Testing LSND at long-baseline neutrino experiments

Recently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino oscillations. We consider the predictions of this scheme for long...

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Detalles Bibliográficos
Autores principales: Barenboim, Gabriela, Narayan, Mohan, Sankar, S.Uma
Lenguaje:eng
Publicado: 2000
Materias:
Particle Physics - Phenomenology
Acceso en línea:http://cds.cern.ch/record/462724
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author Barenboim, Gabriela
Narayan, Mohan
Sankar, S.Uma
author_facet Barenboim, Gabriela
Narayan, Mohan
Sankar, S.Uma
author_sort Barenboim, Gabriela
collection CERN
description Recently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino oscillations. We consider the predictions of this scheme for long-baseline experiments. We find that high statistics experiments, such as MINOS, can observe a clean signal for this scheme, which is clearly distinguishable from the usual scheme of atmospheric neutrino oscillations driven by a single mass-squared difference.
id cern-462724
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
record_format invenio
spelling cern-4627242023-03-14T20:01:24Zhttp://cds.cern.ch/record/462724engBarenboim, GabrielaNarayan, MohanSankar, S.UmaTesting LSND at long-baseline neutrino experimentsParticle Physics - PhenomenologyRecently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino oscillations. We consider the predictions of this scheme for long-baseline experiments. We find that high statistics experiments, such as MINOS, can observe a clean signal for this scheme, which is clearly distinguishable from the usual scheme of atmospheric neutrino oscillations driven by a single mass-squared difference.Recently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino oscillations. We consider the predictions of this scheme for long-baseline experiments. We find that high statistics experiments, such as MINOS, can observe a clean signal for this scheme, which is clearly distinguishable from the usual scheme of atmospheric neutrino oscillations driven by a single mass-squared difference.hep-ph/0009247CERN-TH-2000-273CERN-TH-2000-273oai:cds.cern.ch:4627242000-09-21
spellingShingle Particle Physics - Phenomenology
Barenboim, Gabriela
Narayan, Mohan
Sankar, S.Uma
Testing LSND at long-baseline neutrino experiments
title Testing LSND at long-baseline neutrino experiments
title_full Testing LSND at long-baseline neutrino experiments
title_fullStr Testing LSND at long-baseline neutrino experiments
title_full_unstemmed Testing LSND at long-baseline neutrino experiments
title_short Testing LSND at long-baseline neutrino experiments
title_sort testing lsnd at long-baseline neutrino experiments
topic Particle Physics - Phenomenology
url http://cds.cern.ch/record/462724
work_keys_str_mv AT barenboimgabriela testinglsndatlongbaselineneutrinoexperiments
AT narayanmohan testinglsndatlongbaselineneutrinoexperiments
AT sankarsuma testinglsndatlongbaselineneutrinoexperiments

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