We have measured dijet angular distributions at √s =1.8 TeV with the Collider Detector at Fermilab and the Tevatron p¯p Collider and find agreement with leading-order QCD. By comparing the distribution for the highest dijet invariant masses with the prediction of a model of quark compositeness, we set a lower limit on the associated scale parameter Λc at 330 GeV (95% C.L.).

Dijet angular distributions from p¯p collisions at √s=1.8 TeV / F. Abe;D. Amidei;G. Apollinari;G. Ascoli;M. Atac;P. Auchincloss;A. Baden;A. Barbaro-Galtieri;V. Barnes;F. Bedeschi;S. Behrends;S. Belforte;G. Bellettini;J. Bellinger;J. Bensinger;A. Beretvas;P. Berge;S. Bertolucci;S. Bhadra;M. Binkley;R. Blair;C. Blocker;J. Bofill;A. Booth;G. Brandenburg;D. Brown;A. Byon;K. Byrum;M. Campbell;R. Carey;W. Carithers;D. Carlsmith;J. Carroll;R. Cashmore;F. Cervelli;K. Chadwick;T. Chapin;G. Chiarelli;W. Chinowsky;S. Cihangir;D. Cline;D. Connor;M. Contreras;J. Cooper;M. Cordelli;M. Curatolo;C. Day;R. DelFabbro;M. Dell’Orso;L. DeMortier;T. Devlin;D. DiBitonto;R. Diebold;F. Dittus;A. DiVirgilio;J. Elias;R. Ely;S. Errede;S. Esposito;B. Flaugher;E. Focardi;G. Foster;M. Franklin;J. Freeman;H. Frisch;Y. Fukui;A. Garfinkel;P. Giannetti;N. Giokaris;P. Giromini;L. Gladney;M. Gold;K. Goulianos;C. Grosso-Pilcher;C. Haber;S. Hahn;R. Handler;R. Harris;J. Hauser;T. Hessing;R. Hollebeek;P. Hu;B. Hubbard;P. Hurst;J. Huth;H. Jensen;R. Johnson;U. Joshi;R. Kadel;T. Kamon;S. Kanda;D. Kardelis;I. Karliner;E. Kearns;R. Kephart;P. Kesten;H. Keutelian;S. Kim;L. Kirsch;K. Kondo;U. Kruse;S. Kuhlmann;A. Laasanen;W. Li;T. Liss;N. Lockyer;F. Marchetto;R. Markeloff;L. Markosky;P. McIntyre;A. Menzione;T. Meyer;S. Mikamo;M. Mil-;T. Mimashi;S. Miscetti;M. Mishina;S. Miyashita;N. Mondal;S. Mori;Y. Morita;A. Mukherjee;C. Newman-Holmes;L. Nodulman;R. Paoletti;A. Para;J. Patrick;T. Phillips;H. Piekarz;R. Plunkett;L. Pondrom;J. Proudfoot;G. Punzi;D. Quarrie;K. Ragan;G. Redlinger;J. Rhoades;F. Rimondi;L. Ristori;T. Rohaly;A. Roodman;A. Sansoni;R. Sard;V. Scarpine;P. Schlabach;E. Schmidt;P. Schoessow;M. Schub;R. Schwitters;A. Scribano;S. Segler;M. Sekiguchi;P. Sestini;M. Shapiro;M. Sheaff;M. Shibata;M. Shochet;J. Siegrist;P. Sinervo;J. Skarha;D. Smith;F. Snider;R. St. Denis;A. Stefanini;Y. Takaiwa;K. Takikawa;S. Tarem;D. Theriot;A. Tollestrup;G. Tonelli;Y. Tsay;F. Ukegawa;D. Underwood;R. Vidal;R. Wagner;R. Wagner;J. Walsh;T. Watts;R. Webb;T. Westhusing;S. White;A. Wicklund;H. Williams;T. Yamanouchi;A. Yamashita;K. Yasuoka;G. Yeh;J. Yoh;F. Zetti. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - ELETTRONICO. - 62:(1989), pp. 3020-3023. [10.1103/PhysRevLett.62.3020]

Dijet angular distributions from p¯p collisions at √s=1.8 TeV

FOCARDI, ETTORE;
1989

Abstract

We have measured dijet angular distributions at √s =1.8 TeV with the Collider Detector at Fermilab and the Tevatron p¯p Collider and find agreement with leading-order QCD. By comparing the distribution for the highest dijet invariant masses with the prediction of a model of quark compositeness, we set a lower limit on the associated scale parameter Λc at 330 GeV (95% C.L.).
1989
62
3020
3023
F. Abe;D. Amidei;G. Apollinari;G. Ascoli;M. Atac;P. Auchincloss;A. Baden;A. Barbaro-Galtieri;V. Barnes;F. Bedeschi;S. Behrends;S. Belforte;G. Bellettini;J. Bellinger;J. Bensinger;A. Beretvas;P. Berge;S. Bertolucci;S. Bhadra;M. Binkley;R. Blair;C. Blocker;J. Bofill;A. Booth;G. Brandenburg;D. Brown;A. Byon;K. Byrum;M. Campbell;R. Carey;W. Carithers;D. Carlsmith;J. Carroll;R. Cashmore;F. Cervelli;K. Chadwick;T. Chapin;G. Chiarelli;W. Chinowsky;S. Cihangir;D. Cline;D. Connor;M. Contreras;J. Cooper;M. Cordelli;M. Curatolo;C. Day;R. DelFabbro;M. Dell’Orso;L. DeMortier;T. Devlin;D. DiBitonto;R. Diebold;F. Dittus;A. DiVirgilio;J. Elias;R. Ely;S. Errede;S. Esposito;B. Flaugher;E. Focardi;G. Foster;M. Franklin;J. Freeman;H. Frisch;Y. Fukui;A. Garfinkel;P. Giannetti;N. Giokaris;P. Giromini;L. Gladney;M. Gold;K. Goulianos;C. Grosso-Pilcher;C. Haber;S. Hahn;R. Handler;R. Harris;J. Hauser;T. Hessing;R. Hollebeek;P. Hu;B. Hubbard;P. Hurst;J. Huth;H. Jensen;R. Johnson;U. Joshi;R. Kadel;T. Kamon;S. Kanda;D. Kardelis;I. Karliner;E. Kearns;R. Kephart;P. Kesten;H. Keutelian;S. Kim;L. Kirsch;K. Kondo;U. Kruse;S. Kuhlmann;A. Laasanen;W. Li;T. Liss;N. Lockyer;F. Marchetto;R. Markeloff;L. Markosky;P. McIntyre;A. Menzione;T. Meyer;S. Mikamo;M. Mil-;T. Mimashi;S. Miscetti;M. Mishina;S. Miyashita;N. Mondal;S. Mori;Y. Morita;A. Mukherjee;C. Newman-Holmes;L. Nodulman;R. Paoletti;A. Para;J. Patrick;T. Phillips;H. Piekarz;R. Plunkett;L. Pondrom;J. Proudfoot;G. Punzi;D. Quarrie;K. Ragan;G. Redlinger;J. Rhoades;F. Rimondi;L. Ristori;T. Rohaly;A. Roodman;A. Sansoni;R. Sard;V. Scarpine;P. Schlabach;E. Schmidt;P. Schoessow;M. Schub;R. Schwitters;A. Scribano;S. Segler;M. Sekiguchi;P. Sestini;M. Shapiro;M. Sheaff;M. Shibata;M. Shochet;J. Siegrist;P. Sinervo;J. Skarha;D. Smith;F. Snider;R. St. Denis;A. Stefanini;Y. Takaiwa;K. Takikawa;S. Tarem;D. Theriot;A. Tollestrup;G. Tonelli;Y. Tsay;F. Ukegawa;D. Underwood;R. Vidal;R. Wagner;R. Wagner;J. Walsh;T. Watts;R. Webb;T. Westhusing;S. White;A. Wicklund;H. Williams;T. Yamanouchi;A. Yamashita;K. Yasuoka;G. Yeh;J. Yoh;F. Zetti
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/627192
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