Mixed states for mixing neutrinos
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | |
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 |
|
_version_ |
1808128332011667456 |