Martinez-Vidal51,

S.Marti i Garcia9, J.Masik13, N.Mastroyiannopoulos12, F.Matorras42, C.Matteuzzi29, G.Matthiae39, F.Mazzucato37,

M.Mazzucato37, M.Mc Cubbin23, R.Mc Kay1, R.Mc Nulty23, G.Mc Pherson23, C.Meroni28, W.T.Meyer1, A.Miagkov44,

E.Migliore9, L.Mirabito26, W.A.Mitaro52, U.Mjoernmark25, T.Moa46, M.Moch18, R.Moeller30, K.Moenig9;11,

M.R.Monge14, D.Moraes49, X.Moreau24, P.Morettini14, G.Morton36, U.Mueller54, K.Muenich54, M.Mulders32,

C.Mulet-Marquis15, R.Muresan25, W.J.Murray38, B.Muryn19, G.Myatt36, T.Myklebust34, F.Naraghi15, M.Nassiakou12,

F.L.Navarria5, S.Navas51, K.Nawrocki53, P.Negri29, N.Neufeld9, R.Nicolaidou41, B.S.Nielsen30, P.Niezurawski53,

M.Nikolenko10;17, V.Nomokonov16, A.Nygren25, V.Obraztsov44, A.G.Olshevski17, A.Onofre22, R.Orava16, G.Orazi10,

K.Osterberg16, A.Ouraou41, M.Paganoni29, S.Paiano5, R.Pain24, R.Paiva22, J.Palacios36, H.Palka19,

Th.D.Papadopoulou9;33, K.Papageorgiou12, L.Pape9, C.Parkes9, F.Parodi14, U.Parzefall23, A.Passeri40, O.Passon54,

T.Pavel25, M.Pegoraro37, L.Peralta22, M.Pernicka52, A.Perrotta5, C.Petridou48, A.Petrolini14, H.T.Phillips38,

F.Pierre41, M.Pimenta22, E.Piotto28, T.Podobnik45, M.E.Pol6, G.Polok19, P.Poropat48, V.Pozdniakov17, P.Privitera39,

N.Pukhaeva17, A.Pullia29, D.Radojicic36, S.Ragazzi29, H.Rahmani33, J.Rames13, P.N.Rato21, A.L.Read34,

P.Rebecchi9, N.G.Redaelli28, M.Regler52, J.Rehn18, D.Reid32, R.Reinhardt54, P.B.Renton36, L.K.Resvanis3,

F.Richard20, J.Ridky13, G.Rinaudo47, I.Ripp-Baudot10, O.Rohne34, A.Romero47, P.Ronchese37, E.I.Rosenberg1,

P.Rosinsky7, P.Roudeau20, T.Rovelli5, Ch.Royon41, V.Ruhlmann-Kleider41, A.Ruiz42, H.Saarikko16, Y.Sacquin41,

A.Sadovsky17, G.Sajot15, J.Salt51, D.Sampsonidis12, M.Sannino14, Ph.Schwemling24, B.Schwering54, U.Schwickerath18,

F.Scuri48, P.Seager21, Y.Sedykh17, A.M.Segar36, N.Seibert18, R.Sekulin38, R.C.Shellard6, M.Siebel54, L.Simard41,

F.Simonetto37, A.N.Sisakian17, G.Smadja26, N.Smirnov44, O.Smirnova25, G.R.Smith38, A.Sopczak18, R.Sosnowski53,

T.Spassov22, E.Spiriti40, S.Squarcia14, C.Stanescu40, S.Stanic45, M.Stanitzki18, K.Stevenson36, A.Stocchi20, J.Strauss52,

R.Strub10, B.Stugu4, M.Szczekowski53, M.Szeptycka53, T.Tabarelli29, A.Taard23, O.Tchikilev44, F.Tegenfeldt50,

F.Terranova29, J.Thomas36, J.Timmermans32, N.Tinti5, L.G.Tkatchev17, M.Tobin23, S.Todorova10, A.Tomaradze2,

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N.van Remortel, I.Van Vulpen , G.Vegni , L.Ventura , W.Venus ; , F.Verbeure , P.Verdier , M.Verlato , L.S.Vertogradov17, V.Verzi39, D.Vilanova41, L.Vitale48, E.Vlasov44, A.S.Vodopyanov17, G.Voulgaris3, V.Vrba13,

H.Wahlen54, C.Walck46, A.J.Washbrook23, C.Weiser9, D.Wicke54, J.H.Wickens2, G.R.Wilkinson36, M.Winter10,

M.Witek19, G.Wolf9, J.Yi1, O.Yushchenko44, A.Zalewska19, P.Zalewski53, D.Zavrtanik45, E.Zevgolatakos12,

N.I.Zimin17;25, A.Zintchenko17, Ph.Zoller10, G.C.Zucchelli46, G.Zumerle37

1Department of Physics and Astronomy, Iowa State University, Ames IA 50011-3160, USA

2Physics Department, Univ. Instelling Antwerpen, Universiteitsplein 1, B-2610 Antwerpen, Belgium

and IIHE, ULB-VUB, Pleinlaan 2, B-1050 Brussels, Belgium

and Faculte des Sciences, Univ. de l'Etat Mons, Av. Maistriau 19, B-7000 Mons, Belgium

3Physics Laboratory, University of Athens, Solonos Str. 104, GR-10680 Athens, Greece 4Department of Physics, University of Bergen, Allegaten 55, NO-5007 Bergen, Norway

5Dipartimento di Fisica, Universita di Bologna and INFN, Via Irnerio 46, IT-40126 Bologna, Italy 6Centro Brasileiro de Pesquisas Fsicas, rua Xavier Sigaud 150, BR-22290 Rio de Janeiro, Brazil

and Depto. de Fsica, Pont. Univ. Catolica, C.P. 38071 BR-22453 Rio de Janeiro, Brazil

and Inst. de Fsica, Univ. Estadual do Rio de Janeiro, rua S~ao Francisco Xavier 524, Rio de Janeiro, Brazil

7Comenius University, Faculty of Mathematics and Physics, Mlynska Dolina, SK-84215 Bratislava, Slovakia 8College de France, Lab. de Physique Corpusculaire, IN2P3-CNRS, FR-75231 Paris Cedex 05, France 9CERN, CH-1211 Geneva 23, Switzerland

10Institut de Recherches Subatomiques, IN2P3 - CNRS/ULP - BP20, FR-67037 Strasbourg Cedex, France 11Now at DESY-Zeuthen, Platanenallee 6, D-15735 Zeuthen, Germany

12Institute of Nuclear Physics, N.C.S.R. Demokritos, P.O. Box 60228, GR-15310 Athens, Greece

13FZU, Inst. of Phys. of the C.A.S. High Energy Physics Division, Na Slovance 2, CZ-180 40, Praha 8, Czech Republic 14Dipartimento di Fisica, Universita di Genova and INFN, Via Dodecaneso 33, IT-16146 Genova, Italy

15Institut des Sciences Nucleaires, IN2P3-CNRS, Universite de Grenoble 1, FR-38026 Grenoble Cedex, France 16Helsinki Institute of Physics, HIP, P.O. Box 9, FI-00014 Helsinki, Finland

17Joint Institute for Nuclear Research, Dubna, Head Post Oce, P.O. Box 79, RU-101 000 Moscow, Russian Federation 18Institut fur Experimentelle Kernphysik, Universitat Karlsruhe, Postfach 6980, DE-76128 Karlsruhe, Germany 19Institute of Nuclear Physics and University of Mining and Metalurgy, Ul. Kawiory 26a, PL-30055 Krakow, Poland 20Universite de Paris-Sud, Lab. de l'Accelerateur Lineaire, IN2P3-CNRS, B^at. 200, FR-91405 Orsay Cedex, France 21School of Physics and Chemistry, University of Lancaster, Lancaster LA1 4YB, UK

22LIP, IST, FCUL - Av. Elias Garcia, 14-1o, PT-1000 Lisboa Codex, Portugal

23Department of Physics, University of Liverpool, P.O. Box 147, Liverpool L69 3BX, UK

24LPNHE, IN2P3-CNRS, Univ. Paris VI et VII, Tour 33 (RdC), 4 place Jussieu, FR-75252 Paris Cedex 05, France 25Department of Physics, University of Lund, Solvegatan 14, SE-223 63 Lund, Sweden

26Universite Claude Bernard de Lyon, IPNL, IN2P3-CNRS, FR-69622 Villeurbanne Cedex, France 27Univ. d'Aix - Marseille II - CPP, IN2P3-CNRS, FR-13288 Marseille Cedex 09, France

28Dipartimento di Fisica, Universita di Milano and INFN, Via Celoria 16, IT-20133 Milan, Italy 29Universita degli Studi di Milano - Bicocca, Via Emanuelli 15, IT-20126 Milan, Italy

30Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen , Denmark

31IPNP of MFF, Charles Univ., Areal MFF, V Holesovickach 2, CZ-180 00, Praha 8, Czech Republic 32NIKHEF, Postbus 41882, NL-1009 DB Amsterdam, The Netherlands

33National Technical University, Physics Department, Zografou Campus, GR-15773 Athens, Greece 34Physics Department, University of Oslo, Blindern, NO-1000 Oslo 3, Norway

35Dpto. Fisica, Univ. Oviedo, Avda. Calvo Sotelo s/n, ES-33007 Oviedo, Spain 36Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK

37Dipartimento di Fisica, Universita di Padova and INFN, Via Marzolo 8, IT-35131 Padua, Italy 38Rutherford Appleton Laboratory, Chilton, Didcot OX11 OQX, UK

39Dipartimento di Fisica, Universita di Roma II and INFN, Tor Vergata, IT-00173 Rome, Italy

40Dipartimento di Fisica, Universita di Roma III and INFN, Via della Vasca Navale 84, IT-00146 Rome, Italy 41DAPNIA/Service de Physique des Particules, CEA-Saclay, FR-91191 Gif-sur-Yvette Cedex, France 42Instituto de Fisica de Cantabria (CSIC-UC), Avda. los Castros s/n, ES-39006 Santander, Spain

43Dipartimento di Fisica, Universita degli Studi di Roma La Sapienza, Piazzale Aldo Moro 2, IT-00185 Rome, Italy 44Inst. for High Energy Physics, Serpukov P.O. Box 35, Protvino, (Moscow Region), Russian Federation

45J. Stefan Institute, Jamova 39, SI-1000 Ljubljana, Slovenia and Laboratory for Astroparticle Physics,

Nova Gorica Polytechnic, Kostanjeviska 16a, SI-5000 Nova Gorica, Slovenia, and Department of Physics, University of Ljubljana, SI-1000 Ljubljana, Slovenia

46Fysikum, Stockholm University, Box 6730, SE-113 85 Stockholm, Sweden

47Dipartimento di Fisica Sperimentale, Universita di Torino and INFN, Via P. Giuria 1, IT-10125 Turin, Italy 48Dipartimento di Fisica, Universita di Trieste and INFN, Via A. Valerio 2, IT-34127 Trieste, Italy

and Istituto di Fisica, Universita di Udine, IT-33100 Udine, Italy

49Univ. Federal do Rio de Janeiro, C.P. 68528 Cidade Univ., Ilha do Fund~ao BR-21945-970 Rio de Janeiro, Brazil 50Department of Radiation Sciences, University of Uppsala, P.O. Box 535, SE-751 21 Uppsala, Sweden

51IFIC, Valencia-CSIC, and D.F.A.M.N., U. de Valencia, Avda. Dr. Moliner 50, ES-46100 Burjassot (Valencia), Spain 52Institut fur Hochenergiephysik, Osterr. Akad. d. Wissensch., Nikolsdorfergasse 18, AT-1050 Vienna, Austria 53Inst. Nuclear Studies and University of Warsaw, Ul. Hoza 69, PL-00681 Warsaw, Poland

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1 Introduction

The study of the process e+_e,

!e+e

,+, provides a good way to test QED up to the fourth order of. The photon structure can be studied by measuring photon structure functions which can be extracted in the so-called \single tagged" mode (Fig. 1), where one of the scattered electrons1 _{is detected (\tagged") in an electromagnetic calorimeter}

while the other scattered electron goes undetected (\untagged"). This process can also be used as a reference one for studies of the hadronic structure function of the photon, providing a basis for a better understanding of the detector performance and for checking the analysis procedure.

Previous measurements of muon pair production in both the single tagged mode and the double tagged mode (where the scattered electron and positron are both detected) have shown good agreement with QED predictions [1{14], with one exception [9] where an excess of data events was observed in the double tag mode.

This study, based on the data collected by the DELPHI collaboration at LEP1 at centre-of-mass energies from 89.4 to 93 GeV, complements those results. It improves on previous DELPHI measurements of the leptonic photon structure function F

2 [11] by

in-cluding all the LEP1 statistics and increasing theQ2 _{coverage by an order of magnitude.}

This paper also presents results of studies of the azimuthal correlations, which are used to extract the ratios of the structure functions F

A=F2 and FB =F2 .

2 Event kinematics

In the single tagged mode, where the tagged and untagged electrons are scattered with polar angles tag and untag and energiesEtag and Euntag respectively, and the probe and

target photons have four-momenta q = (xtagEbeam;~q) and p = (xuntagEbeam;~p), the cross

section of the reaction e+_e,

!e+e

,X is given by [15]: d3

dxdQ2_dx_untag = dn(x_dx_untaguntag)

d2_(e!eX)

dxdQ2 : (1)

These two factors, the ux of target photons and the e cross section respectively, are given by: dn(xuntag) dxuntag = xuntag ( 1 + (1,xuntag) 2 ln 2Ebeam(1,xuntag) mexuntag sin max untag 2 ! ,1 +xuntag ) ; (2) d2_(e !eX) dxdQ2 = 2 2 xQ4 n 1 + (1,y) 2 F₂ _(x;Q2_;P2₎ ,y 2_F L(x;Q2;P2) o : (3) HereF₂ _and _F

L are structure functions of the photon, is the QED coupling constant,

Q2 ₌ ,q2 ' 4EtagEbeamsin

2₍_tag_{=2) is the squared 4-momentum transfer, P}2 ₌ ,p2 is the virtuality of the target photon, and x and y are the Bjorken variables

x = Q_2q 2 p = Q2 W2 +Q2₊P2; y = p q pk ' Q2 sxxuntag = 1, Etag Ebeam cos2 tag 2 (4)

where W2 = (q + p)2 _{is the invariant mass of the} _(or+,) system, k is the initial four-vector of the tagged electron, and s = 4E2beam.

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The structure function F2 can be extracted from the dependence of the cross section

on x and Q2_{. But} _F

L is small and is weighted by the small factor y2, making its direct

measurement impractical.

However, additional structure functions can be studied by looking at azimuthal cor-relations of the nal state particles. The dierential cross section of the process can be written as [16] d4_(e !e+ ,) dxdydcosd=4 = 22 Q2 1 + (1,y)2 xy

(2x ~FT +(y) ~FL),(y) ~FAcos + 12(y)~FBcos2

; (5) where is the azimuthal angle, dened in the centre-of-mass frame as the angle between the planes formed by the photon axis and the muon and the scattered electron respectively (Fig. 2), and is the angle between the muon and the photon axis. The functions (y) and (y) are given by (y) = (2,y)

p

1,y=(1 + (1,y)2) and (y) = 2(1 ,y)=(1 + (1,y)2) [17] and can be taken equal to 1 in the accessible kinematical region. The dierential structure functions ~FT, ~FL, ~FA, and ~FB give the corresponding

standard structure functions FT, FL, FA, and FB after integrating appropriately over

cos (see section 7.2) taking into account that F

A is antisymmetric in cos [18]. The cross section can then be written as

d3_(e !e+ ,) dxdyd=2 ' 22 Q2 1 + (1,y)2 xy F₂ 1,(F A=F2 )cos + 12(FB =F2 )cos2 : (6)

The structure functions F_i _{are combinations of transition amplitudes for the dierent}

helicity states of the photons. The structure function F

B is related to the interference

term between the two transverse helicity states of the photons. It is identical to F_L _,

which is related to the longitudinal polarization of the virtual photon, in leading order and for massless muons.

3 DELPHI detector

The DELPHI detector has been described in detail elsewhere [19,20]. In this analysis, the scattered electron was tagged using

the SmallAngle Tagger (SAT), the main luminositymonitor during 1991-93, covering polar angles from 2.5 to 8 (172 to 177.5); it was made of alternating layers of lead sheets (0.9 mm thick) and plastic scintillator bres (1 mm in diameter), aligned parallel to the beam;

the Small angle TIle Calorimeter (STIC), the main luminosity monitor since 1994, covering polar angles from 1.7 to 10.3 (169.7 to 178.3); the STIC is a sampling calorimeter with 49 sandwiches of 3.4 mm steel-laminated lead plates and 3 mm thick scintillator tiles giving a total thickness of 27 radiation lengths;

the Forward ElectroMagnetic Calorimeter (FEMC) covering from 10

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The energy resolution of the tagging calorimeters was around 5% in SAT and FEMC and 3% in STIC for an incident electron energy of 45 GeV.

For muon identication, DELPHI contained barrel and forward muon detectors, each consisting of at least 4 layers of drift chambers. The muon chambers covered 78% of the solid angle.

Combining the information from the tracking detectors, the relative momentum reso-lution p=p varied from 0.001p to 0.01p (p in GeV/c), depending on the polar angle of the charged particle.

4 Monte Carlo simulation

Two event generators were used in order to simulate the signal process e+_e, ! e+_e,+,: BDKRC [21] which includes only the multiperipheral diagram (Fig.1) to-gether with QED radiative corrections, and DIAG36 [22] which lacks the QED radiative corrections but includes also the bremsstrahlung, annihilation and conversion diagrams. DIAG36 was used to check the role of these additional diagrams.

Several generators were used to estimate the backgrounds to the process studied: BDKRC [21] was used to simulatee+_e,

!e

+_e,+,, TWOGAM [23] to simulatehadron production in two-photon collisions, DYMU3 [24] for the e+_e,

!

+,( ) process, and KORALZ [25] fore+_e,

!+

,( ).

The generated events were passed through the full simulation of the DELPHI detector and reconstructed using the same program as for the data.

5 Event selection and correction

Events were selected as single tagged dimuon candidates if the following requirements were met.

There was a cluster in one of the electromagnetic calorimeters with an energy deposi-tion greater than 0.6Ebeam (hereafter called the tagged electron). If the cluster lay within the polar angle range 20 - 160, it was linked to a detected charged particle. There were exactly two additional particles with opposite charges and polar angles between 20 and 160. The relative errors on their momenta were less than 1. Their impact parameters with respect to the average interaction point were below 4 cm in the transverse plane and 10 cm along the beam. Their track lengths seen in the tracking detectors were at least 30 cm. Their momenta were above 0.5 GeV/c and 2.5 GeV/c and the sum of their momenta was below 30 GeV/c.

At least one of the additional particles with a momentum greater than 2.5 GeV/c was identied as a muon by the DELPHI standard muon tagging algorithm [20]. The invariant mass of the two additional particles was above 1.7 GeV/c

2_{. This}

requirement reduced the contribution from diagrams other than the multiperipheral one to below 0.25% for the low Q2 _{and 2% for the high} _Q2 _{sample according to the}

DIAG36 generator, and avoided possible problems with the soft part of the spectrum due to trigger or muon tagging ineciency.

Finally, double-tagged eventswere rejected by requiring there to be no energy deposit exceeding 0.3Ebeamin the detector arm (dened as = 0

,90

and = 90

,180

)

opposite that containing the tagged electron.

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In order to improve the measurements of the tagged electron parameters (energy and angles), the following procedures were used.

1. To avoid edge eects, the tagged electron was required to lie in the polar angle range 3 < < 7:6 (172:4 < < 177) for the SAT, 2:5 < < 9 (171 < < 177:5) for the STIC, or 11 < < 35 (145 < < 169) for the FEMC.

2. To improvethe measurementsin the SAT, which had a limitedgranularity, the radi-al position of the cluster was corrected using the function found from the comparison of the experimental radial distribution for Bhabha events with the theoretical one based on a 1=3 _{cross section dependence (Fig. 3). This improved the} _Q2 _resolution

from 6.0% to 2.9%.

3. To improvethe measurementsin the SAT and STIC, their alignments were checked using Bhabha event samples. The detector on the electron side had a mask in front of it to better dene the acceptance at low. From the number of Bhabha events as a function of the electron azimuthalangle1, it was possible to nd the displacementof

the mask relative to the beam line. The alignment on the opposite side was checked by looking at the dierence of the measured polar anglestag,untag of the scattered electron and positron as a function of the positron azimuthal angle 2 (Fig. 4). The

dependencies observed were used to correct the measured polar angles. The errors of the tted parameters were taken as uncertainties of the procedure, contributing 0.5% uncertainty on low values of Q2_.

4. A more accurate value of the tagged electron energy Etag was calculated from the

requirements of energy and longitudinal momentum conservation in the event: Etag = Pcos+ (2Ebeam,E)cosuntag

cosuntag ,costag

; (7)

where P, E and are the momentum, energy and polar angle of the muon

system, and untag is the polar angle of the untagged electron, assumed to be 0

or . The improvement due to this method can be seen in Fig. 5, obtained from simulation, where the dierence between the reconstructed and true (generated) tag energy Etag,E

gen

tag is shown as a function of the tag angle tag using both the direct

measurement of Etag and this method.

6 Background

The following sources of background to the +, event samples were considered:

e+e

,

! e+e

,+, with a decay product identied as a muon. The background from this process was found to be (1.20.2)% for the SAT and STIC tagged samples and (5.71.1)% for the FEMC, where the errors quoted are statistical.

e+e

,

!+

,( ) with a hard radiated photon or a decay product faking a tagged electron. This background was found to be negligible for the SAT and STIC samples, and (8.91.9)% for the FEMC, after taking into account the on-peak versus o-peak luminosity distribution of the data.

e+e

,

!+

,( ) with the radiated photon faking a tagged electron. This was found to be negligible due to the 30 GeV cut on the sum of the muon momenta.

e+e

,

! e+e

,+, with a pion misidentied as a muon. The ratio of the cross sections for pion pair and muon pair production in two-photon interactions falls to (1-5)% if the invariant mass of the produced pair is above 2.0 GeV/c2_{[26]. With the}

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as a muon was below 1.5% (depending on the pion momentum), so this background was also negligible for all samples.

other e

+_e,

!e

+_e,+hadrons processes. These were also found to be negligible for all event samples.

untagged e

+_e,

!e

+_e,+, in coincidence with an o-momentum electron faking a tagged electron. The o-momentum electrons are beam electrons that have scat-tered o residual gas molecules inside the beam pipe. Using a method similar to the one described in [27], this background was estimated from Z0 ! events in coincidence with a similar o-momentum electron, multiplying by the ratio of the dimuon production cross sections from untagged two-photon interactions and from Z0 _{decays, and was also found to be negligible.}

7 Results

The numbers of selected data events after background subtraction are compared with the predictions of the signal Monte Carlo simulations in Table 1. TheQ2 _{ranges shown are}

calculated given the angular coverage of the detectors and the cut on the tag energy, and the average values< Q2_{> are taken from the data. Figs. 6 { 8 present the distributions of}

a standard set of observables for events tagged by the SAT, STIC and FEMC respectively.

Tagging detector SAT STIC FEMC

Q2 _{range (GeV}2_=c4_{) 3.4},36.6 2.4,51.2 45.9,752.8 < Q2 _>) (GeV2=c4) 13.0 12.1 120.0) data 135737 287554 23918 BDKRC simulation 136214 288422 2506 DIAG36 simulation 129825 278555 23613 ) After requiring E

tag> 0:75Ebeam (see text) ) For events with

tag< 25 (

tag> 155) (see text) Table 1: Numbers of selected events after background subtraction.

Table 1 and Figs. 6 - 8 show that the BDKRC and DIAG36 generators produce similar kinematical distributions, but DIAG36 gives somewhat lower numbers of selected events. In the kinematical region under study, the contribution of the additional diagrams in DIAG36 was found to be very small (see section 5). This dierence (if real) should therefore be attributed to the eect of radiative corrections. The BDKRC generator was therefore used for the structure function studies below.

7.1 Extraction of

F

2

To extract F

2, the experimental x distribution was divided by the Monte Carlo

dis-tribution weighted by the factor =F₂ _(x;Q2_{), where} _F₂ _(x;Q2_{) can be obtained from a}

simulated event sample using either a generator producing events according to a givenF2

or the photon ux approach described, for example, in [13] and brie y outlined below. It follows from Eqs. (1-3) that, neglecting the small contribution from y2 _terms:

F₂ _(x;Q2_;P2_{) = d}2

dxdQ2=W(x;Q

(10)

where the weight (x;Q ) is given by W(x;Q 2_{) = 4}2 xQ4 xmax_untag Z xmin_untag dn(xuntag) dxuntag (1,y) dxuntag: (9) To calculate the integration limits, the fractional energy of the target photon is extracted from the expressions for x and W :

xuntag = 2Q2=sx,2Q2=s + cos + cosuntag,xtag(1 + cos) cos + cosuntag+xtag(1,cos)

; (10)

where

cos = sintagsinuntagcos(),costagcosuntag; (11) and is the azimuthal angle between the scattered e+ _and _e,. In the single tag approximation,untag '0 so that (10) becomes:

xuntag = 2Q2=sx,2Q2=s,costag+ 1,xtag(1,costag) ,costag+ 1 +xtag(1 + costag)

: (12)

The maximum and minimum xuntag values correspond to the minimum and maximum

xtag values, and these result from the tagging conditions:

xmax_tag _{= min}

( 1,

E_tagmin

Ebeam;1,

Q2

ssin2₍max_tag ₌₂₎

)

; xmin_tag _{= max}

( W2

s ;1,

Q2

ssin2₍min_tag ₌₂₎

)

(13) whereE_tagmin_{is the lower cut on the tag energy and}_tagmin₍max_tag _{) is the lower (upper) angular}

acceptance of the tagging device. E_tagmin _{was increased from 0:6}Ebeam to 0:75Ebeam in order to keep the y2 _{contribution small.}

Fig. 9 shows the F₂ _{(x) values obtained by both methods for a simulated event sample}

with STIC tagging conditions, demonstrating that they give similar results. A t to the QED prediction [15,28]

F₂ _{= x} ( x2_{+ (1},x)2 ln_m₂₊_PW₂_x(12 ,x) ,1 + 8x(1,x), P2_x(1 ,x) m2+P2_x(1,x) ) ; (14) where terms of orderm2=Q2 _{are neglected gives values of the eective average target}

pho-ton virtualityP2 _{of 0.022}0.007 and 0.0260.006 GeV2 for the rst and second methods respectively, the errors quoted being statistical. For the SAT tagged events the rst method, which was chosen for the further analysis, gives P2_=0.032

0.007 GeV

2_,

demon-strating the need to take the target photon virtuality into account in studies of F₂ _.

The extracted structure function < F₂ _(x;Q2₎ _{>, transformed to F}₂ _{(x;< Q}2 _>)

us-ing the ratio F₂ _{(x;< Q}2 _{>)= < F}₂ _(x;Q2₎ _{> predicted by QED, is shown in Table 2}

and Fig. 10, which present the weighted combination of the SAT and STIC results with < Q2 _{>= 12:5 GeV}2_=c4 _{and the FEMC result with} _{< Q}2 _{>= 120 GeV}2_=c4_{. The FEMC}

sample included only events withtag below 25 (above 155) in order to exclude the re-gion with large background contamination (Fig. 8b), and the contribution from diagrams other than the multiperipheral one predicted by the BDKRC generator was subtracted. The structure function values have been corrected to the centres of the x bins by multi-plying the measured average values ofF₂ _{for each}_{x bin by the ratio of the value of F}₂ _in

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errors due to the resolutions in Q and x have been evaluated in simulation by varying these variables according to their resolutions and checking the eect on F₂ _{. The role of}

the observed discrepancy between the data and simulation in sometag intervals (Fig. 3)

was checked by weighting the contributions of events in those intervals according to their tag values when producing thex distribution. The largest contribution to the systematic

error comes from theQ2 _resolution.

Fits to the QED prediction (14) give P2 _{= 0:025}0:005 and 0:0730:056 GeV2 for the samples with low and high Q2 _{respectively, in good agreement with the Monte Carlo}

prediction. x <0.1 0.1-0.2 0.2-0.3 0.3-0.4 0.4-0.5 0.5-0.6 0.6-0.7 0.7-0.8 >0.8 F₂ ₌ _{0.106 0.273 0.426 0.515 0.573 0.645 0.743 0.942 1.152} stat. error 0.008 0.012 0.017 0.021 0.024 0.029 0.038 0.060 0.112 syst. error 0.023 0.012 0.012 0.012 0.004 0.003 0.021 0.053 0.094 x <0.2 0.2-0.4 0.4-0.6 0.6-0.8 >0.8 F₂ ₌ _{0.387 0.464 0.673 0.984 1.508} stat. error 0.214 0.133 0.138 0.162 0.231 syst. error 0.015 0.051 0.049 0.026 0.044

Table 2: The measured structure function F₂ _for _{< Q}2 _{>= 12:5 (upper table) and}

120 GeV2_=c4 _{(lower table).}

7.2 Azimuthal correlations

In order to increase the observed azimuthal correlations of the nal state particles, only events with 20 < < 160 have been considered. Taking into account the anti-symmetry ofF

A in cos, events with cos <0 and cos >0 have been combined using the transformation !,.

The selected samples have been corrected for detector acceptance and eciency us-ing either bin-by-bin corrections over a two-dimensional grid of and , or a three-dimensional unfolding [29] in the space of the variables , and x. The corrected distributions (Fig. 11) were tted to the expression:

dN=d = C (1 + P1cos + P2cos2) (15)

where P1 and P2 are closely related to F_A =F2 and FB =F2 , c.f. Eq. (6). The combined

results were obtained by retting the weighted sums of corrected distributions for the SAT and STIC samples (Fig. 12). The parameters determined from the t are shown in Table 3.

The systematic eects were estimated using simulated events, varying the variables Q2_,_W_,_x, and according to their resolution, and adding the resulting variations of the tted parameters in quadrature. This gave errors on the tted parameters of about 0.02. The dierence between the results obtained with the two dierent correction meth-ods gave an additional systematic error of 0.02,0.06.

The results obtained were extrapolated to the full and W

ranges using the

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Q range of 2.4-51.2 GeV without and with the selection cuts. The results thus obtained for F

A=F2 and 12FB =F2 are shown in Table 3 and Fig. 13. They are in agreement with

the theoretical predictions [18] and with the results of other LEP experiments [13,14] (note the factor -1/2 dierence of F

A with [13] due to its dierent denition).

8 Conclusions

Muon pair production in single-tagged collisions has been studied atp

s'91 GeV using data collected by the DELPHI detector at LEP during the years 1992-95. Distri-butions of dierent event variables for Q2 _{ranging from} 2.5 to 750 GeV2=c4 are well reproduced by a Monte Carlo simulation based on QED.

The leptonic structure function F₂ _{has been measured for two regions of momentum}

transfer with average Q2 _{values of 12.5 and 120 GeV}2_=c4_.

Azimuthal correlations of nal state particles have also been studied, giving infor-mation on additional structure functions F_A _and _F_B _{. The measured ratios} _F_A _=F₂ _and

F

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Acknowledgements

We wish to thank V. Andreev and Ch. Carimalo for useful discussions.

We are greatly indebted to our technical collaborators, to the members of the CERN-SL Division for the excellent performance of the LEP collider, and to the funding agencies for their support in building and operating the DELPHI detector.

We acknowledge in particular the support of

Austrian Federal Ministry of Science and Tracs, GZ 616.364/2-III/2a/98, FNRS{FWO, Belgium,

FINEP, CNPq, CAPES, FUJB and FAPERJ, Brazil,

Czech Ministry of Industry and Trade, GA CR 202/96/0450 and GA AVCR A1010521, Danish Natural Research Council,

Commission of the European Communities (DG XII), Direction des Sciences de la Matiere, CEA, France,

Bundesministerium fur Bildung, Wissenschaft, Forschung und Technologie, Germany, General Secretariat for Research and Technology, Greece,

National Science Foundation (NWO) and Foundation for Research on Matter (FOM), The Netherlands,

Norwegian Research Council,

State Committee for Scientic Research, Poland, 2P03B06015, 2P03B1116 and SPUB/P03/178/98,

JNICT{Junta Nacional de Investigac~ao Cientca e Tecnologica, Portugal, Vedecka grantova agentura MS SR, Slovakia, Nr. 95/5195/134,

Ministry of Science and Technology of the Republic of Slovenia, CICYT, Spain, AEN96{1661 and AEN96-1681,

The Swedish Natural Science Research Council,

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References

[1] H.J. Behrend et al. (CELLO Collab.), Phys. Lett. B126 (1983) 384. [2] M.P. Cain et al. (TPC/2 Collab.), Phys. Lett. B147(1984) 232. [3] Ch. Berger et al. (PLUTO Collab.), Z. Phys.C27 (1985) 249. [4] W. Bartel et al. (JADE Collab.), Z. Phys. C30 (1986) 545. [5] B. Adeva et al. (MARK J coolab.), Phys. Rev. D38(1988) 2665. [6] H.J. Behrend et al. (CELLO Collab.), Z. Phys.C43 (1989) 1.

[7] M. Petradza et al. (MARK II Collab.), Phys. Rev.D42 (1990) 2171. [8] M. Petradza et al. (HRS Collab.), Phys. Rev. D42 (1990) 2180. [9] Y.H. Ho et al. (AMY Collab.), Phys. Lett.B244 (1990) 573. [10] R. Akers et al. (OPAL Collab.), Z. Phys. C60(1993) 593. [11] R. Abreu et al. (DELPHI Collab.), Z. Phys. C69(1996) 223. [12] K. Ackersta et al. (OPAL Collab.), Z. Phys. C74(1997) 49. [13] M. Acciarri et al. (L3 Collab.), Phys. Lett.B438 (1998) 363. [14] G. Abbiendi et al. (OPAL Collab.), Eur. Phys. J. C11 (1999) 409. [15] V.M. Budnev et al., Phys. Rep. 15 (1974) 181.

[16] P. Aurenche et al., `Physics at LEP2', eds. G. Altarelli, T. Sjostrand and F. Zwirner, CERN 96-01 (1996) Vol.1 p.291.

[17] C. Peterson, P.M. Zerwas and T.F. Walsh, Nucl. Phys. B229(1983) 301. [18] S. Ong and P. Kessler, Mod. Phys. Lett.A2 (1987) 683.

Note that in the expression for the helicity terms I++;++ +I++;,, a factor

2 _is

missing in front of (1,u

2_{) and in the expression for} _I_++;00 _{there should be the rst}

degree power in the denominator.

[19] P. Aarnio et al. (DELPHI Collab.), Nucl. Inst. Meth. A303 (1991) 233. [20] P. Abreu et al. (DELPHI Collab.), Nucl. Inst. Meth.A378 (1996) 57.

[21] F.A. Berends, P.H. Daverveldt, R. Kleiss, Comp. Phys. Comm.40 (1986) 271. [22] F.A. Berends, P.H. Daverveldt, R. Kleiss, Comp. Phys. Comm.40 (1986) 285. [23] S. Nova, A. Olshevski and T. Todorov, `Physics at LEP2', CERN 96-01 (1996) Vol.2

p.224; updated version described in `Reports of the Working Groups on Precision Calculations for LEP2 Physics', CERN 2000-009 (2000) 243.

[24] J.E. Campagne and R. Zitoun, Z. Phys.C43 (1989) 469. [25] S. Jadach et al., Comp. Phys. Comm.79 (1994) 503.

[26] Ch. Berger et al. (PLUTO Collab.), Phys. Lett. B137(1984) 267. [27] P. Abreu et al. (DELPHI Collab.), Phys. Lett. B342 (1995) 402. [28] C. Berger and W. Wagner, Phys. Rep. 146 (1987) 1.

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x-interval P1 CP

SAT STIC Combined

x < 0:2 0:190:140:03 0:280:080:04 0.250.08 0.541 0:2 < x < 0:4 0:220:090:03 0:200:060:02 0.200.05 0.701 0:4 < x < 0:6 0:130:090:05 0:020:070:05 0.060.07 0.625 x > 0:6 -0:410:100:07 -0:260:070:05 -0.310.07 0.849 allx -0:030:050:03 -0:030:030:03 -0.030.04 0.605 x-interval P2 CP2

SAT STIC Combined

x < 0:2 0:060:120:03 -0:010:080:03 0.010.07 0.391 0:2 < x < 0:4 0:130:080:03 0:160:060:02 0.150.05 0.512 0:4 < x < 0:6 0:150:080:04 0:190:060:03 0.170.06 0.581 x > 0:6 0:200:090:06 0:300:060:04 0.270.06 0.673 all x 0:130:050:02 0:150:030:02 0.150.03 0.570 x-interval F A=F2 1₂FB =F2 x < 0:2 0:1350:043 0:0040:027 0:2 < x < 0:4 0:1400:035 0:0770:026 0:4 < x < 0:6 0:0380:044 0:0990:035 x > 0:6 -0:2630:059 0:1820:040 all x -0:0180:024 0:0860:017

Table 3: Parameters P1 and P2 of the t to the azimuthal angle distributions for the

SAT-tagged, STIC-tagged, and combined event samples withQ2 _{= 2:4},51:2 GeV2. The rst error is statistical and the second is systematic. CP1 andCP2 are the correction factors to extrapolate the parameters to the full range (see text). The values extracted for F_A _=F₂ _and 1

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µ+ µ -E_tag, θ_tag γ (p) γ* (q) θ* µ+ µ -γ γ* e-tag χ

Figure 1: The dominant multiperiph-eral diagram for the reaction e+_e,

! e+_e,+,. E

tag and tag are the energy

and scattering angle of the tagged electron or positron.

Figure 2: Denitions of the angles and in the centre-of-mass sys-tem. DELPHI 0 200 400 600 800 1000 1200 1400 1600 1800 10 12.5 15 17.5 20 22.5 25 27.5 30 32.5 35 Radius, cm Events / 0.2 cm 0 100 200 300 400 500 600 700 800 900 10 12.5 15 17.5 20 22.5 25 27.5 30 32.5 35 Radius, cm Events / 0.2 cm

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DELPHI 2000 2200 2400 2600 2800 3000 3200 0 50 100 150 200 250 300 350 φ1, deg Events / 45 deg -0.04 -0.02 0 0.02 0.04 0 50 100 150 200 250 300 350 φ2, deg θ1 - θ2 , deg

Figure 4: Left - number of detected Bhabha events as a function of the azimuthal angle for the SAT module with the mask. Right - dierence of the polar angles of Bhabha electrons measured by the SAT modules as a function of the azimuthal angle. The lines show the results of the ts.

DELPHI -25 -20 -15 -10 -5 0 5 10 15 5 10 15 20 25 30 θtag, deg Etag -E tag gen

, GeV SAT FEMC

-25 -20 -15 -10 -5 0 5 10 15 5 10 15 20 25 30 θtag, deg Etag -E tag gen

, GeV SAT FEMC

Figure 5: Dierence of reconstructed and true (generated) tag energyEtag versus the tag

angle tag in simulated events: left - measured value of Etag, right - Etag value calculated

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DELPHI 0 20 40 60 80 100 120 140 0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1 1.05 Etag / Ebeam Events / 0.01 a) 0 20 40 60 80 100 120 140 160 2 3 4 5 6 7 8 9 10 θtag , deg Events / 0.2 deg b) 0 50 100 150 200 250 0 10 20 30 40 50 Q 2, GeV 2/c 4 Events / 1.5 GeV 2 /c 4 c) 1 10 102 2.5 5 7.5 10 12.5 15 17.5 20 22.5 25 W, GeV/c 2 Events / 0.6 GeV/c 2 d) 1 10 102 0 2 4 6 8 10 12 14 16 18 20 P_t µ_{, GeV/c} Events / 0.5 GeV/c e) 0 20 40 60 80 100 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x Events / 0.04 f)

Figure 6: Distributions for the SAT single tagged events: a)Etag=Ebeam, b)tag(180

,tag

for positrons), c) squared momentum transferQ2_{, d) invariant mass of muon pair, e) sum}

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DELPHI 0 50 100 150 200 250 300 0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1 1.05 E_tag / E_beam Events / 0.01 a) 0 50 100 150 200 250 300 2 3 4 5 6 7 8 9 10 θtag , deg Events / 0.2 deg b) 0 100 200 300 400 500 0 10 20 30 40 50 Q 2, GeV 2/c 4 Events / 1.5 GeV 2 /c 4 c) 1 10 102 2.5 5 7.5 10 12.5 15 17.5 20 22.5 25 W, GeV/c 2 Events / 0.6 GeV/c 2 d) 1 10 102 0 2 4 6 8 10 12 14 16 18 20 P_t µ_{, GeV/c} Events / 0.5 GeV/c e) 0 25 50 75 100 125 150 175 200 225 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x Events / 0.04 f)

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DELPHI 0 10 20 30 40 50 60 0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.95 1 1.05 1.1 E_tag / E_beam Events / 0.05 a) 0 20 40 60 80 100 5 10 15 20 25 30 35 θtag , deg Events / 2 deg b) 0 20 40 60 80 100 0 100 200 300 400 500 600 700 Q 2, GeV 2/c 4

Events / var. bin

c) 0 10 20 30 40 50 60 70 80 90 5 10 15 20 25 W, GeV/c 2 Events / 3 GeV/c 2 d) 0 20 40 60 80 100 120 0 2.5 5 7.5 10 12.5 15 17.5 20 22.5 25 P_t µ_{, GeV/c} Events / 2.5 GeV/c e) 0 10 20 30 40 50 60 70 80 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x Events / 0.125 f)

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DELPHI 0 0.2 0.4 0.6 0.8 1 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x F2 γ (x) / α

Figure 9: F₂ _{(x) for < Q}2 _{>= 12:5 GeV}2_=c4 _{extracted from a simulated STIC tagged}

event sample (points) and the t to the QED expression (lines): full circles and solid lines are for the extraction using the simulation with known F2, open circles and dashed

lines for the extraction using the photon ux approach.

DELPHI 0 0.5 1 1.5 0 0.2 0.4 0.6 0.8 1 x F2 γ (x) / α <Q2>=12.5 GeV2 <Q2>=120 GeV2 <P2>=0.026 GeV2

Figure 10: F₂ _{(x) extracted from the combined SAT and STIC data (< Q}2 _{>= 12:5}

GeV2_=c4_{, full circles), and from the FEMC data (< Q}2 _{>= 120 GeV}2_=c4_{, open circles).}

Statistical and systematic errors are added in quadrature. The solid and dashed lines show the QED predictions withP2_{=0.026 GeV}2_=c4 _{for the low}_Q2 _{and high} _Q2 _samples,

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DELPHI 0 0.5 1 1.5 2 2.5 3 0 20 40 60 80 100 120 140 160 180 χ, deg

Rel. number of events / 22.5 deg

x<0.2 a) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 0 20 40 60 80 100 120 140 160 180 χ, deg

0.2<x<0.4 b) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 0 20 40 60 80 100 120 140 160 180 χ, deg

0.4<x<0.6 c) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 0 20 40 60 80 100 120 140 160 180 χ, deg

x>0.6 d) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 0 20 40 60 80 100 120 140 160 180 χ, deg

all x e)

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DELPHI 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 0 20 40 60 80 100 120 140 160 180 χ, deg

x<0.2 a) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 0 20 40 60 80 100 120 140 160 180 χ, deg

0.2<x<0.4 b) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 0 20 40 60 80 100 120 140 160 180 χ, deg

0.4<x<0.6 c) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 0 20 40 60 80 100 120 140 160 180 χ, deg

x>0.6 d) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 0 20 40 60 80 100 120 140 160 180 χ, deg

all x e)

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DELPHI -0.2 0 0.2 0 0.2 0.4 0.6 0.8 1 x FA γ / F 2 γ Q2=2.4-51.2 GeV2 0 0.1 0.2 0 0.2 0.4 0.6 0.8 1 x 1/2 F B γ / F 2 γ Q2=2.4-51.2 GeV2

Figure 13: Ratios of leptonic structure functions F_A _=F₂ _{(left) and} 1

2FB =F2 (right)

aver-aged in the Q2 _{range from 2.4 to 51.2 GeV}2 _{as functions of} _{x. The lines show the QED}