OperaV1, PascalFrancis, Curation, bibRecord, 000457

The price of neutrino superluminality continues to rise

Identifieur interne : 000457 ( PascalFrancis/Curation ); précédent : 000456; suivant : 000458

The price of neutrino superluminality continues to rise

Auteurs : Arthur Hebecker [Allemagne] ; Alexander Knochel [Allemagne]

Source :

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

RBID : Pascal:12-0350354

Descripteurs français

Pascal (Inist)
- Neutrino, Modèle, Supernova, Interaction courte portée, Matière dense, Couplage faible, Violation, Particule sans masse, Particule élémentaire.
Wicri :
- topic : Particule élémentaire.

English descriptors

KwdEn :
- Dense matter, Elementary particles, Massless particles, Models, Neutrinos, Short-range interactions, Supernovae, Violations, Weak coupling.

Abstract

We revisit the model building challenges that one faces when trying to reconcile the OPERA claim of neutrino superluminality with other observational constraints. The severity of the supernova bound and of the kinematical constraints of Cohen-Glashow type lead us to focus on scenarios where all types of particles are superluminal inside matter. In contrast to the Dvali-Vikman proposal, this matter effect needs to be very short-ranged to avoid constraints from experiments on the Earth's surface in low-density environments. Due to this short range, the interaction underlying such a matter effect would have to be far stronger than permitted by fifth-force bounds. As a conceivable way out we suggest to make the matter effect "binary", i.e., dense matter does not directly trigger superluminality, but merely induces the transition to a different phase of some weakly coupled hidden sector. This phase exhibits spontaneous Lorentz violation or at least a stronger than usual mediation of some residual Lorentz violation to all matter. The effect has not been observed before since we have never before been able to measure the velocity of high-energy particles in dense matter with sufficient precision.

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A11	`02`	`1`		`@1 KNOCHEL (Alexander)`
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C03	`01`	`3`	`ENG`	`@0 Neutrinos @5 26`
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C03	`05`	`X`	`FRE`	`@0 Matière dense @5 30`
C03	`05`	`X`	`ENG`	`@0 Dense matter @5 30`
C03	`05`	`X`	`SPA`	`@0 Materia densa @5 30`
C03	`06`	`X`	`FRE`	`@0 Couplage faible @5 31`
C03	`06`	`X`	`ENG`	`@0 Weak coupling @5 31`
C03	`06`	`X`	`SPA`	`@0 Acoplamiento débil @5 31`
C03	`07`	`3`	`FRE`	`@0 Violation @5 32`
C03	`07`	`3`	`ENG`	`@0 Violations @5 32`
C03	`08`	`3`	`FRE`	`@0 Particule sans masse @5 33`
C03	`08`	`3`	`ENG`	`@0 Massless particles @5 33`
C03	`09`	`3`	`FRE`	`@0 Particule élémentaire @5 34`
C03	`09`	`3`	`ENG`	`@0 Elementary particles @5 34`
N21				`@1 268`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

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Le document en format XML

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The price of neutrino superluminality continues to rise

The price of neutrino superluminality continues to rise

Source :

Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

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