OperaV1, PascalFrancis, Curation, bibRecord, 000408

Do high-energy neutrinos travel faster than photons in a discrete space-time?

Identifieur interne : 000408 ( PascalFrancis/Curation ); précédent : 000407; suivant : 000409

Do high-energy neutrinos travel faster than photons in a discrete space-time?

Auteurs : She-Sheng Xue [Italie]

Source :

Physics letters. Section B [ 0370-2693 ] ; 2011.

RBID : Pascal:12-0093165

Descripteurs français

Pascal (Inist)
- Neutrino, Espace temps discret, Gravitation quantique, Parité, Symétrie jauge, Champ local, Théorie quantique champ, Opérateur, Interaction neutrino, Oscillation neutrino, Conservation parité, Asymétrie, Electron polarisé, Particule sans masse, Particule élémentaire.
Wicri :
- topic : Particule élémentaire.

English descriptors

KwdEn :
- Asymmetry, Discrete space time, Elementary particles, Gauge symmetry, Local field, Massless particles, Neutrino interactions, Neutrino oscillations, Neutrinos, Operator, Parity, Parity conservation, Polarized electron, Quantum field theory, Quantum gravity.

Abstract

The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.

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A02	`01`			`@0 PYLBAJ`
A03		`1`		`@0 Phys. lett., Sect. B`
A05				`@2 706`
A06				`@2 2-3`
A08	`01`	`1`	`ENG`	`@1 Do high-energy neutrinos travel faster than photons in a discrete space-time?`
A11	`01`	`1`		`@1 XUE (She-Sheng)`
A14	`01`			`@1 ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza @2 Rome @3 ITA @Z 1 aut.`
A20				`@1 213-218`
A21				`@1 2011`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 9425B @5 354000508895920140`
A44				`@0 0000 @1 © 2012 INIST-CNRS. All rights reserved.`
A45				`@0 29 ref.`
A47	`01`	`1`		`@0 12-0093165`
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A61				`@0 A`
A64	`01`	`1`		`@0 Physics letters. Section B`
A66	`01`			`@0 GBR`
C01	`01`		`ENG`	@0 The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.
C02	`01`	`3`		`@0 001B00`
C02	`02`	`3`		`@0 001B20`
C02	`03`	`3`		`@0 001B10`
C03	`01`	`3`	`FRE`	`@0 Neutrino @5 26`
C03	`01`	`3`	`ENG`	`@0 Neutrinos @5 26`
C03	`02`	`X`	`FRE`	`@0 Espace temps discret @5 27`
C03	`02`	`X`	`ENG`	`@0 Discrete space time @5 27`
C03	`02`	`X`	`SPA`	`@0 Espacio tiempo discreto @5 27`
C03	`03`	`3`	`FRE`	`@0 Gravitation quantique @5 28`
C03	`03`	`3`	`ENG`	`@0 Quantum gravity @5 28`
C03	`04`	`3`	`FRE`	`@0 Parité @5 29`
C03	`04`	`3`	`ENG`	`@0 Parity @5 29`
C03	`05`	`X`	`FRE`	`@0 Symétrie jauge @5 30`
C03	`05`	`X`	`ENG`	`@0 Gauge symmetry @5 30`
C03	`05`	`X`	`SPA`	`@0 Simetría galga @5 30`
C03	`06`	`X`	`FRE`	`@0 Champ local @5 31`
C03	`06`	`X`	`ENG`	`@0 Local field @5 31`
C03	`06`	`X`	`SPA`	`@0 Campo local @5 31`
C03	`07`	`3`	`FRE`	`@0 Théorie quantique champ @5 32`
C03	`07`	`3`	`ENG`	`@0 Quantum field theory @5 32`
C03	`08`	`X`	`FRE`	`@0 Opérateur @5 33`
C03	`08`	`X`	`ENG`	`@0 Operator @5 33`
C03	`08`	`X`	`SPA`	`@0 Operador @5 33`
C03	`09`	`3`	`FRE`	`@0 Interaction neutrino @5 34`
C03	`09`	`3`	`ENG`	`@0 Neutrino interactions @5 34`
C03	`10`	`3`	`FRE`	`@0 Oscillation neutrino @5 35`
C03	`10`	`3`	`ENG`	`@0 Neutrino oscillations @5 35`
C03	`11`	`X`	`FRE`	`@0 Conservation parité @5 36`
C03	`11`	`X`	`ENG`	`@0 Parity conservation @5 36`
C03	`11`	`X`	`SPA`	`@0 Conservación paridad @5 36`
C03	`12`	`3`	`FRE`	`@0 Asymétrie @5 37`
C03	`12`	`3`	`ENG`	`@0 Asymmetry @5 37`
C03	`13`	`X`	`FRE`	`@0 Electron polarisé @5 38`
C03	`13`	`X`	`ENG`	`@0 Polarized electron @5 38`
C03	`13`	`X`	`SPA`	`@0 Electrón polarizado @5 38`
C03	`14`	`3`	`FRE`	`@0 Particule sans masse @5 39`
C03	`14`	`3`	`ENG`	`@0 Massless particles @5 39`
C03	`15`	`3`	`FRE`	`@0 Particule élémentaire @5 40`
C03	`15`	`3`	`ENG`	`@0 Elementary particles @5 40`
N21				`@1 072`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

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Le document en format XML

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<front><div type="abstract" xml:lang="en">The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.</div>
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Do high-energy neutrinos travel faster than photons in a discrete space-time?

Do high-energy neutrinos travel faster than photons in a discrete space-time?

Source :

Descripteurs français

English descriptors

Abstract

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Links to Exploration step

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