Complementarity of eastern and western hemisphere long-baseline neutrino oscillation experiments
Autor(a) principal: | |
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Data de Publicação: | 2003 |
Outros Autores: | , |
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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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 |
|
_version_ |
1808128302764785664 |