OperaV1, PascalFrancis, Corpus, bibRecord, 000108

A model of superluminal neutrinos

Identifieur interne : 000108 ( PascalFrancis/Corpus ); précédent : 000107; suivant : 000109

A model of superluminal neutrinos

Auteurs : D. Marfatia ; H. P S ; S. Pakvasa ; T. J. Weiler

Source :

Physics letters. Section B [ 0370-2693 ] ; 2012.

RBID : Pascal:12-0120612

Descripteurs français

Pascal (Inist)
- Modèle, Neutrino, Oscillation neutrino, Mélangeage, Particule sans masse, Particule élémentaire.

English descriptors

KwdEn :
- Elementary particles, Massless particles, Mixing, Models, Neutrino oscillations, Neutrinos.

Abstract

Motivated by the tentative observation of superluminal neutrinos by the OPERA experiment, we present a model of active-sterile neutrino oscillations in which sterile neutrinos are superluminal and active neutrinos appear superluminal by virtue of neutrino mixing. The model demonstrates some interesting possibilities and challenges that apply to a large class of models aiming to explain the OPERA result.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

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A05				`@2 707`
A06				`@2 5`
A08	`01`	`1`	`ENG`	`@1 A model of superluminal neutrinos`
A11	`01`	`1`		`@1 MARFATIA (D.)`
A11	`02`	`1`		`@1 PÄS (H.)`
A11	`03`	`1`		`@1 PAKVASA (S.)`
A11	`04`	`1`		`@1 WEILER (T. J.)`
A14	`01`			`@1 Department of Physics & Astronomy, University of Kansas @2 Lawrence, KS 66045 @3 USA @Z 1 aut.`
A14	`02`			`@1 Fakultät für Physik, Technische Universitat Dortmund @2 44221 Dortmund @3 DEU @Z 2 aut.`
A14	`03`			`@1 Department of Physics & Astronomy, University of Hawaii @2 Honolulu, H196822 @3 USA @Z 3 aut.`
A14	`04`			`@1 Department of Physics & Astronomy, Vanderbilt University @2 Nashville, TN 37235 @3 USA @Z 4 aut.`
A20				`@1 553-557`
A21				`@1 2012`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 9425B @5 354000502827490150`
A44				`@0 0000 @1 © 2012 INIST-CNRS. All rights reserved.`
A45				`@0 12 ref.`
A47	`01`	`1`		`@0 12-0120612`
A60				`@1 P`
A61				`@0 A`
A64	`01`	`1`		`@0 Physics letters. Section B`
A66	`01`			`@0 GBR`
C01	`01`		`ENG`	`@0 Motivated by the tentative observation of superluminal neutrinos by the OPERA experiment, we present a model of active-sterile neutrino oscillations in which sterile neutrinos are superluminal and active neutrinos appear superluminal by virtue of neutrino mixing. The model demonstrates some interesting possibilities and challenges that apply to a large class of models aiming to explain the OPERA result.`
C02	`01`	`3`		`@0 001B00`
C02	`02`	`3`		`@0 001B20`
C02	`03`	`3`		`@0 001B10`
C03	`01`	`X`	`FRE`	`@0 Modèle @5 26`
C03	`01`	`X`	`ENG`	`@0 Models @5 26`
C03	`01`	`X`	`SPA`	`@0 Modelo @5 26`
C03	`02`	`3`	`FRE`	`@0 Neutrino @5 27`
C03	`02`	`3`	`ENG`	`@0 Neutrinos @5 27`
C03	`03`	`3`	`FRE`	`@0 Oscillation neutrino @5 28`
C03	`03`	`3`	`ENG`	`@0 Neutrino oscillations @5 28`
C03	`04`	`3`	`FRE`	`@0 Mélangeage @5 29`
C03	`04`	`3`	`ENG`	`@0 Mixing @5 29`
C03	`05`	`3`	`FRE`	`@0 Particule sans masse @5 30`
C03	`05`	`3`	`ENG`	`@0 Massless particles @5 30`
C03	`06`	`3`	`FRE`	`@0 Particule élémentaire @5 31`
C03	`06`	`3`	`ENG`	`@0 Elementary particles @5 31`
N21				`@1 093`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

Format Inist (serveur)

NO :	PASCAL 12-0120612 INIST
ET :	A model of superluminal neutrinos
AU :	MARFATIA (D.); PÄS (H.); PAKVASA (S.); WEILER (T. J.)
AF :	Department of Physics & Astronomy, University of Kansas/Lawrence, KS 66045/Etats-Unis (1 aut.); Fakultät für Physik, Technische Universitat Dortmund/44221 Dortmund/Allemagne (2 aut.); Department of Physics & Astronomy, University of Hawaii/Honolulu, H196822/Etats-Unis (3 aut.); Department of Physics & Astronomy, Vanderbilt University/Nashville, TN 37235/Etats-Unis (4 aut.)
DT :	Publication en série; Niveau analytique
SO :	Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2012; Vol. 707; No. 5; Pp. 553-557; Bibl. 12 ref.
LA :	Anglais
EA :	Motivated by the tentative observation of superluminal neutrinos by the OPERA experiment, we present a model of active-sterile neutrino oscillations in which sterile neutrinos are superluminal and active neutrinos appear superluminal by virtue of neutrino mixing. The model demonstrates some interesting possibilities and challenges that apply to a large class of models aiming to explain the OPERA result.
CC :	001B00; 001B20; 001B10
FD :	Modèle; Neutrino; Oscillation neutrino; Mélangeage; Particule sans masse; Particule élémentaire
ED :	Models; Neutrinos; Neutrino oscillations; Mixing; Massless particles; Elementary particles
SD :	Modelo
LO :	INIST-9425B.354000502827490150
ID :	12-0120612

Links to Exploration step

Pascal:12-0120612

Le document en format XML

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A model of superluminal neutrinos

A model of superluminal neutrinos

Source :

Descripteurs français

English descriptors

Abstract

Notice en format standard (ISO 2709)

Format Inist (serveur)

Links to Exploration step

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri