論文

1996年6月

Search for chargino and neutralino production using the OPAL detector at root s=130-136GeV at LEP

PHYSICS LETTERS B
  • G Alexander
  • J Allison
  • N Altekamp
  • K Ametewee
  • KJ Anderson
  • S Anderson
  • S Arcelli
  • S Asai
  • D Axen
  • G Azuelos
  • AH Ball
  • E Barberio
  • RJ Barlow
  • R Bartoldus
  • Batley, JR
  • G Beaudoin
  • J Bechtluft
  • C Beeston
  • T Behnke
  • AN Bell
  • KW Bell
  • G Bella
  • S Bentvelsen
  • P Berlich
  • S Bethke
  • O Biebel
  • Blobel, V
  • IJ Bloodworth
  • JE Bloomer
  • P Bock
  • HM Bosch
  • M Boutemeur
  • BT Bouwens
  • S Braibant
  • RM Brown
  • HJ Burckhart
  • C Burgard
  • R Burgin
  • P Capiluppi
  • RK Carnegie
  • AA Carter
  • Carter, JR
  • CY Chang
  • C Charlesworth
  • DG Charlton
  • D Chrisman
  • SL Chu
  • PEL Clarke
  • Cohen, I
  • JE Conboy
  • OC Cooke
  • M Cuffiani
  • S Dado
  • C Dallapiccola
  • GM Dallavalle
  • C Darling
  • S DeJong
  • LA delPozo
  • MS Dixit
  • ED Silva
  • E Duchovni
  • G Duckeck
  • IP Duerdoth
  • JEG Edwards
  • PG Estabrooks
  • HG Evans
  • M Evans
  • F Fabbri
  • P Fath
  • F Fiedler
  • M Fierro
  • HM Fischer
  • R Folman
  • DG Fong
  • M Foucher
  • H Fukui
  • A Furtjes
  • P Gagnon
  • A Gaidot
  • JW Gary
  • J Gascon
  • SM GasconShotkin
  • NI Geddes
  • C GeichGimbel
  • SW Gensler
  • FX Gentit
  • T Geralis
  • G Giacomelli
  • P Giacomelli
  • R Giacomelli
  • Gibson, V
  • WR Gibson
  • DM Gingrich
  • J Goldberg
  • MJ Goodrick
  • W Gorn
  • C Grandi
  • E Gross
  • M Gruwe
  • C Hajdu
  • GG Hanson
  • M Hansroul
  • M Hapke
  • CK Hargrove
  • PA Hart
  • C Hartmann
  • M Hauschild
  • CM Hawkes
  • R Hawkings
  • RJ Hemingway
  • G Herten
  • RD Heuer
  • MD Hildreth
  • JC Hill
  • SJ Hillier
  • T Hilse
  • PR Hobson
  • RJ Homer
  • AK Honma
  • D Horvath
  • R Howard
  • RE HughesJones
  • DE Hutchcroft
  • P IgoKemenes
  • DC Imrie
  • MR Ingram
  • A Jawahery
  • PW Jeffreys
  • H Jeremie
  • M Jimack
  • A Joly
  • G Jones
  • M Jones
  • RWL Jones
  • U Jost
  • P Jovanovic
  • J Kanzaki
  • D Karlen
  • T Kawamoto
  • RK Keeler
  • RG Kellogg
  • BW Kennedy
  • J King
  • J Kirk
  • S Kluth
  • T Kobayashi
  • M Kobel
  • DS Koetke
  • TP Kokott
  • S Komamiya
  • R Kowalewski
  • T Kress
  • P Krieger
  • J vonKrogh
  • P Kyberd
  • GD Lafferty
  • H Lafoux
  • R Lahmann
  • WP Lai
  • D Lanske
  • J Lauber
  • JG Layter
  • AM Lee
  • E Lefebvre
  • D Lellouch
  • J Letts
  • L Levinson
  • C Lewis
  • SL Lloyd
  • FK Loebinger
  • GD Long
  • B Lorazo
  • MJ Losty
  • J Ludwig
  • A Luig
  • A Malik
  • M Mannelli
  • S Marcellini
  • C Markus
  • AJ Martin
  • JP Martin
  • G Martinez
  • T Mashimo
  • W Matthews
  • P Mattig
  • WJ McDonald
  • J McKenna
  • EA Mckigney
  • TJ McMahon
  • AI McNab
  • F Meijers
  • S Menke
  • FS Merritt
  • H Mes
  • J Meyer
  • A Michelini
  • G Mikenberg
  • B Miller
  • R Mir
  • W Mohr
  • A Montanari
  • T Mori
  • M Morii
  • U Muller
  • B Nellen
  • B Nijjhar
  • R Nisius
  • SW ONeale
  • FG Oakham
  • F Odorici
  • HO Ogren
  • T Omori
  • MJ Oreglia
  • S Orito
  • M Palazzo
  • J Palinkas
  • FM Palmonari
  • JP Pansart
  • G Pasztor
  • Pater, JR
  • GN Patrick
  • MJ Pearce
  • S Petzold
  • JE Pilcher
  • J Pinfold
  • DE Plane
  • P Poffenberger
  • B Poli
  • A Posthaus
  • H Przysiezniak
  • DL Rees
  • D Rigby
  • MG Rison
  • SA Robins
  • N Rodning
  • JM Roney
  • A Rooke
  • E Ros
  • AM Rossi
  • M Rosvick
  • P Routenburg
  • Y Rozen
  • K Runge
  • O Runolfsson
  • DR Rust
  • R Rylko
  • EKG Sarkisyan
  • M Sasaki
  • C Sbarra
  • AD Schaile
  • O Schaile
  • F Scharf
  • P ScharffHansen
  • P Schenk
  • B Schmitt
  • M Schroder
  • HC SchultzCoulon
  • M Schulz
  • P Schutz
  • J Schwiening
  • WG Scott
  • TG Shears
  • BC Shen
  • CH ShepherdThemistocleous
  • P Sherwood
  • GP Siroli
  • A Sittler
  • A Skillman
  • A Skuja
  • AM Smith
  • TJ Smith
  • GA Snow
  • R Sobie
  • S SoldnerRembold
  • RW Springer
  • M Sproston
  • A Stahl
  • M Starks
  • K Stephens
  • J Steuerer
  • B Stockhausen
  • D Strom
  • F Strumia
  • P Szymanski
  • R Tafirout
  • H Takeda
  • P Taras
  • S Tarem
  • M Tecchio
  • N Tesch
  • M Thiergen
  • MA Thomson
  • E vonTorne
  • S Towers
  • M Tscheulin
  • E Tsur
  • AS Turcot
  • MF TurnerWatson
  • P Utzat
  • R VanKooten
  • G Vasseur
  • M Verzocchi
  • P Vikas
  • M Vincter
  • EH Vokurka
  • F Wackerle
  • A Wagner
  • CP Ward
  • DR Ward
  • JJ Ward
  • PM Watkins
  • AT Watson
  • NK Watson
  • P Weber
  • PS Wells
  • N Wermes
  • JS White
  • B Wilkens
  • GW Wilson
  • JA Wilson
  • T Wlodek
  • G Wolf
  • S Wotton
  • TR Wyatt
  • S Xella
  • S Yamashita
  • G Yekutieli
  • K Yoshimura
  • Zacek, V
  • 全て表示

377
1-3
開始ページ
181
終了ページ
194
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/0370-2693(96)00301-2
出版者・発行元
ELSEVIER SCIENCE BV

A search for charginos and neutralinos, predicted by supersymmetric theories, has been performed using a data sample of 2.6 pb(-1) at a centre-of-mass energy of root s = 130 GeV and 2.6 pb(-1) at 136 GeV collected with the OPAL detector at LEP during November 1995. No candidate events were observed. The 95% C.L. lower limit on the lightest chargino mass in the Minimal Supersymmetric Standard Model is 65.4 GeV if the universal scalar mass m(o) is greater than 1 TeV, and 58.7 GeV for the smallest m(o) compatible with slepton and sneutrino mass limits obtained at centre-of-mass energies near the Z peak. These limits were obtained under the conditions that the lightest chargino is heavier than the lightest neutralino by more than 10 GeV and tan beta is larger than 1.5. The results of a model independent search for charginos and neutralinos are also given.

リンク情報
DOI
https://doi.org/10.1016/0370-2693(96)00301-2
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:A1996UT14800029&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/0370-2693(96)00301-2
  • ISSN : 0370-2693
  • Web of Science ID : WOS:A1996UT14800029

エクスポート
BibTeX RIS