Bounds on the tau and muon neutrino vector and axial vector charge radius

ABSTRACT: Experimental evidence for neutrino oscillations implies that neutrinos are the first elementary particles whose properties cannot be fully described within the standard model. This hints at the possibility that other properties of these intriguing particles might substantially deviate from...

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Autores:
Hirsch, Martin
Nardi, Enrico
Restrepo Quintero, Diego Alejandro
Tipo de recurso:
Article of investigation
Fecha de publicación:
2003
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/8295
Acceso en línea:
http://hdl.handle.net/10495/8295
Palabra clave:
Partículas elementales
Elementary Particles
Astrofísica
Astrophysics
Neutrinos
Neutrines
Cosmología
Cosmology
Vectores
Vectors
Electromagnética
http://aims.fao.org/aos/agrovoc/c_8164
http://vocabularies.unesco.org/thesaurus/concept3218
Rights
openAccess
License
http://creativecommons.org/licenses/by-nc-nd/2.5/co/
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network_acronym_str UDEA2
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dc.title.spa.fl_str_mv Bounds on the tau and muon neutrino vector and axial vector charge radius
title Bounds on the tau and muon neutrino vector and axial vector charge radius
spellingShingle Bounds on the tau and muon neutrino vector and axial vector charge radius
Partículas elementales
Elementary Particles
Astrofísica
Astrophysics
Neutrinos
Neutrines
Cosmología
Cosmology
Vectores
Vectors
Electromagnética
http://aims.fao.org/aos/agrovoc/c_8164
http://vocabularies.unesco.org/thesaurus/concept3218
title_short Bounds on the tau and muon neutrino vector and axial vector charge radius
title_full Bounds on the tau and muon neutrino vector and axial vector charge radius
title_fullStr Bounds on the tau and muon neutrino vector and axial vector charge radius
title_full_unstemmed Bounds on the tau and muon neutrino vector and axial vector charge radius
title_sort Bounds on the tau and muon neutrino vector and axial vector charge radius
dc.creator.fl_str_mv Hirsch, Martin
Nardi, Enrico
Restrepo Quintero, Diego Alejandro
dc.contributor.author.none.fl_str_mv Hirsch, Martin
Nardi, Enrico
Restrepo Quintero, Diego Alejandro
dc.contributor.researchgroup.spa.fl_str_mv Grupo de Fenomenologia de Interacciones Fundamentales
dc.subject.decs.none.fl_str_mv Partículas elementales
Elementary Particles
topic Partículas elementales
Elementary Particles
Astrofísica
Astrophysics
Neutrinos
Neutrines
Cosmología
Cosmology
Vectores
Vectors
Electromagnética
http://aims.fao.org/aos/agrovoc/c_8164
http://vocabularies.unesco.org/thesaurus/concept3218
dc.subject.unesco.none.fl_str_mv Astrofísica
Astrophysics
dc.subject.lemb.none.fl_str_mv Neutrinos
Neutrines
Cosmología
Cosmology
dc.subject.agrovoc.none.fl_str_mv Vectores
Vectors
dc.subject.proposal.spa.fl_str_mv Electromagnética
dc.subject.agrovocuri.none.fl_str_mv http://aims.fao.org/aos/agrovoc/c_8164
http://vocabularies.unesco.org/thesaurus/concept3218
description ABSTRACT: Experimental evidence for neutrino oscillations implies that neutrinos are the first elementary particles whose properties cannot be fully described within the standard model. This hints at the possibility that other properties of these intriguing particles might substantially deviate from the predictions of the SM, and is presently motivating vigorous efforts, on both theoretical and experimental sides, to understand in more depth the detailed properties of neutrinos and of their interactions. In particular, the electromagnetic properties of the neutrinos can play important roles in a wide variety of domains such as cosmology and astrophysics and can also provide a viable explanation for the observed depletion of the electron neutrino flux from the Sun. The electromagnetic interaction of Dirac neutrinos is described in terms of four form factors. The matrix element of the electromagnetic current between an initial neutrino state in with momentum pi and a final state with momentum reads.
publishDate 2003
dc.date.issued.none.fl_str_mv 2003
dc.date.accessioned.none.fl_str_mv 2017-09-21T20:39:31Z
dc.date.available.none.fl_str_mv 2017-09-21T20:39:31Z
dc.type.spa.fl_str_mv Artículo de investigación
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dc.identifier.citation.spa.fl_str_mv Hirsch, M., Nardi, E., & Restrepo Quintero, D. A. (2003). Bounds on the tau and muon neutrino vector and axial vector charge radius. Physical Review D. 67(033005), 1-10.
dc.identifier.issn.none.fl_str_mv 1550-7998
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/10495/8295
dc.identifier.eissn.none.fl_str_mv 2470-0031
identifier_str_mv Hirsch, M., Nardi, E., & Restrepo Quintero, D. A. (2003). Bounds on the tau and muon neutrino vector and axial vector charge radius. Physical Review D. 67(033005), 1-10.
1550-7998
2470-0031
url http://hdl.handle.net/10495/8295
dc.language.iso.spa.fl_str_mv eng
language eng
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dc.relation.citationendpage.spa.fl_str_mv 10
dc.relation.citationissue.spa.fl_str_mv 33005
dc.relation.citationstartpage.spa.fl_str_mv 1
dc.relation.citationvolume.spa.fl_str_mv 67
dc.relation.ispartofjournal.spa.fl_str_mv Physical Review D
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dc.publisher.spa.fl_str_mv The American Physical Society
dc.publisher.place.spa.fl_str_mv Estados Unidos
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spelling Hirsch, MartinNardi, EnricoRestrepo Quintero, Diego AlejandroGrupo de Fenomenologia de Interacciones Fundamentales2017-09-21T20:39:31Z2017-09-21T20:39:31Z2003Hirsch, M., Nardi, E., & Restrepo Quintero, D. A. (2003). Bounds on the tau and muon neutrino vector and axial vector charge radius. Physical Review D. 67(033005), 1-10.1550-7998http://hdl.handle.net/10495/82952470-0031ABSTRACT: Experimental evidence for neutrino oscillations implies that neutrinos are the first elementary particles whose properties cannot be fully described within the standard model. This hints at the possibility that other properties of these intriguing particles might substantially deviate from the predictions of the SM, and is presently motivating vigorous efforts, on both theoretical and experimental sides, to understand in more depth the detailed properties of neutrinos and of their interactions. In particular, the electromagnetic properties of the neutrinos can play important roles in a wide variety of domains such as cosmology and astrophysics and can also provide a viable explanation for the observed depletion of the electron neutrino flux from the Sun. The electromagnetic interaction of Dirac neutrinos is described in terms of four form factors. 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