Mixed states for mixing neutrinos

Detalhes bibliográficos
Autor(a) principal: Cozzella, Gabriel [UNESP]
Data de Publicação: 2018
Outros Autores: Giunti, Carlo
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.98.096010
http://hdl.handle.net/11449/228638
Resumo: Here we discuss the description of flavor neutrinos produced or detected in processes which involve more than one neutrino. We show that in these cases flavor neutrinos cannot be separately described by pure states, but require a density matrix description. We consider explicitly the examples of νe and νμ production in μ+ decay and νμ detection through scattering on electrons. We show that the density matrix which describes a flavor neutrino can be approximated with a density matrix of a pure state only when the differences of the neutrino masses are neglected in the interaction process. In this approximation, the pure states are the standard flavor states and one recovers the standard expression for the neutrino oscillation probability. We discuss also the effects of mixing of the three standard light neutrinos with heavy neutrinos which can be either decoupled because their masses are much larger than the maximum neutrino energy in the neutrino production process or because they are produced and detected incoherently. Finally, we discuss the more complicated case of neutrino-electron elastic scattering, in which the initial and final neutrinos do not have determined flavors, but there is a flavor dependence due to the different contributions of charged-current and neutral-current interactions.
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spelling Mixed states for mixing neutrinosHere we discuss the description of flavor neutrinos produced or detected in processes which involve more than one neutrino. We show that in these cases flavor neutrinos cannot be separately described by pure states, but require a density matrix description. We consider explicitly the examples of νe and νμ production in μ+ decay and νμ detection through scattering on electrons. We show that the density matrix which describes a flavor neutrino can be approximated with a density matrix of a pure state only when the differences of the neutrino masses are neglected in the interaction process. In this approximation, the pure states are the standard flavor states and one recovers the standard expression for the neutrino oscillation probability. We discuss also the effects of mixing of the three standard light neutrinos with heavy neutrinos which can be either decoupled because their masses are much larger than the maximum neutrino energy in the neutrino production process or because they are produced and detected incoherently. Finally, we discuss the more complicated case of neutrino-electron elastic scattering, in which the initial and final neutrinos do not have determined flavors, but there is a flavor dependence due to the different contributions of charged-current and neutral-current interactions.Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz, 271INFN Sezione di Torino, Via P. Giuria 1Instituto de Física Teórica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz, 271Universidade Estadual Paulista (UNESP)Sezione di TorinoCozzella, Gabriel [UNESP]Giunti, Carlo2022-04-29T08:27:52Z2022-04-29T08:27:52Z2018-11-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.98.096010Physical Review D, v. 98, n. 9, 2018.2470-00292470-0010http://hdl.handle.net/11449/22863810.1103/PhysRevD.98.0960102-s2.0-85058084828Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:27:52Zoai:repositorio.unesp.br:11449/228638Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:12:14.943787Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Mixed states for mixing neutrinos
title Mixed states for mixing neutrinos
spellingShingle Mixed states for mixing neutrinos
Cozzella, Gabriel [UNESP]
title_short Mixed states for mixing neutrinos
title_full Mixed states for mixing neutrinos
title_fullStr Mixed states for mixing neutrinos
title_full_unstemmed Mixed states for mixing neutrinos
title_sort Mixed states for mixing neutrinos
author Cozzella, Gabriel [UNESP]
author_facet Cozzella, Gabriel [UNESP]
Giunti, Carlo
author_role author
author2 Giunti, Carlo
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Sezione di Torino
dc.contributor.author.fl_str_mv Cozzella, Gabriel [UNESP]
Giunti, Carlo
description Here we discuss the description of flavor neutrinos produced or detected in processes which involve more than one neutrino. We show that in these cases flavor neutrinos cannot be separately described by pure states, but require a density matrix description. We consider explicitly the examples of νe and νμ production in μ+ decay and νμ detection through scattering on electrons. We show that the density matrix which describes a flavor neutrino can be approximated with a density matrix of a pure state only when the differences of the neutrino masses are neglected in the interaction process. In this approximation, the pure states are the standard flavor states and one recovers the standard expression for the neutrino oscillation probability. We discuss also the effects of mixing of the three standard light neutrinos with heavy neutrinos which can be either decoupled because their masses are much larger than the maximum neutrino energy in the neutrino production process or because they are produced and detected incoherently. Finally, we discuss the more complicated case of neutrino-electron elastic scattering, in which the initial and final neutrinos do not have determined flavors, but there is a flavor dependence due to the different contributions of charged-current and neutral-current interactions.
publishDate 2018
dc.date.none.fl_str_mv 2018-11-01
2022-04-29T08:27:52Z
2022-04-29T08:27:52Z
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.98.096010
Physical Review D, v. 98, n. 9, 2018.
2470-0029
2470-0010
http://hdl.handle.net/11449/228638
10.1103/PhysRevD.98.096010
2-s2.0-85058084828
url http://dx.doi.org/10.1103/PhysRevD.98.096010
http://hdl.handle.net/11449/228638
identifier_str_mv Physical Review D, v. 98, n. 9, 2018.
2470-0029
2470-0010
10.1103/PhysRevD.98.096010
2-s2.0-85058084828
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
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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