PDF hosted at the Radboud Repository of the Radboud University Nijmegen The version of the following full text has not yet been defined or was untraceable and may differ from the publisher's version. For additional information about this publication click this link. http://hdl.handle.net/2066/35427 Please be advised that this information was generated on 2015-02-06 and may be subject to change. F erm ilab-P ub-06/081-E arXiv:hep-ex/0604040v1 19 Apr 2006 S earch for E x c ite d M u o n s in p p C ollisions a t y /s = 1.96 TeV V.M . A bazov,36 B. A b b o tt,76 M. A bolins,66 B.S. A charya,29 M. A dam s,52 T. A dam s,50 M. A gelou,18 J.-L. A g ram ,19 S.H. A hn,31 M. A h san ,60 G.D. Alexeev,36 G. A lkhazov,40 A. A lton,65 G. A lverson,64 G.A. Alves,2 M. A nastasoaie,35 T. A ndeen,54 S. A nderson,46 B. A n d rieu ,17 M.S. Anzelc,54 Y. A rn o u d ,14 M. A rov,53 A. Askew,50 B. Â sm an,41 A.C.S. Assis Jesu s,3 O. A tram en to v ,58 C. A u te rm a n n ,21 C. A vila,8 C. Ay,24 F. B a d a u d ,13 A. B ad en ,62 L. Bagby,53 B. B ald in ,51 D.V. B a n d u rin ,36 P. B anerjee,29 S. B anerjee,29 E. B arb eris,64 P. B argassa,81 P. B aringer,59 C. B arnes,44 J. B a rre to ,2 J.F . B a rtle tt,51 U. B assler,17 D. B auer,44 A. B ean,59 M. Begalli,3 M. Begel,72 C. B elanger-C ham pagne,5 A. Bellavance,68 J.A . B en itez,66 S.B. B eri,27 G. B e rn a rd i,17 R. B ern h ard ,42 L. B ern tzo n ,15 I. B e rtra m ,43 M. B esan co n ,18 R. B euselinck,44 V.A. B ezzubov,39 P.C. B h a t,51 V. B h a tn a g a r,27 M. B inder,25 C. B isc ara t,43 K.M . B lack,63 I. B lackler,44 G. Blazey,53 F . B lekm an,44 S. B lessing,50 D. B loch,19 K. B loom ,68 U. B lum enschein,23 A. B oehnlein,51 O. B oeriu,56 T .A . B o lto n ,60 F . B orcherding,51 G. B orissov,43 K. Bos,34 T. B ose,78 A. B ra n d t,79 R. B rock,66 G. B rooijm ans,71 A. B ross,51 D. B row n,79 N .J. B u chanan,50 D. Buchholz,54 M. B uehler,82 V. B uescher,23 S. B u rd in ,51 S. B urke,46 T.H . B u rn e tt,83 E. B u sa to ,17 C.P. Buszello,44 J.M . B u tle r,63 S. C alv e t,15 J. C am m in,72 S. C aro n ,34 W . C arvalho,3 B .C .K . Casey,78 N.M. C ason,56 H. C astilla-V aldez,33 S. C h a k ra b a rti,29 D. C h ak rab o rty ,53 K .M . C h a n ,72 A. C h a n d ra ,49 D. C h ap in ,78 F. C h arles,19 E. C heu,46 F . C hevallier,14 D.K. C ho,63 S. C hoi,32 B. C h o u d h ary ,28 L. C hristofek,59 D. C laes,68 B. C lem en t,19 C. C lem ent,41 Y. C oadou,5 J. C oenen,21 M. C ooke,81 W .E . C ooper,51 D. C oppage,59 M. C orcoran,81 M .-C. C ousinou,15 B. Cox,45 S. C rep e-R en au d in ,14 D. C u tts ,78 M. Cw iok,30 H. d a M o tta ,2 A. D as,63 M. D as,61 B. D avies,43 G. D avies,44 G .A. D avis,54 K. D e,79 P. de Jo n g ,34 S.J. de Jo n g ,35 E. De L a C ruz-B urelo,65 C. De O liveira M artin s,3 J.D . D eg en h ard t,65 F. D eliot,18 M. D em arteau ,51 R. D em ina,72 P. D em ine,18 D. D enisov,51 S.P. D enisov,39 S. D esai,73 H .T . D iehl,51 M. D iesburg,51 M. D oidge,43 A. D om inguez,68 H. D ong,73 L.V. D udko,38 L. D uflot,16 S.R. D ugad,29 A. D u p e rrin ,15 J. D yer,66 A. D yshkant,53 M. E a d s,68 D. E d m u n d s,66 T. E dw ards,45 J. E llison,49 J. E lm sheuser,25 V.D. E lv ira,51 S. E n o ,62 P. E rm olov,38 J. E s tra d a ,51 H. E vans,55 A. E vdokim ov,37 V.N. E vdokim ov,39 S.N. F a ta k ia ,63 L. Feligioni,63 A.V. F erap o n to v ,60 T. F erbel,72 F. F ied ler,25 F. F ilth a u t,35 W . F isher,51 H .E. F isk,51 I. Fleck,23 M. F ord,45 M. F o rtn e r,53 H. Fox,23 S. F u,51 S. Fuess,51 T. G ad fo rt,83 C .F. G alea,35 E. G allas,51 E. G alyaev,56 C. G arcia,72 A. G arcia-B ellido,83 J. G ard n er,59 V. G avrilov,37 A. G ay,19 P. G ay,13 D. G ele,19 R. G elhaus,49 C .E. G erb er,52 Y. G ershtein,50 D. G illberg,5 G. G in th e r,72 N. G ollub,41 B. G om ez,8 K. G ounder,51 A. G oussiou,56 P.D. G ran n is,73 H. G reenlee,51 Z.D. G reenw ood,61 E.M . G regores,4 G. G renier,20 P h. G ris,13 J.-F . G rivaz,16 S. G rän e n d a h l,51 M .W . G rünew ald,30 F. G uo,73 J. G uo,73 G. G u tierrez,51 P. G u tierrez,76 A. H aas,71 N .J. H adley,62 P. H aefner,25 S. H agopian,50 J. H aley,69 I. H all,76 R .E. H all,48 L. H an ,7 K. H anagaki,51 K. H a rd e r,60 A. H arel,72 R. H a rrin g to n ,64 J.M . H a u p tm a n ,58 R. H auser,66 J. H ays,54 T. H ebbeker,21 D. H edin,53 J.G . H egem an,34 J.M . H einm iller,52 A.P. H einson,49 U. H eintz,63 C. H ensel,59 G. H esketh,64 M.D. H ild reth ,56 R. H irosky,82 J.D . H obbs,73 B. H oeneisen,12 M. H ohlfeld,16 S.J. H ong,31 R. H ooper,78 P. H ouben,34 Y. H u ,73 V. H ynek,9 I. Iashvili,70 R. Illingw orth,51 A.S. Ito ,51 S. Ja b e e n ,63 M. Jaffre,16 S. Ja in ,76 K. Jak o b s,23 C. Ja rv is,62 A. Jen k in s,44 R. Jesik,44 K. Jo h n s,46 C. Jo h n so n ,71 M. Johnson,51 A. Jonckheere,51 P. Jonsson,44 A. Ju ste ,51 D. K üfer,21 S. K a h n ,74 E. K a jfasz,15 A.M . K alinin,36 J.M . K alk ,61 J.R . K alk ,66 S. K ap p le r,21 D. K arm anov,38 J. K a sp er,63 I. K a tsa n o s,71 D. K a u ,50 R. K a u r,27 R. K ehoe,80 S. K erm iche,15 S. K esisoglou,78 A. K hanov,77 A. K harchilava,70 Y.M . K h arzheev,36 D. K h atid ze,71 H. K im ,79 T .J. K im ,31 M.H. K irby,35 B. K lim a,51 J.M . K ohli,27 J.-P. K o n ra th ,23 M. K o p al,76 V.M . K orablev,39 J. K o tch er,74 B. K o th a ri,71 A. K oubarovsky,38 A.V. K ozelov,39 J. K ozm inski,66 A. K ry em ad h i,82 S. K rzyw dzinski,51 T. K u h l,24 A. K u m a r,70 S. K u n o ri,62 A. K u p c o ,11 T. K u rca ,20’* J. K v ita ,9 S. L ager,41 S. L am m ers,71 G. L an d sb erg ,78 J. Lazoflores,50 A.-C. Le B ih a n ,19 P. L ebrun,20 W .M . Lee,53 A. Leflat,38 F. L ehner,42 C. L eonidopoulos,71 V. L esne,13 J. Leveque,46 P. Lewis,44 J. L i,79 Q.Z. Li,51 J.G .R . L im a,53 D. L incoln,51 J. L in n em an n ,66 V.V. L ipaev,39 R. L ip to n ,51 Z. L iu,5 L. Lobo,44 A. L obodenko,40 M. L okajicek,11 A. L ounis,19 P. Love,43 H .J. L u b a tti,83 M. L ynker,56 A.L. Lyon,51 A.K.A. M aciel,2 R .J. M ad aras,47 P. M üttig ,26 C. M agass,21 A. M ag erk u rth ,65 A.-M . M ag n an ,14 N. M akovec,16 P.K. M al,56 H.B. M albouisson,3 S. M alik,68 V.L. M alyshev,36 H.S. M ao,6 Y. M arav in ,60 M. M arten s,51 S.E.K . M attingly,78 R. M cC arthy,73 R. M cCroskey,46 D. M eder,24 A. M elnitchouk,67 A. M endes,15 L. M endoza,8 M. M erkin,38 K .W . M e rritt,51 A. M eyer,21 J. M eyer,22 M. M ich au t,18 H. M iettin en ,81 T. M illet,20 J. M itrevski,71 J. M olina,3 N.K. M ondal,29 J. M onk,45 R.W . M oore,5 T. M oulik,59 G.S. M u an za,16 M. M ulders,51 M. M ulhearn,71 L. M undim ,3 Y.D. M u taf,73 E. N agy,15 M. N aim uddin,28 M. N arain ,63 N.A. N aum ann,35 H.A. N eal,65 J.P . N egret,8 S. N elson,50 P. N eustroev,40 C. N oeding,23 A. N om erotski,51 S.F. Novaes,4 T. N u nnem ann,25 V. O ’Dell,51 D.C. O ’Neil,5 G. O b ra n t,40 2 V. O guri,3 N. O liveira,3 N. O shim a,51 R. O te c ,10 G .J. O tero y G arzon,52 M. O wen,45 P. Padley,81 N. P a ra sh a r,57 S.-J. P a rk ,72 S.K. P a rk ,31 J. P arso n s,71 R. P a rtrid g e ,78 N. P a ru a ,73 A. P a tw a ,74 G. Paw loski,81 P.M . P erea,49 E. P erez,18 K. P eters,45 P. P etro ff,16 M. P e tte n i,44 R. P ieg a ia,1 M.-A. P leier,22 P.L.M . P o d esta-L erm a,33 V.M . P o dstavkov,51 Y. Pogorelov,56 M .-E. P ol,2 A. P om pos,76 B .G . P o p e,66 A.V. P opov,39 W .L. P ra d o d a Silva,3 H.B. P ro sp e r,50 S. P ro to p o p escu ,74 J. Q ian ,65 A. Q u a d t,22 B. Q u in n ,67 K .J. R an i,29 K. R a n jan ,28 P.A. R apidis,51 P.N. R atoff,43 P. R enkel,80 S. R eucroft,64 M. R ijssenbeek,73 I. R ip p -B au d o t,19 F . R izatdinova,77 S. R obinson,44 R .F. R odrigues,3 C. R oyon,18 P. R ubinov,51 R. R uchti,56 V.I. R ud,38 G. S a jo t,14 A. Sânchez-H ernandez,33 M .P. S anders,62 A. S antoro,3 G. Savage,51 L. Saw yer,61 T. Scanlon,44 D. Schaile,25 R.D . Scham berger,73 Y. Scheglov,40 H. Schellm an,54 P. Schieferdecker,25 C. S ch m itt,26 C. Schw anenberger,45 A. Schw artzm an,69 R. Schw ienhorst,66 S. S en g u p ta,50 H. Severini,76 E. S habalina,52 M. Sham im ,60 V. S hary,18 A.A. Shchukin,39 W .D . S h ep h ard ,56 R .K . S hivpuri,28 D. Shpakov,64 V. S iccardi,19 R.A. Sidwell,60 V. S im ak,10 V. Sirotenko,51 P. Skubic,76 P. S lattery ,72 R.P. S m ith,51 G .R . Snow,68 J. Snow,75 S. Snyder,74 S. Soldner-R em bold,45 X. Song,53 L. S onnenschein,17 A. Sopczak,43 M. Sosebee,79 K. S oustruznik,9 M. Souza,2 B. Spurlock,79 J. S ta rk ,14 J. Steele,61 K. Stevenson,55 V. S tolin,37 A. S tone,52 D.A. Stoyanova,39 J. S tra n d b e rg ,41 M.A. S tran g ,70 M. S trau ss,76 R. S tro h m er,25 D. S tro m ,54 M. Strovink,47 L. S tu tte ,51 S. Sum ow idagdo,50 A. S znajder,3 M. T alby,15 P. T am burello,46 W . T aylor,5 P. T elford,45 J. Tem ple,46 B. T ille r,25 M. T ito v ,23 V.V. Tokm enin,36 M. T om oto,51 T. Toole,62 I. T orchiani,23 S. Towers,43 T. Trefzger,24 S. T rincaz-D uvoid,17 D. T sybychev,73 B. T uchm ing,18 C. Tully,69 A.S. T u rco t,45 P.M . T u ts,71 R. U n alan ,66 L. U varov,40 S. U varov,40 S. U zunyan,53 B. V achon,5 P .J. van den B erg,34 R. V an K o o ten ,55 W .M . van Leeuwen,34 N. V arelas,52 E.W . V arnes,46 A. V a rta p e tia n ,79 I.A. Vasilyev,39 M. V aupel,26 P. V erdier,20 L.S. V ertogradov,36 M. Verzocchi,51 F. V illeneuve-Seguier,44 P. V in t,44 J.-R . V lim a n t,17 E. Von T oerne,60 M. V outilainen,68’^ M. Vreeswijk,34 H.D. W ahl,50 L. W ang,62 J. W archol,56 G. W a tts,83 M. W ayne,56 M. W eber,51 H. W eerts,66 N. W erm es,22 M. W etstein,62 A. W h ite,79 D. W icke,26 G .W . W ilson,59 S.J. W im penny,49 M. W obisch,51 J. W omersley,51 D.R. W ood,64 T .R . W y a tt,45 Y. X ie,78 N. X u an ,56 S. Y acoob,54 R. Y am ada,51 M. Y an,62 T. Y asuda,51 Y.A. Y atsunenko,36 K. Y ip,74 H.D. Yoo,78 S.W . Y oun,54 C. Y u,14 J. Y u,79 A. Y urkewicz,73 A. Zatserklyaniy,53 C. Z eitnitz,26 D. Z hang,51 T. Z hao,83 Z. Z hao,65 B. Z hou,65 J. Z hu,73 M. Zielinski,72 D. Ziem inska,55 A. Ziem inski,55 V. Z utshi,53 and E .G . Zverev38 (D 0 C ollaboration) 1 Universidad de Buenos Aires, Buenos Aires, Argentina 2LAFEX, Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Brazil 3 Universidade do Estado do Rio de Janeiro, Rio de Janeiro, Brazil 4Instituto de Fisica Teorica, Universidade Estadual Paulista, Sao Paulo, Brazil 5 University of Alberta, Edmonton, Alberta, Canada,, Simon Fraser University, Burnaby, British Columbia, Canada,, York University, Toronto, Ontario, Canada, and McGill University, Montreal, Quebec, Canada 6Institute of High Energy Physics, Beijing, People’s Republic of China 7 University of Science and Technology of China, Hefei, People ’s Republic of China 8 Universidad de los Andes, Bogota, Colombia, 9 Center fo r Particle Physics, Charles University, Prague, Czech Republic 10 Czech Technical University, Prague, Czech Republic 11 Center for Particle Physics, Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic 12 Universidad San Francisco de Quito, Quito, Ecuador 13Laboratoire de Physique Corpusculaire, IN2P3-CNRS, Université Blaise Pascal, Clermont-Ferrand, France 14Laboratoire de Physique Subatomique et de Cosmologie, IN2P3-CNRS, Universite de Grenoble 1, Grenoble, France 15 CPPM, IN2P3-CNRS, Université de la Méditerranée, Marseille, France 16IN2P3-CNRS, Laboratoire de l ’Accélérateur Linéaire, Orsay, France 17LPNHE, IN2P3-CNRS, Universités Paris VI and VII, Paris, France 18DAPNIA/Service de Physique des Particules, CEA, Saclay, France 19IReS, IN2P3-CNRS, Université Louis Pasteur, Strasbourg, France, and Université de Ha,ute Alsace, Mulhouse, France 20Institut de Physique Nucléaire de Lyon, IN2P3-CNRS, Université Claude Bernard, Villeurbanne, France 21III. Physikalisches Institut A, R W TH Aachen, Aachen, Germany 22Physikalisches Institut, Universitat Bonn, Bonn, Germany 23Physikalisches Institut, Universität Freiburg, Freiburg, Germany 24Institut fü r Physik, Universitat Mainz, Mainz, Germany 25Ludwig-Maximilians-Universitat München, München, Germany 26Fachbereich Physik, University of Wuppertal, Wuppertal, Germany 27 Pa,nja,b University, Chandigarh, India, 28Delhi University, Delhi, India, 29 Tata Institute of Fundamental Research, Mumbai, India, 30 University College Dublin, Dublin, Ireland 31Korea Detector Laboratory, Korea University, Seoul, Korea, 3 32 SungKyunKwan University, Suwon, Korea 33 CINVESTAV, Mexico City, Mexico 34FOM-Institute NIKH EF and University of Amsterdam/NIKHEF, Amsterdam, The Netherlands 35 Radboud University Nijmegen/NIKHEF, Nijmegen, The Netherlands 36 Joint Institute fo r Nuclear Research, Dubna, Russia, 37Institute fo r Theoretical and Experimental Physics, Moscow, Russia 38 Moscow State University, Moscow, Russia, 39Institute fo r High Energy Physics, Protvino, Russia 40 Petersburg Nuclear Physics Institute, St. Petersburg, Russia 41Lund University, Lund, Sweden, Royal Institute of Technology and Stockholm University, Stockholm, Sweden, and Uppsala University, Uppsala, Sweden 42 Physik Institut der Universität Zurich, Zurich, Switzerland, 43Lancaster University, Lancaster, United Kingdom 44Imperial College, London, United Kingdom 45 University of Manchester, Manchester, United Kingdom 46 University of Arizona, Tucson, Arizona 85721, USA 47Lawrence Berkeley National Laboratory and University of California, Berkeley, California 94720, USA 48 California State University, Fresno, California 93740, USA 49 University of California, Riverside, California 92521, USA 50Florida State University, Tallahassee, Florida 32306, USA 51Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA 52 University of Illinois at Chicago, Chicago, Illinois 60607, USA 53Northern Illinois University, DeKalb, Illinois 60115, USA 54Northwestern University, Evanston, Illinois 60208, USA 55Indiana University, Bloomington, Indiana 47405, USA 56 University of Notre Dame, Notre Dame, Indiana 46556, USA 57Purdue University Calumet, Hammond, Indiana 46323, USA 58Iowa State University, Ames, Iowa 50011, USA 59 University of Kansas, Lawrence, Kansas 66045, USA 60Kansas State University, Manhattan, Kansas 66506, USA 61Louisiana Tech University, Ruston, Louisiana 71272, USA 62 University of Maryland, College Park, Maryland 20742, USA 63Boston University, Boston, Massachusetts 02215, USA 64Northeastern University, Boston, Massachusetts 02115, USA 65 University of Michigan, A nn Arbor, Michigan 48109, USA 66Michigan State University, East Lansing, Michigan 48824, USA 67 University of Mississippi, University, Mississippi 38677, USA 68 University of Nebraska, Lincoln, Nebraska 68588, USA 69 Princeton University, Princeton, New Jersey 08544, USA 70State University of New York, Buffalo, New York 14260, USA 71 Columbia University, New York, New York 10027, USA 72 University of Rochester, Rochester, New York 14627, USA 73State University of New York, Stony Brook, New York 11794, USA 74 Brookhaven National Laboratory, Upton, New York 11973, USA 75Langston University, Langston, Oklahoma 73050, USA 76 University of Oklahoma, Norman, Oklahoma 73019, USA 77 Oklahoma State University, Stillwater, Oklahoma 74078, USA 78 Brown University, Providence, Rhode Island 02912, USA 79 University of Texas, Arlington, Texas 76019, USA 80Southern Methodist University, Dallas, Texas 75275, USA 81 Rice University, Houston, Texas 77005, USA 82 University of Virginia, Charlottesville, Virginia 22901, USA 83 University of Washington, Seattle, Washington 98195, USA (Dated: April 19, 2006) We present the results of a search for the production of an excited state of the muon, ß *, in proton antiproton collisions at *Js = 1.96 TeV. The data have been collected with the DO experiment at the Fermilab Tevatron Collider and correspond to an integrated luminosity of approximately 380 pb- 1 . We search for ß* in the process pp ^ ß*ß, with the ß* subsequently decaying to a muon plus photon. No excess above the standard model expectation is observed in data. Interpreting our data in the context of a model th a t describes ß* production by four-fermion contact interactions and ß* decay via electroweak processes, we exclude production cross sections higher than 0.057 pb 0.112 pb at the 95% confidence level, depending on the mass of the excited muon. Choosing the 4 scale for contact interactions to be A = 1 TeV, excited muon masses below 618 GeV are excluded. PACS numbers: 12.60.Rc, 14.60.Hi, 12.60.-i, 13.85.Rm A n open question in p article physics is th e observed m ass h ierarchy of th e q u a rk an d lepton SU(2) doublets in th e sta n d a rd m odel (SM). A com m only proposed ex p lan atio n for th e th ree generations is a com positeness m odel [1] of th e know n leptons an d quarks. A ccording to th is approach, a q u ark or lep to n is a b o u n d sta te of th ree ferm ions, or of a ferm ion an d a boson [2]. Due to th e underlying su b stru c tu re , com positeness m odels im ply a large sp ectru m of excited states. T h e coupling of excited ferm ions to o rd in ary q u ark s an d leptons, resu lt ing from novel stro n g interactions, can be described by co n tact in teractio n s (CI) w ith th e effective four-ferm ion L agrangian [3] £cl = reach has been lim ited by th e center-of-m ass energy avail able to m M* < 190 GeV. Searches for quark-lepton com positeness via deviations from th e Drell-Yan cross section have excluded values of A of up to « 6 TeV depending on th e chirality [5]. T he present analysis is com plem entary to those results in th e sense th a t an exclusive channel and different couplings (n factors) are probed. T he CD F collaboration has recently presented results [6 ] for the pro d u ctio n of excited electrons which will be discussed later. 2 X 5 ^ ^ ’ w here j M is th e ferm ion cu rren t = nt f L L + n l f l Ymf L + n l /L Ym/l + h.c. + (L ——R). T h e SM an d excited ferm ions are den o ted by f and f *, respectively; g 2 is chosen to be 4n, th e n factors for the left-handed cu rren ts are conventionally set to one, and th e rig h t-h an d ed cu rren ts are set to zero. T h e com pos iteness scale is A. G auge m ed iated tra n sitio n s betw een o rd in a ry and ex cited ferm ions can be described by th e effective Lagran g ian [3] C EW \a f t + h.c. where G M a V, WMV, an d B mv are th e field stre n g th tensors of th e gluon, th e SU(2) an d U(1) gauge fields, respectively; f s, f an d f ' are p a ra m e te rs of o rd er one. T h e p resent analysis considers single p ro d u ctio n of an excited m uon u * in association w ith a m uon via fourferm ion CI, w ith th e subsequent electrow eak decay of th e u* in to a m uon an d a p h o to n (Fig. 1). T his de cay m ode leads to th e fully reco n stru ctab le and alm ost background-free final s ta te UUY. W ith th e d a ta consid ered herein, collected w ith th e D0 d etecto r a t th e Ferm ilab T evatron C ollider in pp collisions a t a/s = 1.96 TeV, th e largest expected SM background is from th e DrellYan (DY) process pp — Z / y * — u+ U - (y), w ith th e final sta te p h o to n ra d ia te d by eith er a p a rto n in th e initial sta te p or p, or from one of th e final s ta te m uons. T his background can be stro n g ly suppressed by th e applica tio n of suitable selection criteria. O th er backgrounds are small. E xcited m uons have been searched for unsuccessfully previously [4], e.g. a t th e L E P e + e - collider; however the FIG. 1: Four-fermion contact interaction qq ^ ß*ß, and electroweak decay ß* ^ ßY. On the right, the relative contribu tion of decays via CI and via electroweak interactions (EW) as a function of m M*/A is shown. For th e sim ulation of th e signal a custom ized ver sion of th e PYTHIA event generator [7] is used, following th e m odel of [3]. T he branching fraction for th e decay U* — UY norm alized to all gauge particle decay m odes is 30% for m asses above 300 GeV, and for sm aller u* m asses it increases up to 73% a t m M* = 100 GeV. Decays via con ta c t interactions, n o t im plem ented in PYTHIA, co n tribute betw een a few percent of all decays for A ^ m M* and 92% for A = m M* [3, 8 ] (see Fig. 1). T his has been tak en into account for th e signal expectation. T he leading or der cross section calculated w ith PYTHIA has been cor rected to n ex t-to-next-to-leading order (NNLO) [9, 10]; th e corresponding correction factor varies betw een 1.430 (1.468) for m M* = 100 GeV (200 GeV) and 1.312 for m M* = 1 TeV. T he to ta l w idth is greater th a n 1 GeV for 100 G eV < m M* < 1000 GeV, th u s lifetim e effects can be neglected. For th e values of m M* and A studied here, the to ta l w idth is always less th a n 10% of m M* [3]. T he dom inant SM background process a t all stages of th e selection is DY p ro d u ctio n of u+ U - pairs. T his back ground, as well as diboson ( W W , W Z , Z Z ) production, has been sim ulated w ith th e PY TH IA M onte C arlo (MC) program . T he DY ex p ectatio n has been corrected us ing th e NNLO calculation from [9]. For diboson produc tion, th e next-to-leading order cross sections from [11 ] are used. M onte C arlo events, b o th for SM and signal, have been passed th ro u g h a detecto r sim ulation based on th e G EA N T [12] package, and reco n stru cted using the sam e reco n stru ctio n p rogram as th e d a ta . T he C T E Q 5L p a rto n d istrib u tio n functions (P D F ) [13] are used for the generation of all MC sam ples. T he analysis is based on th e d a ta collected w ith th e D0 detecto r [14] betw een A ugust 2002 and Septem ber 2004, 5 corresponding to an in te g ra te d lum inosity of 380 p b - 1 . T he D0 d etecto r includes a cen tral track in g system , com prised of a silicon m icrostrip track er (SM T) an d a central fiber track er (C F T ), b o th located w ithin a 2 T supercon d u ctin g solenoidal m agnet. T he SM T has « 800,000 individual strips, w ith typical p itch of 50 — 80 ^m , and a design optim ized for track in g an d vertexing capability a t p seudorapidities [15] of |n| < 2.5. T he C F T has eight coaxial barrels, each su p p o rtin g tw o d oublets of scintil latin g fibers of 0.835 m m diam eter, one doublet being parallel to th e collision axis, an d th e o th er a lte rn a tin g by ± 3 ° relative to th e axis. T hree liquid argon an d uran iu m calorim eters provide coverage o u t to |n| « 4.2: a central section covering |n| u p to « 1 . 1 , an d tw o end calorim e ters. A m uon system resides beyond th e calorim etry, and consists of a layer of track in g d etecto rs an d scintillation trig g er counters before 1.8 T iron toroids, followed by two sim ilar layers after th e toroids. Tracking a t |n| < 1 relies on 10 cm wide d rift tub es, while 1 cm m ini-drift tu b es are used a t 1 < |n| < 2. L um inosity is m easured using scin tillato r array s located in front of th e end calorim eter cry o stats, covering 2.7 < |n| < 4.4. Trigger an d d a ta acquisition system s are designed to accom m odate th e high lum inosities of th e T evatron R un II. B ased on inform ation from tracking, calorim etry, and m uon system s, th e o u tp u t of th e first tw o levels of the trig g er is used to lim it th e ra te for accepted events to < 1 kHz, relying on hard w are an d firm ware. T he th ird an d final level of th e trigger uses softw are algorithm s and a com puting farm to reduce th e o u tp u t ra te to « 50 Hz, which is w ritte n to tap e. Efficiencies for m uon an d p h o to n identification and tra c k reco n stru ctio n are determ in ed from th e sim ula tion. To verify th e sim ulation an d to estim ate system atic un certain ties, th e efficiencies have also been calculated from d a ta sam ples, using Z ^ can d id ate events and inclusive dim uon events for m uons an d tracks, and Z ^ e + e - events to determ ine th e efficiency of recon stru c tin g electrons. We assum e th a t th e different re sponse for electrons an d photo n s in th e calorim eter is p ro p erly m odelled by th e sim ulation. T he transverse (w ith respect to th e beam axis) m om entum resolution of th e cen tral track er an d th e energy resolution of the calorim eter have been tu n e d in th e sim ulation to repro duce th e resolutions observed in th e d a ta using Z ^ I I (I = e, ^ ) events. T he process pp ^ w ith ^ ^ 7 leads to a final sta te w ith tw o highly energetic isolated m uons and a pho ton. We require tw o m uons to be identified in th e m uon system an d each m atch ed to a tra c k in th e central track ing system w ith tran sv erse m om entum p T > 15 GeV. T he events have been collected w ith Level 1 trigger con ditions requiring tw o m uons d etected by th e m uon scin tillatio n counters, w ith a t least one m uon w ith tightened criteria identified by th e Level 2 trigger, an d requiring a segm ent reco n stru cted in th e m uon system above certain p T thresholds a n d /o r a tra c k in th e cen tral tracking sys tem above c ertain p T thresholds a t Level 3. T he trigger DO 3 8 0 p b -1 ■ Data h{ ® Z mm W Z incl. ■ I 100 200 300 Z Z incl. W W incl. I g misid. 400 500 600 [GeV] FIG. 2: a) Invariant dimuon mass distribution in the dimuon data sample compared to the SM expectation, b) invariant mass of the leading muon and the photon in the ßßY sam ple, for data (points with statistical uncertainties), SM back grounds (DY and diboson production, shaded histograms, as well as the uncertainty due to jets misidentified as photons), and the expected signal for m M* = 400 GeV and A = 1 TeV. efficiency has been determ ined from independent d a ta sam ples for each trigger object (muon) and trigger level separately. T he overall trigger efficiency which is applied to th e sim ulation is found to be 88 ± 6 % for th e signal after application of all selection criteria. T im ing inform ation from th e m uon scintillation coun ters is used in order to reject cosmic ray background. Since th e signal is expected to produce isolated m uons, a t least one of th e m uons is required to be isolated: th e am ount of energy deposited in th e calorim eter along th e m uon direction in a, hollow cone w ith inner radius A T I = 0.1 (A7Z = {Ai])2 + (A <f>)2) and o u te r radius A R = 0.4 is required to be less th a n 2.5 GeV, and th e sum of th e transverse m om enta of track s w ithin a cone of A R = 0.5 has to be below 2.5 GeV, excluding th e m uon track. T he cum ulative efficiency of th e m uon and trac k reco n stru ctio n and m uon identification is found to be 88 ± 4% per m uon, and th e isolation condition is 95 ± 4% efficient. T he selected dim uon sam ple contains 24853 events, w hereas 23200 ± 2700 events are expected from DY processes, and 34 ± 4 events are expected from diboson production. T he invariant dim uon m ass d istri b u tio n is show n in Fig. 2 a). N ext, a ph o to n is identified in th e event as an iso la ted cluster of calorim eter energy w ith a characteristic shower shape an d a t least 90% of th e energy deposited in th e electrom agnetic section of th e calorim eter. T he isola tio n condition is (E tot (0.4) —E em(0 .2 ))/E em(0.2) < 0.15, where E to t(0.4) and E em(0.2) denote th e energy de posited in th e calorim eter and only its electrom agnetic section in cones of size A R = 0.4 and 0.2, respectively. T he transverse energy E T m ust be larger th a n 16 GeV, no trac k is allowed to be m atched to th e ph o to n candi d ate w ith a x 2 p ro b ab lility of g reater th a n 0 . 1%, and the sum of th e transverse m om enta of tracks w ithin a hollow cone defined by 0.05 < A R < 0.4 aro u n d th e ph o to n di rection has to be below 2 G eV to fu rth er ensure isolation. T he ph o to n can d id ate is required to be sep a ra ted from 6 DO 3 8 0 p b -1 ■ Data z/g' ® mm I I g misid. Signal Et g [GeV] m ln cut «V* [GeV] [GeV] 100 200 200 200 300 280 400 330 500 440 600 440 700 440 800 440 900 440 1000 440 D ata 0 0 0 0 0 0 0 0 0 0 SM expectation 0.170 ±0.126 0.170 ±0.126 0.041 ±0.023 0.016 ±0.011 0.003 ±0.001 0.003 ±0.001 0.003 ±0.001 0.003 ±0.001 0.003 ±0.001 0.003 ±0.001 Signal eff. [%] 7.5 ± 1.0 12.5 ± 1.5 12.1 ± 1.5 14.7 ± 1.8 11.9 ± 1.5 14.4 ± 1 .8 13.6 ± 1 .7 14.5 ± 1 .8 14.7 ± 1.8 14.4 ± 1 .8 FIG. 3: For the ßßY sample, a) the distribution of the leading muon pT, and b) the photon E T. Shown are the d ata as points with statistical uncertainties, the dominant SM background (DY, shaded histogram, also shown is the uncertainty due to jets misidentified as photons), and the expected signal for m u* = 400 GeV and A = 1 TeV. TABLE I: For different values of m M*, the final selection re quirement on the invariant mass of the leading muon and the photon, the remaining data events, the SM expectation, and the signal efficiency. The quoted uncertainties include statis tical and systematic uncertainties added in quadrature. th e m uon can d id ates in th e event by a t least A R = 0.4, and has to be reco n stru cted w ithin th e cen tral p a rt of th e calorim eter (|n| < 1.1). A fter th is selection, we expect 65 ± 8 events from DY processes, an d less th a n one event from diboson produc tion. To estim ate th e possible ad d itio n al background from je ts m isidentified as photo n s an d n o t included in th e sim ulation, th e m isidentification ra te has been d eter m ined from an inclusive je t d a ta sam ple; th is ra te applied to th e dim uon plus je t sam ple resu lts in 39 ± 5 such events in th e UUY selection. As a function of E T , th e p h o to n fake ra te is a b o u t 0.5% p er je t a t low E T , an d is negligible above « 80 GeV. T he b ackground from je ts m isidentified as photo n s is tre a te d as a system atic uncertainty, resu lt ing in a to ta l SM ex p ectatio n of 65 ± 8 - 0 9 events. We find 90 events in th e d a ta , in good agreem ent w ith the expectatio n . T he invariant m ass of th e leading m uon and th e p h o to n is show n in Fig. 2 b) for th e d a ta , SM expec ta tio n , an d signal ex p ectatio n for m M* = 400 G eV and A = 1 TeV. T he p T d istrib u tio n of th e leading m uon and th e E t d istrib u tio n of th e p h o to n are show n in Fig. 3. A dditional selection criteria are applied to reduce the rem aining SM background. T he p h o to n E T is required to be larger th a n 27 GeV. T he efficiency to identify a pho to n is co n stan t a t a b o u t 90% above th is value. T he final discrim in an t to suppress rem aining SM backgrounds is th e invariant m ass of th e leading m uon an d th e photon. For m asses m M* above « 300 GeV, th e leading m uon is pred o m in an tly th e m uon from th e u * decay. In order to m axim ize th e sensitivity of th e analysis, th e signal ex p ec ta tio n is calcu lated for A = 1 TeV, th e background including DY processes an d diboson p ro d u ction is con sidered, an d a c u t value is chosen for each value of m M*. T he resu lt is shown in Table I along w ith th e SM ex p ec ta tio n for th e num ber of d a ta events an d th e signal efficiency, w hich varies betw een 8% an d 15%. T he d o m in an t sy stem atic u n certain ties are as follows. T he u n c e rta in ty on th e SM cross sections is dom inated by th e DY process an d th e u n c e rta in ty from th e choice of P D F and renorm alization and factorization scales (4%). M uon reco n stru ctio n and identification have an uncer ta in ty of 4% per m uon, and a 3% erro r is assigned to the ph o to n identification. T he u n certa in ty due to th e trig ger efficiency is 7%. T he in te g ra ted lum inosity is know n to a precision of 6.5% [16]. T he u n c e rtain ty due to je ts m isidentified as photons is dom inant after all selection criteria for m M* u p to 400 GeV: for m M* = 100 GeV (400 GeV), 0.097 (0.008) such “fake” photons are ex pected, while for m M* = 500 GeV and above th is back ground is negligible (< 10-5 events). T he u n ce rtain ty on th e signal cross section is e stim ated to be 10%, con sisting of P D F u n certainties and unknow n higher order corrections. Since no events are found in th e d a ta , in agreem ent w ith th e SM expectation, we set 95% confidence level lim its on th e u * p ro d u ctio n cross section tim es th e branching fraction into UY. A B ayesian technique [17] is used, ta k ing into account all u n certainties and tre a tin g th em as sym m etric for simplicity. T he resulting lim it as a func tio n of m M* is show n in Fig. 4 to g eth er w ith predictions of th e co n tact in teractio n m odel for different choices of th e scale A. For A = 1 TeV (A = m M* ), m asses below 618 GeV (688 GeV) are excluded. In Fig. 5 th e excluded region in term s of A and m M* is shown. T he C D F collaboration has recently searched [6] for th e pro d u ctio n of excited electrons, and ob tain ed com p arable cross section lim its, b u t th e C D F m ass lim it of m e* > 879 GeV a t 95% C.L. for A = m e* can n o t be d irectly com pared to ours for two reasons. T he cross section calculated w ith th e version of PY TH IA used by C D F is a factor of two higher th a n in subsequent ver sions corrected by th e PY TH IA authors. F urtherm ore, C D F assum es th a t decays via co n tact in teractio n s can be neglected, while in our analysis such decays are tak en into account in th e calculation of th e branching frac tio n u* ^ UY, following [3, 8]. If we ad ju sted our re sult for these two differences, we would o b tain a lim it of m M* > 890 GeV a t 95% C.L. for A = m M*. 7 In sum m ary, we have searched for th e pro d u ctio n of excited m uons in th e process p p ^ u* U w ith u* ^ UY, using 380 p b -1 of d a ta collected w ith th e D0 detector. We find no events in th e d a ta , com patible w ith th e SM expectation, and set lim its on th e p ro d u ctio n cross sec tio n tim es branching fraction as a function of th e m ass of th e excited m uon. For a scale p ara m e ter A = 1 TeV, m asses below 618 G eV are excluded, representing the m ost strin g e n t lim it to date. FIG. 4: The measured cross section x branching fraction limit, compared to the contact interaction model prediction for different choices of A. For the case A = 1 TeV, the theo retical uncertainty of the model prediction is indicated. : D O 3 8 0 p b -1 p p ® m"m m ® mg ' e x c lu d e d at 95% CL ......................I . . . . I . . . ...................................... 200 250 300 350 400 450 500 550 600 mm[GeV] FIG. 5: The region in the plane of A and m M* excluded by the present analysis. We th a n k A. Daleo and M. K ram er for useful discus sions, and A. Daleo for providing us w ith th e NNLO cor rections to th e u* pro d u ctio n cross section. We th a n k th e staffs a t Ferm ilab and collaborating in stitu tio n s, and acknowledge su p p o rt from th e D O E and NSF (USA); C E A and C N R S /IN 2 P 3 (France); FASI, R osatom and R F B R (Russia); C A PE S, C N Pq, F A P E R J, F A P E S P and FU N D U N E SP (Brazil); DAE and D ST (India); Colciencias (Colom bia); C O N A C yT (Mexico); K R F and K O S E F (K orea); C O N IC E T and U B A C yT (A rgentina); FO M (T he N etherlands); P PA R C (U nited K ingdom ); M SM T (Czech Republic); CRC P rogram , C FI, NSERC and W estG rid P ro je c t (C anada); B M B F and D FG (G er m any); SFI (Ireland); T he Swedish R esearch Council (Sweden); Research C orporation; A lexander von H um b o ld t F oundation; and th e M arie C urie P rogram . [*] On leave from IEP SAS Kosice, Slovakia. [f] Visitor from Helsinki Institute of Physics, Helsinki, Fin land. [1] H. Terazawa, M. Yasue, K. Akama and M. Hayashi, Phys. Lett. B 112, 387 (l982); F.M. Renard, Il Nuovo Cimento 77 A, 1 (1983); A. 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