Measurement of dijet angular distributions by the collider detector at fermilab

Published

Journal Article

We have used 106pb-1 of data collected in pp collisions at √s = 1.8 TeV by the Collider Detector at Fermilab to measure jet angular distributions in events with two jets in the final state. The angular distributions agree with next to leading order predictions of QCD in all dijet invariant mass regions. The data exclude at 95% CL a model of quark substructure in which only up and down quarks are composite and the contact interaction scale is ⩘+ud≤1.6 TeV or ⩘-ud≤1.4 TeV. For a model in which all quarks are composite the excluded regions are ⩘+≤1.8 TeV and ⩘-≤1.6 TeV. © 1996 The American Physical Society.

Full Text

Duke Authors

Cited Authors

  • Abe, F; Akimoto, H; Akopian, A; Albrow, MG; Amendolia, SR; Amidei, D; Antos, J; Anway-Wiese, C; Aota, S; Apollinari, G; Arisawa, T; Asakawa, T; Ashmanskas, W; Atac, M; Azfar, F; Azzi-Bacchetta, P; Bacchetta, N; Badgett, W; Bagdasarov, S; Bailey, MW; Bao, J; de Barbaro, P; Barbaro-Galtieri, A; Barnes, VE; Barnett, BA; Barzi, E; Bauer, G; Baumann, T; Bedeschi, F; Behrends, S; Belforte, S; Bellettini, G; Bellinger, J; Benjamin, D; Benlloch, J; Bensinger, J; Benton, D; Beretvas, A; Berge, JP; Berryhill, J; Bertolucci, S; Bevensee, B; Bhatti, A; Biery, K; Binkley, M; Bisello, D; Blair, RE; Blocker, C; Bodek, A; Bokhari, W; Bolognesi, V; Bolla, G; Bortoletto, D; Boudreau, J; Breccia, L; Bromberg, C; Bruner, N; Buckley-Geer, E; Budd, HS; Burkett, K; Busetto, G; Byon-Wagner, A; Byrum, KL; Cammerata, J; Campagnari, C; Campbell, M; Caner, A; Carithers, W; Carlsmith, D; Castro, A; Cauz, D; Cen, Y; Cervelli, F; Chang, PS; Chang, PT; Chao, HY; Chapman, J; Cheng, MT; Chiarelli, G; Chikamatsu, T; Chiou, CN; Christofek, L; Cihangir, S; Clark, AG; Cobal, M; Cocca, E; Contreras, M; Conway, J; Cooper, J; Cordelli, M; Couyoumtzelis, C; Crane, D; Cronin-Hennessy, D; Culbertson, R; Daniels, T; De Jongh, F; Delchamps, S; Dell’agnello, S; Dell’orso, M; Demina, R

Published Date

  • January 1, 1996

Published In

Volume / Issue

  • 77 / 27

Start / End Page

  • 5336 - 5341

Electronic International Standard Serial Number (EISSN)

  • 1079-7114

International Standard Serial Number (ISSN)

  • 0031-9007

Digital Object Identifier (DOI)

  • 10.1103/PhysRevLett.77.5336

Citation Source

  • Scopus