1. High pt Jets in $p\bar p$ Collisions at $\sqrt S$ = 630 and 1800 GeV
- Author
-
Abbott, B., Abdesselam, Abdelmalek, Abolins, M., Abramov, V., Acharya, B S., Adams, D L., Adams, M., Alves, G A., Amos, N., Anderson, E W., Astur, R., Baarmand, M M., Babintsev, V V., Babukhadia, L., Bacon, T C., Baden, A., Baldin, B., Balm, P W., Todorova-Nova, S., Barberis, E., Baringer, P., Bartlett, J F., Bassler, U., Bauer, D., Bean, A., Begel, M., Belyaev, A., Beri, S B., Bernardi, G., Bertram, I., Besson, A., Beuselinck, R., Bezzubov, V A., Bhat, P C., Bhatnagar, V., Bhattacharjee, M., Blazey, G C., Blessing, S., Bohnlein, A., Bozhko, N., Borcherding, F., Brandt, A., Breedon, R., Briskin, G., Brock, R., Brooijmans, G., Bross, A., Buchholz, D., Buehler, M., Buescher, V., Burtovoi, V S., Butler, J M., Canelli, F., Carvalho, W., Casey, D., Casilum, Z., Castilla-Valdez, H., Chakraborty, D., Chan, K M., Chekulaev, S V., Cho, D K., Choi, S., Chopra, S., Christenson, J H., Chung, M., Claes, D., Clark, a R., Cochran, J., Coney, L., Connolly, B., Cooper, W E., Coppage, D., Cummings, M a C., Cutts, D., Davis, G A., Davis, K., De, K., del Signore, K., Demarteau, M., Demina, R., Demine, P., Denisov, D S., Denisov, S P., Desai, S., Diehl, H T., Diesburg, M., Diloreto, G., Doulas, S., Draper, P., Ducros, Y., Dudko, L V., Duensing, S., Duflot, L., Dugad, S R., Dyshkant, A., Edmunds, D., Ellison, J., Elvira, V D., Engelmann, R., Eno, S., Eppley, G., Ermolov, P., Eroshin, O V., Estrada, J., Evans, H., Evdokimov, V N., Fahland, T., Fatyga, M K., Feher, S., Fein, D., Ferbel, T., Fisk, H E., Fisyak, Yu., Flattum, E., Fleuret, F., Fortner, M., Frame, K C., Fuess, S., Gallas, E., Galyaev, a N., Gao, M., Gavrilov, V., Geld, T L., Genik, R J., Genser, K., Gerber, C E., Gershtein, Yu., Gilmartin, R., Ginther, G., Gomez, B., Gomez, G., Goncharov, P I., Gonzalez-Solis, J L., Gordon, H., Goss, L T., Gounder, K., Goussiou, A., Graf, N., Graham, G., Grannis, P D., Green, J A., Greenlee, H., Grinstein, S., Groer, L., Gruenendahl, S., Sen-Gupta, A., Gurzhev, S N., Gutierrez, G., Gutierrez, P., Hadley, N J., Haggerty, H., Hagopian, S., Hagopian, V., Hahn, K S., Hall, R E., Hanlet, P., Hansen, Scott, Hauptman, J M., Hays, C., Hebert, Christian, Hedin, D., Heinson, a P., Heintz, U., Heuring, T C., Hirosky, R., Hobbs, J D., Hoeneisen, B., Hoftun, J S., Hou, S., Huang, Yue, Illingworth, R., Ito, a S., Jaffre, M., Jerger, S A., Jesik, R., Johns, K., Johnson, M., Jonckheere, A., Jones, M., Joestlein, H., Juste, A., Kahn, S., Kajfasz, E., Karmanov, D., Karmgard, D., Kehoe, R., Kim, S K., Klima, B., Klopfenstein, C., Knuteson, B., Ko, W., Kohli, J M., Kostritskii, a V., Kotcher, J., Kotwal, a V., Kozelov, a V., Kozlovskii, E A., Krane, J., Krishnaswamy, M R., Krzywdzinski, S., Kubantsev, M., Kuleshov, S., Kulik, Y., Kunori, S., Kuznetsov, V E., Landsberg, G L., Leflat, A., Leggett, C., Lehner, F., Li, J., Li, Q Z., Lima, J G R., Lincoln, D., Linn, S L., Linnemann, J., Lipton, R., Lucotte, A., Lueking, L., Lundstedt, C., Luo, C., Maciel, a K A., Madaras, R J., Manankov, V., Mao, H S., Marshall, T., Martin, M I., Martin, R D., Mauritz, K M., May, B., Mayorov, a A., Mccarthy, R., Mcdonald, J., Mcmahon, T., Melanson, H L., Meng, X C., Merkin, M., Merritt, K W., Miao, C., Miettinen, H., Mihalcea, D., Mishra, C S., Mokhov, N., Mondal, N K., Montgomery, H E., Moore, R W., Mostafa, M., da Motta, H., Nagy, E., Nang, F., Narain, M., Narasimham, V S., Neal, H A., Negret, J P., Negroni, S., Norman, D., Nunnemann, T., Oesch, L., Oguri, V., Olivier, B., Oshima, N., Padley, P., Pan, L J., Papageorgiou, K., Para, A., Parashar, N., Partridge, R., Parua, N., Paterno, M., Patwa, A., Pawlik, B., Perkins, J., Peters, M., Peters, O., Petroff, P., Piegaia, R., Piekarz, H., Pope, B G., Popkov, E., Prosper, H B., Protopopescu, S., Qian, J., Quintas, P Z., Raja, R., Rajagopalan, S., Ramberg, E., Rapidis, P A., Reay, N W., Reucroft, S., Rha, J., Ridel, M., Rijssenbeek, M., Rockwell, T., Roco, M., Rubinov, P., Ruchti, R., Rutherfoord, J., Santoro, A., Sawyer, L., Schamberger, R D., Schellman, H., Schwartzman, A., Sen, N., Shabalina, E., Shivpuri, R K., Shpakov, D., Shupe, M., Sidwell, R A., Simak, V., Singh, H., Singh, J B., Sirotenko, V., Slattery, P., Smith, E., Smith, R P., Snihur, R., Snow, G R., Snow, J., Snyder, S., Solomon, J., Sorin, V., Sosebee, M., Sotnikova, N., Soustruznik, K., Souza, M., Stanton, N R., Steinbruck, G., Stephens, R W., Stichelbaut, F., Stoker, D., Stolin, V., Stoyanova, D A., Strauss, M., Strovink, M., Stutte, L., Sznajder, A., Taylor, W., Tentindo-Repond, S., Thompson, J., Toback, D., Tripathi, S M., Trippe, T G., Turcot, a S., Tuts, P M., van Gemmeren, P., Vaniev, V., van Kooten, R., Varelas, N., Volkov, a A., Vorobev, a P., Wahl, H D., Wang, H., Wang, Z M., Warchol, J., Watts, G., Wayne, M., Weerts, H., White, A., White, J T., Whiteson, D., Wightman, J A., Wijngaarden, D A., Willis, S., Wimpenny, S J., Wirjawan, J V D., Womersley, J., Wood, D R., Yamada, R., Yamin, P., Yasuda, T., Yip, K., Youssef, S., Yu, J., Yu, Z., Zanabria, M., Zheng, H., Zhou, Z., Zielinski, M., Zieminska, D., Zieminski, A., Zutshi, V., Zverev, E G., Zylberstejn, A., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), D0, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
- Subjects
High Energy Physics - Experiment (hep-ex) ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Phenomenology ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,FOS: Physical sciences ,High Energy Physics::Experiment ,Nuclear Experiment ,High Energy Physics - Experiment - Abstract
Results are presented from analyses of jet data produced in pbarp collisions at sqrt{s} = 630 and 1800 GeV collected with the DO detector during the 1994-95 Fermilab Tevatron Collider run. We discuss details of detector calibration, and jet selection criteria in measurements of various jet production cross sections at sqrt{s} = 630 and 1800 GeV. The inclusive jet cross sections, the dijet mass spectrum, the dijet angular distributions, and the ratio of inclusive jet cross sections at sqrt{s} = 630 and 1800 GeV are compared to next-to-leading-order QCD predictions. The order alpha_s^3 calculations are in good agreement with the data. We also use the data at sqrt{s} = 1800 GeV to rule out models of quark compositeness with a contact interaction scale less than 2.2 TeV at the 95% confidence level., 158 pages, 105 figures, submitted to Phys. Rev. D. Corrected missing citation on page 137 (should be [55])
- Published
- 2001
- Full Text
- View/download PDF