OperaV1, PascalFrancis, Corpus, bibRecord, 000095

On the possibility of superluminal neutrino propagation

Identifieur interne : 000095 ( PascalFrancis/Corpus ); précédent : 000094; suivant : 000096

On the possibility of superluminal neutrino propagation

Auteurs : Jean Alexandre ; John Ellis ; Nick E. Mavromatos

Source :

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

RBID : Pascal:12-0224570

Descripteurs français

Pascal (Inist)
- Neutrino, Supernova, Rayonnement gravitationnel, Invariance Lorentz, Modèle théorique, Fermion, Théorie jauge, Champ fermion, Particule sans masse, Particule élémentaire.

English descriptors

KwdEn :
- Elementary particles, Fermion field, Fermions, Gauge theory, Gravitational radiation, Lorentz invariance, Massless particles, Neutrinos, Supernovae, Theoretical model.

Abstract

We analyze the possibility of superluminal neutrino propagation δν ≡ (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that the SN1987a data rule out δν ∼ (E_ν/M_N)^N for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

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A08	`01`	`1`	`ENG`	`@1 On the possibility of superluminal neutrino propagation`
A11	`01`	`1`		`@1 ALEXANDRE (Jean)`
A11	`02`	`1`		`@1 ELLIS (John)`
A11	`03`	`1`		`@1 MAVROMATOS (Nick E.)`
A14	`01`			`@1 Department of Physics, King's College London Strand @2 London WC2R 2LS @3 GBR @Z 1 aut. @Z 2 aut. @Z 3 aut.`
A14	`02`			`@1 Theory Division, Department of Physics, CERN, CH @2 1211. Geneva @3 CHE @Z 2 aut. @Z 3 aut.`
A20				`@1 456-461`
A21				`@1 2012`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 9425B @5 354000509343070330`
A44				`@0 0000 @1 © 2012 INIST-CNRS. All rights reserved.`
A45				`@0 27 ref.`
A47	`01`	`1`		`@0 12-0224570`
A60				`@1 P`
A61				`@0 A`
A64	`01`	`1`		`@0 Physics letters. Section B`
A66	`01`			`@0 GBR`
C01	`01`		`ENG`	@0 We analyze the possibility of superluminal neutrino propagation δν ≡ (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that the SN1987a data rule out δν ∼ (E_ν/M_N)^N for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.
C02	`01`	`3`		`@0 001B00`
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C03	`01`	`3`	`ENG`	`@0 Neutrinos @5 26`
C03	`02`	`3`	`FRE`	`@0 Supernova @5 27`
C03	`02`	`3`	`ENG`	`@0 Supernovae @5 27`
C03	`03`	`3`	`FRE`	`@0 Rayonnement gravitationnel @5 28`
C03	`03`	`3`	`ENG`	`@0 Gravitational radiation @5 28`
C03	`04`	`3`	`FRE`	`@0 Invariance Lorentz @5 29`
C03	`04`	`3`	`ENG`	`@0 Lorentz invariance @5 29`
C03	`05`	`X`	`FRE`	`@0 Modèle théorique @5 30`
C03	`05`	`X`	`ENG`	`@0 Theoretical model @5 30`
C03	`05`	`X`	`SPA`	`@0 Modelo teórico @5 30`
C03	`06`	`3`	`FRE`	`@0 Fermion @5 31`
C03	`06`	`3`	`ENG`	`@0 Fermions @5 31`
C03	`07`	`X`	`FRE`	`@0 Théorie jauge @5 32`
C03	`07`	`X`	`ENG`	`@0 Gauge theory @5 32`
C03	`07`	`X`	`SPA`	`@0 Teoría gauge @5 32`
C03	`08`	`X`	`FRE`	`@0 Champ fermion @5 33`
C03	`08`	`X`	`ENG`	`@0 Fermion field @5 33`
C03	`08`	`X`	`SPA`	`@0 Campo fermiónico @5 33`
C03	`09`	`3`	`FRE`	`@0 Particule sans masse @5 34`
C03	`09`	`3`	`ENG`	`@0 Massless particles @5 34`
C03	`10`	`3`	`FRE`	`@0 Particule élémentaire @5 35`
C03	`10`	`3`	`ENG`	`@0 Elementary particles @5 35`
N21				`@1 170`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

Format Inist (serveur)

NO :	PASCAL 12-0224570 INIST
ET :	On the possibility of superluminal neutrino propagation
AU :	ALEXANDRE (Jean); ELLIS (John); MAVROMATOS (Nick E.)
AF :	Department of Physics, King's College London Strand/London WC2R 2LS/Royaume-Uni (1 aut., 2 aut., 3 aut.); Theory Division, Department of Physics, CERN, CH/1211. Geneva/Suisse (2 aut., 3 aut.)
DT :	Publication en série; Niveau analytique
SO :	Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2012; Vol. 706; No. 4-5; Pp. 456-461; Bibl. 27 ref.
LA :	Anglais
EA :	We analyze the possibility of superluminal neutrino propagation δν ≡ (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that the SN1987a data rule out δν ∼ (E_ν/M_N)^N for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.
CC :	001B00; 001B20; 001B10
FD :	Neutrino; Supernova; Rayonnement gravitationnel; Invariance Lorentz; Modèle théorique; Fermion; Théorie jauge; Champ fermion; Particule sans masse; Particule élémentaire
ED :	Neutrinos; Supernovae; Gravitational radiation; Lorentz invariance; Theoretical model; Fermions; Gauge theory; Fermion field; Massless particles; Elementary particles
SD :	Modelo teórico; Teoría gauge; Campo fermiónico
LO :	INIST-9425B.354000509343070330
ID :	12-0224570

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Pascal:12-0224570

Le document en format XML

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<front><div type="abstract" xml:lang="en">We analyze the possibility of superluminal neutrino propagation δν ≡ (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that the SN1987a data rule out δν ∼ (E<sub>ν/</sub>
M<sub>N</sub>
)<sup>N</sup>
 for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.</div>
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M<sub>N</sub>
)<sup>N</sup>
 for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.</s0>
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<server><NO>PASCAL 12-0224570 INIST</NO>
<ET>On the possibility of superluminal neutrino propagation</ET>
<AU>ALEXANDRE (Jean); ELLIS (John); MAVROMATOS (Nick E.)</AU>
<AF>Department of Physics, King's College London Strand/London WC2R 2LS/Royaume-Uni (1 aut., 2 aut., 3 aut.); Theory Division, Department of Physics, CERN, CH/1211. Geneva/Suisse (2 aut., 3 aut.)</AF>
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<LA>Anglais</LA>
<EA>We analyze the possibility of superluminal neutrino propagation δν ≡ (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that the SN1987a data rule out δν ∼ (E<sub>ν/</sub>
M<sub>N</sub>
)<sup>N</sup>
 for N ≤ 2 and exclude, in particular, a Lorentz-invariant interpretation in terms of a 'conventional' tachyonic neutrino. We present two toy Lorentz-violating theoretical models, one a Lifshitz-type fermion model with superluminality depending quadratically on energy, and the other a Lorentz-violating modification of a massless Abelian gauge theory with axial-vector couplings to fermions. In the presence of an appropriate background field, fermions may propagate superluminally or subluminally, depending inversely on energy, and on direction. Reconciling OPERA with SN1987a would require this background field to depend on location.</EA>
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   |flux=    PascalFrancis
   |étape=   Corpus
   |type=    RBID
   |clé=     Pascal:12-0224570
   |texte=   On the possibility of superluminal neutrino propagation
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On the possibility of superluminal neutrino propagation

On the possibility of superluminal neutrino propagation

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