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Performance of the NOMAD-STAR detector

The NOMAD-STAR detector is a silicon vertex installed in the NOMAD spectrometer at the CERN SPS neutrino beam. It consists of four layers of a passive boron carbide target with a total mass of 45 kg and five layers of 600 single sided silicon microstrip detectors covering a total area of 1.14m^2. Ab...

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Autores principales: Barichello, G, Cervera-Villanueva, A, Daniels, D C, Ellis, M, Ferrère, D, Gouanère, M, Gómez-Cadenas, J J, Gössling, C, Hernando, J A, Huta, W, Kokkonen, J, Kuznetsov, V E, Linssen, Lucie, Lisowski, B, Long, J, Lupi, A, Runólfsson, O, Schmidt, B, Soler, F J P, Steele, D, Stipcevic, M, Veltri, M, Vidal-Sitjes, G, do Couto e Silva, E
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0168-9002(03)01379-2
http://cds.cern.ch/record/624431
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author Barichello, G
Cervera-Villanueva, A
Daniels, D C
Ellis, M
Ferrère, D
Gouanère, M
Gómez-Cadenas, J J
Gössling, C
Hernando, J A
Huta, W
Kokkonen, J
Kuznetsov, V E
Linssen, Lucie
Lisowski, B
Long, J
Lupi, A
Runólfsson, O
Schmidt, B
Soler, F J P
Steele, D
Stipcevic, M
Veltri, M
Vidal-Sitjes, G
do Couto e Silva, E
author_facet Barichello, G
Cervera-Villanueva, A
Daniels, D C
Ellis, M
Ferrère, D
Gouanère, M
Gómez-Cadenas, J J
Gössling, C
Hernando, J A
Huta, W
Kokkonen, J
Kuznetsov, V E
Linssen, Lucie
Lisowski, B
Long, J
Lupi, A
Runólfsson, O
Schmidt, B
Soler, F J P
Steele, D
Stipcevic, M
Veltri, M
Vidal-Sitjes, G
do Couto e Silva, E
author_sort Barichello, G
collection CERN
description The NOMAD-STAR detector is a silicon vertex installed in the NOMAD spectrometer at the CERN SPS neutrino beam. It consists of four layers of a passive boron carbide target with a total mass of 45 kg and five layers of 600 single sided silicon microstrip detectors covering a total area of 1.14m^2. About 11,500 nu_mu charged current interactions were reconstructed in the fiducial volume of NOMAD-STAR from the neutrino run in 1998. The potential use of silicon detectors for nu_mu (nu_e)<-> nu_tau oscillations depends on the observation of the tau candidates by the experimental signature of a large impact parameter, in the case of the one prong decay of the tau, or a double vertex, in the case of the three prong decay. The main aim of NOMAD-STAR is to measure the impact parameter and vertex distributions of charged current interactions, which constitute the main backgrounds for the oscillation signals, to understand the significance of a potential signal in a future experiment. The present paper describes the experience gained in the operation of this silicon vertex detector, and the peformance achieved with it. PACS : 13.15.+g; 14.60.Lm; 14.60.Pq; 29.40Gx; 29.40.Wk Keywords Neutrino physics; Silicon microstrip detectors
id cern-624431
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
record_format invenio
spelling cern-6244312019-09-30T06:29:59Zdoi:10.1016/S0168-9002(03)01379-2http://cds.cern.ch/record/624431engBarichello, GCervera-Villanueva, ADaniels, D CEllis, MFerrère, DGouanère, MGómez-Cadenas, J JGössling, CHernando, J AHuta, WKokkonen, JKuznetsov, V ELinssen, LucieLisowski, BLong, JLupi, ARunólfsson, OSchmidt, BSoler, F J PSteele, DStipcevic, MVeltri, MVidal-Sitjes, Gdo Couto e Silva, EPerformance of the NOMAD-STAR detectorDetectors and Experimental TechniquesThe NOMAD-STAR detector is a silicon vertex installed in the NOMAD spectrometer at the CERN SPS neutrino beam. It consists of four layers of a passive boron carbide target with a total mass of 45 kg and five layers of 600 single sided silicon microstrip detectors covering a total area of 1.14m^2. About 11,500 nu_mu charged current interactions were reconstructed in the fiducial volume of NOMAD-STAR from the neutrino run in 1998. The potential use of silicon detectors for nu_mu (nu_e)<-> nu_tau oscillations depends on the observation of the tau candidates by the experimental signature of a large impact parameter, in the case of the one prong decay of the tau, or a double vertex, in the case of the three prong decay. The main aim of NOMAD-STAR is to measure the impact parameter and vertex distributions of charged current interactions, which constitute the main backgrounds for the oscillation signals, to understand the significance of a potential signal in a future experiment. The present paper describes the experience gained in the operation of this silicon vertex detector, and the peformance achieved with it. PACS : 13.15.+g; 14.60.Lm; 14.60.Pq; 29.40Gx; 29.40.Wk Keywords Neutrino physics; Silicon microstrip detectorsCERN-EP-2003-017oai:cds.cern.ch:6244312003-03-31
spellingShingle Detectors and Experimental Techniques
Barichello, G
Cervera-Villanueva, A
Daniels, D C
Ellis, M
Ferrère, D
Gouanère, M
Gómez-Cadenas, J J
Gössling, C
Hernando, J A
Huta, W
Kokkonen, J
Kuznetsov, V E
Linssen, Lucie
Lisowski, B
Long, J
Lupi, A
Runólfsson, O
Schmidt, B
Soler, F J P
Steele, D
Stipcevic, M
Veltri, M
Vidal-Sitjes, G
do Couto e Silva, E
Performance of the NOMAD-STAR detector
title Performance of the NOMAD-STAR detector
title_full Performance of the NOMAD-STAR detector
title_fullStr Performance of the NOMAD-STAR detector
title_full_unstemmed Performance of the NOMAD-STAR detector
title_short Performance of the NOMAD-STAR detector
title_sort performance of the nomad-star detector
topic Detectors and Experimental Techniques
url https://dx.doi.org/10.1016/S0168-9002(03)01379-2
http://cds.cern.ch/record/624431
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