UvA-DARE ( Digital Academic Repository ) Rapidity gaps between jets in photoproduction at HERA
UvA-DARE ( Digital Academic Repository ) Rapidity gaps between jets in photoproduction at HERA
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UvA-DARE(数字学术存储库)HERA 摄影制作中喷气机之间的速度差距
DOI:
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发表时间:
2003
期刊:
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通讯作者:
A. Whitfield
中科院分区:
文献类型:
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作者:
L. Adamczyk;B. Bednarek;K. Jeleń;D. Kisielewska;T. Kowalski;M. Przybycied;E. Rulikowska;L. Suszycki;J. Zaja̧c;H. Beier;J. Bienlein;C. Coldewey;K. Desler;D. Gilkinson;C. Glasman;P. Giittlicher;J. Grobe;B. Gutj;D. Hasell;H. Helling;Y. Iga;K. Johnson;P. Joos;M. Kasemann;R. Klanner;W. Koch;L. Kiipke;H. Kowalski;B. Liihr;M. Lowe;D. Luke;J. Mainusch;T. Monteiro;J. Ng;S. Nickel;Notz;K. Ohrenberg;M. Roco;M. Rohde;J. Roldan;U. Schneekloth;W. Schulz;F. Selonke;E. Stiliaris;B. Surrow;D. Westphal;G. Wolf;C. Youngman;W. Zeuner;J. F. Zhou;A. Leich;Sm;Mari;K. M.;Mattingly;A. Meyer;S. Schlenstedt;G. Maccarrone;S. Pasquale;L. Votano;A. Freidhof;J. Schroeder;T. Trefzger;M. Utley;E. Baduraz;B. Burow;L. Hagge;Lohrmann;J. Milewski;M. Nakahata;A. Whitfield
Photoproduction events which have two or more jets have been studied in the W,, range 135 GeV < W,, < 280 GeV with the ZEUS detector at HERA. A class of events is observed with little hadronic activity between the jets. The jets are separated by pseudorapidity intervals (Ar]) of up to four units and have transverse energies greater than 6 GeV. A gap is defined as the absence between the jets of particles with transverse energy greater than 300 MeV. The fraction of events containing a gap is measured as a function of AT. It decreases exponentially as expected for processes in which colour is exchanged between the jets, up to a value of AT 3, then reaches a constant value of about 0.1. The excess above the exponential fall-off can be interpreted as evidence for hard diffractive scattering via a strongly interacting colour singlet object. ’ Also at IROE Florence, Italy. * Now at Univ. of Salerno and INFN Napoli, Italy. 3 Supported by EU HCM contract ERB-CHRX-CT93-0376. 4 Supported by Worldlab, Lausanne, Switzerland. 5 Now a self-employed consultant. 6 Now at ELEKLUFT, Bonn. ’ Now also at University of Torino. * Alexander von Humboldt Fellow. g Alfred P. Sloan Foundation Fellow. lo Now at Inst. of Computer Science, Jagellonian Univ., Cracow. l1 Now at Comma-Soft, Bonn. ‘* Visitor from Florida State University. I3 Now at Univ. of Mainz. I4 Now at DESY Computer Center. I5 Supported by European Community Program PRAXIS XXI. l6 Now at Dr. Seidel Informationssysteme, Frankfurt/M. ” Now at Inst. of Accelerating Systems & Applications (IASA), Athens. l8 Now at Mercer Management Consulting, Munich. lg Now at Univ. de Strasbourg. ” Now at Andrews University, Barrien Springs, USA. *’ Now with OPAL Collaboration, Faculty of Physics at Univ. of Freiburg. ** Now at SAS-Institut GmbH, Heidelberg. u Now at GSI Darmstadt. 24 Also supported by NSERC. Z Now at Institute for Cosmic Ray Research, University of Tokyo. 26 Partially supported by CAM. ” Partially supported by DESY. 28 Now at Philips Natlab, Eindhoven, NL. 2g Now at Carleton University, Ottawa, Canada. 3o Now at Department of Energy, Washington. 31 Now at HEP Div., Argonne National Lab., Argonne, IL, USA. 32 Now at Oxford Magnet Technology, Eynsham, Oxon. 33 In part supported by Argonne National Laboratory. 34 Supported by a MINERVA Fellowship. 35 Now at Centre for Subatomic Research, Univ.of Alberta, Canada and TRIUMF, Vancouver, Canada. 36 Supported by the Polish State Committee for Scientific Research, grant No. 2P03B09308. 37 Supported by the Polish State Committee for Scientific Research, grant No. 2P03B09208. 38 Now at University of Colorado, USA. 3g Now at High Energy Group of State University of New York, 60 ZEUS Collaboration/Physics Letters B 369 (1996) 55-68