Single-and multi-photon production in e+e- collisions at a centre-of-mass energy of 183 GeV

被引:59
作者
Barate, R [1 ]
Buskulic, D
Decamp, D
Ghez, P
Goy, C
Jezequel, S
Lees, JP
Lucotte, A
Martin, F
Merle, E
Minard, MN
Nief, JY
Pietrzyk, B
Alemany, R
Boix, G
Casado, MP
Chmeissani, M
Crespo, JM
Delfino, M
Fernandez, E
Fernandez-Bosman, M
Garrido, L
Grauges, E
Juste, A
Martinez, M
Merino, G
Miquel, R
Mir, LM
Morawitz, P
Park, IC
Pascual, A
Perlas, JA
Riu, I
Sanchez, F
Colaleo, A
Creanza,D
de Palma, M
Gelao, G
Iaselli, G
Maggi, G
Maggi, M
Nuzzo, S
Ranieri, A
Raso, G
Ruggieri, F
Selvaggi, G
Silvestris, L
Tempesta, P
Tricomi, A
Zito, G
机构
[1] IN2P3, Lab Phys Particules LAPP, CNRS, F-74019 Annecy Le Vieux, France
[2] Univ Autonoma Barcelona, Inst Fis Altes Energies, E-08193 Bellaterra, Barcelona, Spain
[3] Ist Nazl Fis Nucl, Dipartimento Fis, Sezione Bari, I-70126 Bari, Italy
[4] Acad Sinica, Inst High Energy Phys, Beijing, Peoples R China
[5] CERN, European Lab Particle Phys, CH-1211 Geneva 23, Switzerland
[6] Univ Blaise Pascal, Phys Corpusculaire Lab, IN2P3, CNRS, F-63177 Clermont Ferrand, France
[7] Niels Bohr Inst, DK-2100 Copenhagen, Denmark
[8] Nucl Res Ctr Demokritos NRCD, GR-15310 Attiki, Greece
[9] Ecole Polytech, Phys Theor & Hautes Energies Lab, IN2P3, CNRS, F-91128 Palaiseau, France
[10] Univ Florence, Dipartimento Fis, INFN, Sezione Firenze, I-50125 Florence, Italy
[11] Florida State Univ, Supercomp Computat Res Inst, Tallahassee, FL 32306 USA
[12] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[13] Univ Glasgow, Dept Phys & Astron, Glasgow G12 8QQ, Lanark, Scotland
[14] Heidelberg Univ, Inst Hochenergiephys, D-69120 Heidelberg, Germany
[15] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London SW7 2BZ, England
[16] Univ Innsbruck, Inst Expt Phys, A-6020 Innsbruck, Austria
[17] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
[18] Johannes Gutenberg Univ Mainz, Inst Phys, D-55099 Mainz, Germany
[19] Fac Sci Luminy, Ctr Phys Particules, IN2P3, CNRS, F-13288 Marseille, France
[20] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy
[21] Ist Nazl Fis Nucl, Sezione Milano, I-20133 Milan, Italy
[22] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany
[23] Univ Paris 11, Lab Accelerateur Lineaire, IN2P3, CNRS, F-91405 Orsay, France
[24] Ist Nazl Fis Nucl, Sezione Pisa, I-56010 Pisa, Italy
[25] Univ Pisa, Dipartimento Fis, I-56010 Pisa, Italy
[26] Scuola Normale Super Pisa, I-56010 Pisa, Italy
[27] Univ London Royal Holloway & Bedford New Coll, Dept Phys, Egham TW20 0EX, Surrey, England
[28] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England
[29] CENS, CEA, DAPNIA, Serv Phys Particules, F-91191 Gif Sur Yvette, France
[30] Univ Calif Santa Cruz, Inst Particle Phys, Santa Cruz, CA 95064 USA
[31] Univ Sheffield, Dept Phys, Sheffield S3 7RH, S Yorkshire, England
[32] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany
[33] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy
[34] Ist Nazl Fis Nucl, Sezione Trieste, I-34127 Trieste, Italy
[35] Univ Washington, Seattle, WA 98195 USA
[36] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[37] Univ Barcelona, Barcelona 08208, Spain
[38] Ist Nazl Fis Nucl, Dipartimento Fis, Sezione Catania, I-95129 Catania, Italy
[39] Univ Turin, Ist Fis Gen, Turin, Italy
[40] CNR, Ist Cosmogeofis, I-10126 Turin, Italy
[41] CERN, CH-1211 Geneva 23, Switzerland
[42] Kangnung Natl Univ, Kangnung, South Korea
关键词
D O I
10.1016/S0370-2693(98)00468-7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The production of final states involving one or more energetic photons from e(+)e(-) collisions is studied in a sample of 58.5 pb(-1) of data recorded at a centre-of-mass energy of 183 GeV by the ALEPH detector at LEP. The e(+)e(-) --> v (v) over bar gamma(gamma) and e(+)e(-) --> gamma gamma(gamma) cross sections are measured. The data are in good agreement with predictions based on the Standard Model and are used to set upper limits on the cross sections for anomalous photon production in the context of two supersymmetric models and for various extensions to QED. In particular, in the context of a super-light gravitino model a cross section upper limit of 0.38 pb is placed on the process e(+)e(-) --> (G) over tilde (G) over tilde gamma, allowing a lower limit to be set on the mass of the gravitino. Limits are also set on the mass of the lightest neutralino in Gauge Mediated Supersymmetry Breaking models. In the case of equal ee *gamma and ee gamma couplings a 95% C.L. lower limit on M-e* of 250 GeV/c(2) is obtained. (C) 1998 Published by Elsevier Science B.V. All rights reserved.
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收藏
页码:201 / 214
页数:14
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