OperaV1, Main, Exploration, bibRecord, 000860

Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass

Identifieur interne : 000860 ( Main/Exploration ); précédent : 000859; suivant : 000861

Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass

Auteurs : Daniele Fargion [Italie] ; Daniele D'Armiento [Italie]

Source :

Journal of Physics G Nuclear and Particle Physics [ 0954-3899 ] ; 2012-08.

RBID : ISTEX:73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14

Descripteurs français

Pascal (Inist)
- CERN, Détection neutrino, Explosion supernova, Flaveur, Graviton, Gravité, Masse neutrino, Masse particule élémentaire, Modèle, Mélangeage, Neutrino, Neutronisation, Oscillation neutrino, Particule sans masse, Particule élémentaire, Physique mathématique, Physique nucléaire, Supernova, Tachyon, Temps retard, Timing.
Wicri :
- topic : Particule élémentaire, Physique nucléaire.

English descriptors

KwdEn :
- CERN, Elementary particle mass, Elementary particles, Flavor, Gravitons, Gravity, Massless particles, Mathematical physics, Mixing, Models, Neutrino detection, Neutrino mass, Neutrino oscillations, Neutrinos, Neutronization, Nuclear physics, Supernovae, Supernovae explosion, Tachyons, Time delay, Timing.

Abstract

We tried to fit in any way the recent OPERACERN claims of a neutrino super-luminal speed with the observed supernova SN1987A neutrino burst and all (or most) neutrino flavor oscillations. We considered three main frameworks: (1) tachyon imaginary neutrino mass, whose timing is nevertheless in conflict with the observed IMBKamiokande SN1987A burst by thousands of billion times longer. (2) An ad hoc anti-tachyon model whose timing shrinkage may accommodate the SN1987A burst but greatly disagrees with the energy-independent CERNOPERA super-luminal speed. (3) A split neutrino flavor speed (among a common real mass relativistic e component and a super-luminal ) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between e and , ) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERACERN time calibration (as indeed recent rumors seem to confirm). We concluded recalling the relevance of the real guaranteed minimal atmospheric neutrino mass whose detection may be achieved by a millisecond gravitonneutrino split time delay among the gravity burst and neutronization neutrino peak in any future supernova explosion in Andromeda recordable in the Megaton neutrino detector.

Url:

https://api.istex.fr/document/73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14/fulltext/pdf

DOI: 10.1088/0954-3899/39/8/085002

Affiliations:

Le document en format XML

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<front><div type="abstract">We tried to fit in any way the recent OPERACERN claims of a neutrino super-luminal speed with the observed supernova SN1987A neutrino burst and all (or most) neutrino flavor oscillations. We considered three main frameworks: (1) tachyon imaginary neutrino mass, whose timing is nevertheless in conflict with the observed IMBKamiokande SN1987A burst by thousands of billion times longer. (2) An ad hoc anti-tachyon model whose timing shrinkage may accommodate the SN1987A burst but greatly disagrees with the energy-independent CERNOPERA super-luminal speed. (3) A split neutrino flavor speed (among a common real mass relativistic e component and a super-luminal ) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between e and , ) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERACERN time calibration (as indeed recent rumors seem to confirm). We concluded recalling the relevance of the real guaranteed minimal atmospheric neutrino mass whose detection may be achieved by a millisecond gravitonneutrino split time delay among the gravity burst and neutronization neutrino peak in any future supernova explosion in Andromeda recordable in the Megaton neutrino detector.</div>
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Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass

Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass

Source :

Descripteurs français

English descriptors

Abstract

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

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

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