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Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV
A spin-parity 1/sup +/ rho pi enhancement is observed for the 3 pi mass spectrum in the reaction K/sup -/p to Sigma /sup -/ pi /sup +/ pi /sup +/ pi /sup -/ where events with a small (K/sup -/ to Sigma /sup - /) momentum transfer are selected. The mass (1040 MeV) and width (230 MeV) of this enhancem...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
1977
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(77)90148-4 http://cds.cern.ch/record/878579 |
_version_ | 1780908000738803712 |
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author | Gavillet, P Bergé, P Blokzijl, R De van de Walle, R Engeler, J Ferrando, A Foster, B Grossman, P Hemingway, R J Holmgren, S O Jongejans, B Kittel, E W Kluyver, J C Lamb, P Losty, Michael J Marin, J C Massaro, G G G McDowell, W L Montanet, Lucien Pagiola, E Vergeest, J Yamdagni, N |
author_facet | Gavillet, P Bergé, P Blokzijl, R De van de Walle, R Engeler, J Ferrando, A Foster, B Grossman, P Hemingway, R J Holmgren, S O Jongejans, B Kittel, E W Kluyver, J C Lamb, P Losty, Michael J Marin, J C Massaro, G G G McDowell, W L Montanet, Lucien Pagiola, E Vergeest, J Yamdagni, N |
author_sort | Gavillet, P |
collection | CERN |
description | A spin-parity 1/sup +/ rho pi enhancement is observed for the 3 pi mass spectrum in the reaction K/sup -/p to Sigma /sup -/ pi /sup +/ pi /sup +/ pi /sup -/ where events with a small (K/sup -/ to Sigma /sup - /) momentum transfer are selected. The mass (1040 MeV) and width (230 MeV) of this enhancement are reminiscent of the A/sub 1/ to rho pi bump which has mainly been observed in the diffractive-like processes. The cross section for this enhancement at 4.15 GeV/c incident K/sup -/ momentum is (3.6+or-0.5) mu b. (16 refs). |
id | cern-878579 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1977 |
record_format | invenio |
spelling | cern-8785792019-09-30T06:29:59Zdoi:10.1016/0370-2693(77)90148-4http://cds.cern.ch/record/878579engGavillet, PBergé, PBlokzijl, RDe van de Walle, REngeler, JFerrando, AFoster, BGrossman, PHemingway, R JHolmgren, S OJongejans, BKittel, E WKluyver, J CLamb, PLosty, Michael JMarin, J CMassaro, G G GMcDowell, W LMontanet, LucienPagiola, EVergeest, JYamdagni, NBackward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeVParticle Physics - PhenomenologyA spin-parity 1/sup +/ rho pi enhancement is observed for the 3 pi mass spectrum in the reaction K/sup -/p to Sigma /sup -/ pi /sup +/ pi /sup +/ pi /sup -/ where events with a small (K/sup -/ to Sigma /sup - /) momentum transfer are selected. The mass (1040 MeV) and width (230 MeV) of this enhancement are reminiscent of the A/sub 1/ to rho pi bump which has mainly been observed in the diffractive-like processes. The cross section for this enhancement at 4.15 GeV/c incident K/sup -/ momentum is (3.6+or-0.5) mu b. (16 refs).oai:cds.cern.ch:8785791977 |
spellingShingle | Particle Physics - Phenomenology Gavillet, P Bergé, P Blokzijl, R De van de Walle, R Engeler, J Ferrando, A Foster, B Grossman, P Hemingway, R J Holmgren, S O Jongejans, B Kittel, E W Kluyver, J C Lamb, P Losty, Michael J Marin, J C Massaro, G G G McDowell, W L Montanet, Lucien Pagiola, E Vergeest, J Yamdagni, N Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title | Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title_full | Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title_fullStr | Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title_full_unstemmed | Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title_short | Backward production of a spin parity 1/sup +/ rho pi enhancement at 104 GeV |
title_sort | backward production of a spin parity 1/sup +/ rho pi enhancement at 104 gev |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/0370-2693(77)90148-4 http://cds.cern.ch/record/878579 |
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