Paper
Document
Download
Flag content
0

Evidence for top quark production inp ̄pcollisions at √s=1.8 TeV

Authors
F. Abe,M. Albrow
S. Amendolia,L. Feligioni,L. Scodellaro,C. Anway-Wiese,G. Apollinari,H. Areti,P. Auchincloss,Matthew Austern,G. Latino,L. Lista,N. Bacchetta,W. Badgett,M. Bailey,J. Bao,P. Barbaro,D. Cauz,B. Akgün,P. Barria,P. Bartalini,G. Bauer,T. Baumann,F. Bedeschi,S. Behrends,S. Belforte,G. Bellettini,J. Dittmann,G. Introzzi,O. Botner,J. Bensinger,D. Benton,A. Beretvas,J. Bergé,S. Bertolucci,A. Bhatti,K. Biery,M. Binkley,J. Bird,D. Bisello,R. Blair,C. Blocker,A. Bodek,V. Bolognesi,D. Bortoletto,C. Boswell,T. Boulos,P. Branchini,E. Buckley‐Geer,H. Budd,K. Burkett,G. Busetto,A. Byon-Wagner,K. Byrum,C. Campagnari,M. Campbell,A. Caner,W. Carithers,M. Casarsa,M. Cuffiani,Y. Cen,F. Cervelli,J. Chapman,M.-T. Cheng,G. Chiarelli,T. Chikamatsu,S. Cihangir,A. Clark,M. Cobal,M. Contreras,J. Conway,J. Cooper,V. Sharma,D. Crane,J. Cunningham,T. Daniels,F. DeJongh,S. Delchamps,F. Grancagnolo,M. Dell’Orso,L. Demortier,B. Denby,G. Velev,P. Derwent,T. Devlin,M. Dickson,M. Donadelli,J. Conrad,A. Dunn,H. Jarrari,J. Elias,R. Ely,E. Engels,Sarah Eno,D. Errede,S. Errede,Q. Fan,B. Farhat,I. Palma,R. Foley,A. Wicklund,M. Franklin,M. Frautschi,J. Freeman,J. Friedman,M. Iori,A. Fry,T. Fuess,Y. Fukui,S. Funaki,G. Gagliardi,S. Galeotti,M. Gallinaro,A. Garfinkel,S. Geer,D. Gerdes,P. Giannetti,P. Giromini,L. Gladney,D. Glenzinski,M. Gold,R. Suarez,A. Gordon,I. Gorelov,K. Goulianos,H. Grassmann,A. Grewal,G. Grieco,L. Groer,C. Grosso-Pilcher,C. Haber,J. Huston,R. Hamilton,R. Handler,R. Hans,K. Hara,B. Harral,R. Harris,S. Hauger,J. Hauser,C. Hawk,J. Heinrich,Daniel Hennessy,R. Hollebeek,L. Holloway,A. Hölscher,S. Hong,G. Houk,P. Hu,T. Huffman,M. Mooney,P. Hurst,A. Laasanen,G. Iacobucci,J. Hylen,M. Incagli,J. Incandela,H. Iso,H. Jensen,G. Simi,U. Joshi,R. Kadel,E. Kajfasz,D. Kar,T. Kaneko,D. Kardelis,H. Kasha,Y. Kato,L. Keeble,R. Kennedy,R. Kephart,P. Kesten,D. Kestenbaum,R. Keup,H. Keutelian,F. Keyvan,D. Kim,H. Kim,S. Kim,Y. Kim,J. Kirk,P. Koehn,T. Kobayashi,J. Konigsberg,S. Köpp,K. Korcyl,W. Koska,E. Kovacs,W. Kowald,M. Krasberg,J. Kroll,M. Kruse,S. Kuhlmann,E. Kuns,G. Alverson,J. Lamoureux,I. Lazzizzera,S. Leone,P. Limon,M. Lindgren,A. Lister,O. Long,M. Loreti,E. Low,J. Lu,D. Lucchesi,C. Luchini,P. Lukens,R. Lysák,P. Maas,K. Maeshima,A. Maghakian,P. Maksimovic,Cristina Manuel,J. Mansour,M. Mariotti,A. Martin,R. Mattingly,K. McFarland,P. Mélèse,A. Menzione,E. Meschi,G. Michail,S. Mikamo,M. Miller,Robert Miller,T. Mimashi,S. Miscetti,M. Mishina,H. Mitsushio,S. Miyashita,R. Moore,S. Moulding,J. Mueller,A. Mukherjee,T. Müller,P. Musgrave,L. Nakae,M. Nagel,Charles Nelson,D. Neuberger,L. Taylor,J. Nielsen,S. Nishida,J. Ocariz,K. Ohl,R. Oishi,T. Okusawa,R. Orava,R. Paoletti,A. Parri,M. Paulini,Michael Peters,T. Phillips,G. Piacentino,M. Pillai,L. Pondrom,N. Produit,F. Ptochos,G. Punzi,F. Rimondi,A. Robson,M. Roach-Bellino,V. Zutshi,Teresa Rodrigo,J. Romano,L. Rosenson,T. Saab,D. Saltzberg,A. Santra,A. Plazas,A. Schindler,P. Schlabach,E. Schmidt,M. Schmidt,O. Schneider,C. Sciacca,S. Segler,S. Seidel,Y. Seiya,G. Sganos,A. Sgolacchia,E. Shabalina,M. Shimojima,Q. Shen,J. Siegrist,A. Sill,P. Singh,J. Skarha,K. Śliwa,C. Vernieri,P. Sørensen,T. Song,J. Spalding,L. Spiegel,P. Sphicas,A. Spies,L. Stančo,J. Steele,A. Stefanini,K. Strahl,J. Strait,David Stuart,G. Sullivan,G. Raven,R. Swartz,T. Takahashi,K. Takikawa,W. Taylor,G. Taylor,K. Terashi,D. Theriot,R. Takashima,M. Togawa,R. Thun,M. Timko,E. Thomson,A. Titov,S. Tkaczyk,A. Tollestrup,J. Tonnison,B. González,S. Trincaz-Duvoid,M. Bóna,N. Turini,N. Uemura,G. Unal,S. Brink,S. Vejcik,R. Cortabitarte,R. Wagner,N. Wainer,R. Walker,G. Wang,J. Wang,M. Wang,Q. Wang,A. Warburton,R. Webb,C. Wendt,H. Wenzel,T. Westhusing,R. Wilkinson,P. Wilson,B. Winer,J. Wolinski,D. Wu,X. Wu,J. Wyss,A. Yagil,W-M. Yao,K. Yasuoka,Y. Ye,G. Yeh,P. Yeh,M. Yin,K. Yorita,D. Yovanovitch,I. Yu,J. Yun,A. Zanetti,F. Zetti,L. Zhang,S. Zhang,W. Zhang,R. Coutinho,D. Amidei,J. Antos̆,F. Azfar,Patrizia Azzi,A. Barbaro‐Galtieri,V. Barnes,B. Barnett,J. Bellinger,D. Benjamin,James Bensinger,G. Brandenburg,D. Carlsmith,A. Castro,M. Cordelli,D. Coupal,S. Dell’Agnello,M. Deninno,S. Donati,R. Drucker,K. Einsweiler,S. Eno,I. Fiori,Lorenzo Feligioni,Raffaello d'Alessandro,Bora Akgün,Patrizia Barria,Jay Dittmann,A. Ivanov,Marco Cuffiani,Yassine Ghazali
+394 authors
,A. Ereditato
Published
Sep 1, 1994
Show more
Save
TipTip
Document
Download
Flag content
0
TipTip
Save
Document
Download
Flag content

Abstract

We present the results of a search for the top quark in 19.3 pb−1 of p¯p collisions at √s =1.8 TeV. The data were collected at the Fermilab Tevatron collider using the Collider Detector at Fermilab (CDF). The search includes standard model tt¯ decays to final states eeνν¯, eμνν¯, and μμνν¯ as well as e+ν+jets or μ+ν+jets. In the (e,μ)+ν+jets channel we search for b quarks from t decays via secondary vertex identification and via semileptonic decays of the b and cascade c quarks. In the dilepton final states we find two events with a background of 0.56+0.25−0.13 events. In the e,μ+ν+jets channel with a b identified via a secondary vertex, we find six events with a background of 2.3±0.3. With a b identified via a semileptonic decay, we find seven events with a background of 3.1±0.3. The secondary vertex and semileptonic-decay samples have three events in common. The probability that the observed yield is consistent with the background is estimated to be 0.26%. The statistics are too limited to firmly establish the existence of the top quark; however, a natural interpretation of the excess is that it is due to tt¯ production. We present several cross-checks. Some support this hypothesis; others do not. Under the assumption that the excess yield over background is due to tt¯, constrained fitting on a subset of the events yields a mass of 174±10+13−12 GeV/c2 for the top quark. The tt¯ cross section, using this top quark mass to compute the acceptance, is measured to be 13.9+6.1−4.8 pb.Received 25 April 1994DOI:https://doi.org/10.1103/PhysRevD.50.2966©1994 American Physical Society

Paper PDF

This paper's license is marked as closed access or non-commercial and cannot be viewed on ResearchHub. Visit the paper's external site.