Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments

Detalhes bibliográficos
Autor(a) principal: Minakata, Hisakazu
Data de Publicação: 2003
Outros Autores: Nunokawa, Hiroshi [UNESP], Parke, Stephen
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.68.013010
http://hdl.handle.net/11449/224350
Resumo: We present a general formalism for extracting information on the fundamental parameters associated with neutrino masses and mixings from two or more long baseline neutrino oscillation experiments. This formalism is then applied to the current most likely experiments using neutrino beams from the Japan Hadron Facility (JHF) and Fermilab’s NuMI beamline. Different combinations of muon neutrino or muon anti-neutrino running are considered. The type of neutrino mass hierarchy is extracted using the effects of matter on neutrino propogation. Contrary to naive expectation, we find that both beams using neutrinos is more suitable for determining the hierarchy provided that the neutrino energy divided by baseline [Formula Presented] for NuMI is smaller than or equal to that of JHF, whereas to determine the small mixing angle, [Formula Presented] and the [Formula Presented] or T violating phase [Formula Presented] one neutrino and the other anti-neutrino are most suitable. We make extensive use of bi-probability diagrams for both understanding and extracting the physics involved in such comparisons. © 2003 The American Physical Society.
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spelling Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experimentsWe present a general formalism for extracting information on the fundamental parameters associated with neutrino masses and mixings from two or more long baseline neutrino oscillation experiments. This formalism is then applied to the current most likely experiments using neutrino beams from the Japan Hadron Facility (JHF) and Fermilab’s NuMI beamline. Different combinations of muon neutrino or muon anti-neutrino running are considered. The type of neutrino mass hierarchy is extracted using the effects of matter on neutrino propogation. Contrary to naive expectation, we find that both beams using neutrinos is more suitable for determining the hierarchy provided that the neutrino energy divided by baseline [Formula Presented] for NuMI is smaller than or equal to that of JHF, whereas to determine the small mixing angle, [Formula Presented] and the [Formula Presented] or T violating phase [Formula Presented] one neutrino and the other anti-neutrino are most suitable. We make extensive use of bi-probability diagrams for both understanding and extracting the physics involved in such comparisons. © 2003 The American Physical Society.Department of Physics Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo, 192-0397Instituto de Física Teórica Universidade Estadual Paulista, 01405-900Theoretical Physics Department Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL, 60510Instituto de Física Teórica Universidade Estadual Paulista, 01405-900Tokyo Metropolitan UniversityUniversidade Estadual Paulista (UNESP)Fermi National Accelerator LaboratoryMinakata, HisakazuNunokawa, Hiroshi [UNESP]Parke, Stephen2022-04-28T19:56:04Z2022-04-28T19:56:04Z2003-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.68.013010Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 68, n. 1, 2003.1550-23681550-7998http://hdl.handle.net/11449/22435010.1103/PhysRevD.68.0130102-s2.0-0042387845Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T19:56:04Zoai:repositorio.unesp.br:11449/224350Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:00:10.690387Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
title Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
spellingShingle Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
Minakata, Hisakazu
title_short Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
title_full Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
title_fullStr Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
title_full_unstemmed Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
title_sort Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
author Minakata, Hisakazu
author_facet Minakata, Hisakazu
Nunokawa, Hiroshi [UNESP]
Parke, Stephen
author_role author
author2 Nunokawa, Hiroshi [UNESP]
Parke, Stephen
author2_role author
author
dc.contributor.none.fl_str_mv Tokyo Metropolitan University
Universidade Estadual Paulista (UNESP)
Fermi National Accelerator Laboratory
dc.contributor.author.fl_str_mv Minakata, Hisakazu
Nunokawa, Hiroshi [UNESP]
Parke, Stephen
description We present a general formalism for extracting information on the fundamental parameters associated with neutrino masses and mixings from two or more long baseline neutrino oscillation experiments. This formalism is then applied to the current most likely experiments using neutrino beams from the Japan Hadron Facility (JHF) and Fermilab’s NuMI beamline. Different combinations of muon neutrino or muon anti-neutrino running are considered. The type of neutrino mass hierarchy is extracted using the effects of matter on neutrino propogation. Contrary to naive expectation, we find that both beams using neutrinos is more suitable for determining the hierarchy provided that the neutrino energy divided by baseline [Formula Presented] for NuMI is smaller than or equal to that of JHF, whereas to determine the small mixing angle, [Formula Presented] and the [Formula Presented] or T violating phase [Formula Presented] one neutrino and the other anti-neutrino are most suitable. We make extensive use of bi-probability diagrams for both understanding and extracting the physics involved in such comparisons. © 2003 The American Physical Society.
publishDate 2003
dc.date.none.fl_str_mv 2003-01-01
2022-04-28T19:56:04Z
2022-04-28T19:56:04Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.68.013010
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 68, n. 1, 2003.
1550-2368
1550-7998
http://hdl.handle.net/11449/224350
10.1103/PhysRevD.68.013010
2-s2.0-0042387845
url http://dx.doi.org/10.1103/PhysRevD.68.013010
http://hdl.handle.net/11449/224350
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 68, n. 1, 2003.
1550-2368
1550-7998
10.1103/PhysRevD.68.013010
2-s2.0-0042387845
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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