Search for charginos, neutralinos and gravitinos at LEP

An update of the searches for charginos and neutralinos in DELPHI is presented, based mainly on recent data collected at centre-of-mass energies of 161 GeV and 172 GeV. No signal is found. For a sneutrino with mass above 300 GeV/c2 and a mass difference between the chargino and the lightest neutrali...

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Main Authors: Abreu, P, Adam, W, Adye, T, Ajinenko, I, Alekseev, G, Alemany, R, Allport, P, Almehed, S, Amaldi, U, Amato, S, Andersson, P, Andreazza, A, Antilogus, P, Apel, W, Arnoud, Y, Asman, B, Augustin, J, Augustinus, A, Baillon, P, Bambade, P, Barbi, M, Bardin, D, Barker, G, Baroncelli, A, Barring, O
格式: Journal article
语言:English
出版: 1998
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author Abreu, P
Adam, W
Adye, T
Ajinenko, I
Alekseev, G
Alemany, R
Allport, P
Almehed, S
Amaldi, U
Amato, S
Andersson, P
Andreazza, A
Antilogus, P
Apel, W
Arnoud, Y
Asman, B
Augustin, J
Augustinus, A
Baillon, P
Bambade, P
Barbi, M
Bardin, D
Barker, G
Baroncelli, A
Barring, O
author_facet Abreu, P
Adam, W
Adye, T
Ajinenko, I
Alekseev, G
Alemany, R
Allport, P
Almehed, S
Amaldi, U
Amato, S
Andersson, P
Andreazza, A
Antilogus, P
Apel, W
Arnoud, Y
Asman, B
Augustin, J
Augustinus, A
Baillon, P
Bambade, P
Barbi, M
Bardin, D
Barker, G
Baroncelli, A
Barring, O
author_sort Abreu, P
collection OXFORD
description An update of the searches for charginos and neutralinos in DELPHI is presented, based mainly on recent data collected at centre-of-mass energies of 161 GeV and 172 GeV. No signal is found. For a sneutrino with mass above 300 GeV/c2 and a mass difference between the chargino and the lightest neutralino above 10 GeV/c2, the lower limit at 95% confidence level on the chargino mass ranges from 84.3 GeV/c2 to the kinematical limit (86.0 GeV/c2), depending on the mixing parameters. The limit decreases for lower chargino-neutralino mass differences. The limit in the case of a light sneutrino is 67.6 GeV/c2, provided that that there is no light sneutrino with a mass within 10 GeV/c2 below the chargino mass. Upper limits on neutralino pair production cross-sections of about a picobarn are derived. The (μ, M2) domain excluded in the MSSM-GUT scenario is determined by combining the neutralino and chargino searches. These results imply a limit on the mass of the lightest neutralino which, for a heavy sneutrino, is constrained to be above 24.9 GeV/c2 for tanβ ≥ 1. The search has also been extended to the case where the lightest neutralino is unstable and decays into a photon and a gravitino.
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spelling oxford-uuid:3aa894e2-db45-492a-a795-bf63918d95aa2022-03-26T14:02:57ZSearch for charginos, neutralinos and gravitinos at LEPJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:3aa894e2-db45-492a-a795-bf63918d95aaEnglishSymplectic Elements at Oxford1998Abreu, PAdam, WAdye, TAjinenko, IAlekseev, GAlemany, RAllport, PAlmehed, SAmaldi, UAmato, SAndersson, PAndreazza, AAntilogus, PApel, WArnoud, YAsman, BAugustin, JAugustinus, ABaillon, PBambade, PBarbi, MBardin, DBarker, GBaroncelli, ABarring, OAn update of the searches for charginos and neutralinos in DELPHI is presented, based mainly on recent data collected at centre-of-mass energies of 161 GeV and 172 GeV. No signal is found. For a sneutrino with mass above 300 GeV/c2 and a mass difference between the chargino and the lightest neutralino above 10 GeV/c2, the lower limit at 95% confidence level on the chargino mass ranges from 84.3 GeV/c2 to the kinematical limit (86.0 GeV/c2), depending on the mixing parameters. The limit decreases for lower chargino-neutralino mass differences. The limit in the case of a light sneutrino is 67.6 GeV/c2, provided that that there is no light sneutrino with a mass within 10 GeV/c2 below the chargino mass. Upper limits on neutralino pair production cross-sections of about a picobarn are derived. The (μ, M2) domain excluded in the MSSM-GUT scenario is determined by combining the neutralino and chargino searches. These results imply a limit on the mass of the lightest neutralino which, for a heavy sneutrino, is constrained to be above 24.9 GeV/c2 for tanβ ≥ 1. The search has also been extended to the case where the lightest neutralino is unstable and decays into a photon and a gravitino.
spellingShingle Abreu, P
Adam, W
Adye, T
Ajinenko, I
Alekseev, G
Alemany, R
Allport, P
Almehed, S
Amaldi, U
Amato, S
Andersson, P
Andreazza, A
Antilogus, P
Apel, W
Arnoud, Y
Asman, B
Augustin, J
Augustinus, A
Baillon, P
Bambade, P
Barbi, M
Bardin, D
Barker, G
Baroncelli, A
Barring, O
Search for charginos, neutralinos and gravitinos at LEP
title Search for charginos, neutralinos and gravitinos at LEP
title_full Search for charginos, neutralinos and gravitinos at LEP
title_fullStr Search for charginos, neutralinos and gravitinos at LEP
title_full_unstemmed Search for charginos, neutralinos and gravitinos at LEP
title_short Search for charginos, neutralinos and gravitinos at LEP
title_sort search for charginos neutralinos and gravitinos at lep
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