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About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron
We study the feasibility of a long-baseline neutrino experiment from CERN to Gran Sasso LNGS Laboratories using the CERN PS accelerator. Baseline and neutrino energy spectrum are suitable to explore a region of the Dm2 and sin2(thetat) parameters space which is not reached by K2K, the first experime...
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Lenguaje: | eng |
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1999
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Acceso en línea: | http://cds.cern.ch/record/409307 |
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author | Loverre, P.F. Santacesaria, R. Spada, F.R. |
author_facet | Loverre, P.F. Santacesaria, R. Spada, F.R. |
author_sort | Loverre, P.F. |
collection | CERN |
description | We study the feasibility of a long-baseline neutrino experiment from CERN to Gran Sasso LNGS Laboratories using the CERN PS accelerator. Baseline and neutrino energy spectrum are suitable to explore a region of the Dm2 and sin2(thetat) parameters space which is not reached by K2K, the first experiment that will test at accelerator the atmospheric neutrino anomaly put in evidence by Super Kamiokande |
id | cern-409307 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
spelling | cern-4093072023-03-14T18:59:51Zhttp://cds.cern.ch/record/409307engLoverre, P.F.Santacesaria, R.Spada, F.R.About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton SynchrotronDetectors and Experimental TechniquesWe study the feasibility of a long-baseline neutrino experiment from CERN to Gran Sasso LNGS Laboratories using the CERN PS accelerator. Baseline and neutrino energy spectrum are suitable to explore a region of the Dm2 and sin2(thetat) parameters space which is not reached by K2K, the first experiment that will test at accelerator the atmospheric neutrino anomaly put in evidence by Super KamiokandeWe study the feasibility of a long baseline neutrino experiment from CERN to Gran Sasso LNGS Laboratories using the CERN PS accelerator. Baseline and neutrino energy spectrum are suitable to explore a region of the (Dm2, Sin2(theta)) parameters space which is not reached by K2K, the first experiment that will test at accelerator the atmospheric neutrino anomaly put in evidence by SuperKamiokande.hep-ex/9911043CERN-OPEN-99-347CERN-OPEN-99-347oai:cds.cern.ch:4093071999-07-30 |
spellingShingle | Detectors and Experimental Techniques Loverre, P.F. Santacesaria, R. Spada, F.R. About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title | About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title_full | About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title_fullStr | About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title_full_unstemmed | About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title_short | About testing $\nu_\mu$ oscillation with $\Delta m^2$ smaller than 0.001 $eV^2$ with the CERN Proton Synchrotron |
title_sort | about testing $\nu_\mu$ oscillation with $\delta m^2$ smaller than 0.001 $ev^2$ with the cern proton synchrotron |
topic | Detectors and Experimental Techniques |
url | http://cds.cern.ch/record/409307 |
work_keys_str_mv | AT loverrepf abouttestingnumuoscillationwithdeltam2smallerthan0001ev2withthecernprotonsynchrotron AT santacesariar abouttestingnumuoscillationwithdeltam2smallerthan0001ev2withthecernprotonsynchrotron AT spadafr abouttestingnumuoscillationwithdeltam2smallerthan0001ev2withthecernprotonsynchrotron |