Search for anomalous photonic events with missing energy in e+e- collisions at √s = 130, 136 and 183 GeV

被引:39
作者
Abbiendi, G [1 ]
Ackerstaff, K
Alexander, G
Allison, J
Altekamp, N
Anderson, KJ
Anderson, S
Arcelli, S
Asai, S
Ashby, SF
Axen, D
Azuelos, G
Ball, AH
Barberio, E
Barlow, RJ
Bartoldus, R
Batley, JR
Baumann, S
Bechtluft, J
Behnke, T
Bell, KW
Bella, G
Bellerive, A
Bentvelsen, S
Bethke, S
Betts, S
Biebel, O
Biguzzi, A
Bird, SD
Blobel, V
Bloodworth, IJ
Bobinski, M
Bock, P
Böhme, J
Bonacorsi, D
Boutemeur, M
Braibant, S
Bright-Thomas, P
Brigliadori, L
Brown, RM
Burckhart, HJ
Burgard, C
Bürgin, R
Capiluppi, P
Carnegie, RK
Carter, AA
Carter, JR
Chang, CY
Charlton, DG
Chrisman, D
机构
[1] Univ Bologna, Dipartimento Fis, I-40126 Bologna, Italy
[2] Ist Nazl Fis Nucl, I-40126 Bologna, Italy
[3] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[4] Univ Bonn, Inst Phys, D-53115 Bonn, Germany
[5] Univ Calif Riverside, Dept Phys, Riverside, CA 92521 USA
[6] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England
[7] Carleton Univ, Ottawa Carleton Inst Phys, Dept Phys, Ottawa, ON K1S 5B6, Canada
[8] Carleton Univ, Ctr Res Particle Phys, Ottawa, ON K1S 5B6, Canada
[9] CERN, European Org Particle Phys, CH-1211 Geneva 23, Switzerland
[10] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[11] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[12] Univ Freiburg, Fak Phys, D-79104 Freiburg, Germany
[13] Univ Heidelberg, Inst Phys, D-69120 Heidelberg, Germany
[14] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
[15] Queen Mary Univ London, London E1 4NS, England
[16] Rhein Westfal TH Aachen, Inst Phys 3, D-52056 Aachen, Germany
[17] Univ London Univ Coll, London WC1E 6BT, England
[18] Univ Manchester, Schuster Lab, Dept Phys, Manchester M13 9PL, Lancs, England
[19] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[20] Univ Montreal, Phys Nucl Lab, Montreal, PQ H3C 3J7, Canada
[21] Univ Oregon, Dept Phys, Eugene, OR 97403 USA
[22] CLRC, Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[23] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel
[24] Tel Aviv Univ, Dept Phys & Astron, IL-69978 Tel Aviv, Israel
[25] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo 1130033, Japan
[26] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[27] Kobe Univ, Kobe, Hyogo 6578501, Japan
[28] Brunel Univ, Inst Phys & Environm Sci, Uxbridge UB8 3PH, Middx, England
[29] Weizmann Inst Sci, Particle Phys Dept, IL-76100 Rehovot, Israel
[30] Univ Hamburg, DESY, Inst Expt Phys 2, D-22607 Hamburg, Germany
[31] Univ Victoria, Dept Phys, Victoria, BC V8W 3P6, Canada
[32] Univ British Columbia, Dept Phys, Vancouver, BC V6T 1Z1, Canada
[33] Univ Alberta, Dept Phys, Edmonton, AB T6G 2J1, Canada
[34] Duke Univ, Dept Phys, Durham, NC 27708 USA
[35] Res Inst Particle & Nucl Phys, H-1525 Budapest, Hungary
[36] Inst Nucl Res, H-4001 Debrecen, Hungary
[37] Univ Munich, Sekt Phys, D-85748 Garching, Germany
[38] TRIUMF, Vancouver, BC V6T 2A3, Canada
[39] Nucl Res Inst, Debrecen, Hungary
[40] Lajos Kossuth Univ, Dept Expt Phys, Debrecen, Hungary
来源
EUROPEAN PHYSICAL JOURNAL C | 1999年 / 8卷 / 01期
关键词
D O I
10.1007/s100520050442
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Photonic events with large missing energy have been observed in e(+)e(-) collisions at centre-of-mass energies of 130, 136 and 183 GeV collected in 1997 using the OPAL detector at LEP. Results are presented for event topologies with a single photon and missing transverse energy or with an acoplanar photon pair. Cross-section measurements are performed within the kinematic acceptance of each selection. These results are compared with the expectations from the Standard Model process e(+)e(-) --> v (v) over bar + photon(s). No evidence is observed for new physics contributions to these final states. Using the data at root s = 183 GeV, upper limits on sigma(e(+)e(-) --> XY) BR(X --> Y gamma) and sigma(e(+)e(-) --> XX) BR2 (X --> Y gamma) are derived for the case of stable and invisible Y. These limits apply to single and pair production of excited neutrinos (X = nu*,Y = nu), to neutralino production (X = <(chi)over tilde>(0)(2), Y = <(chi)over tilde>(0)(1)) and to supersymmetric models in which X = <(chi)over tilde>(0)(1) and Y = (G) over bar is a light gravitino.
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页码:23 / 40
页数:18
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