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

Identifieur interne : 000451 ( PascalFrancis/Curation ); précédent : 000450; suivant : 000452

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

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

Source :

RBID : Pascal:12-0326865

Descripteurs français

English descriptors

Abstract

We tried to fit in any way the recent OPERA-CERN claims of a neutrino superluminal 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 IMB-Kamiokande 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 CERN-OPERA super-luminal speed. (3) A split neutrino flavor speed (among a common real mass relativistic ve component and a superluminal vμ) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between ve and vμ, vτ) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERA-CERN 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 graviton-neutrino split time delay among the gravity burst and neutronization neutrino peak in any future supernova explosion in Andromeda recordable in the Megaton neutrino detector.
pA  
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A06       @2 8
A08 01  1  ENG  @1 Inconsistency in super-luminal CERN-OPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass
A11 01  1    @1 FARGION (Daniele)
A11 02  1    @1 D'ARMIENTO (Daniele)
A14 01      @1 Physics Department, Rome University 1, Sapienza and INFN, Roma1 -PI A Moro 2 @2 00185 Rome @3 ITA @Z 1 aut. @Z 2 aut.
A20       @2 085002.1-085002.9
A21       @1 2012
A23 01      @0 ENG
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C01 01    ENG  @0 We tried to fit in any way the recent OPERA-CERN claims of a neutrino superluminal 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 IMB-Kamiokande 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 CERN-OPERA super-luminal speed. (3) A split neutrino flavor speed (among a common real mass relativistic ve component and a superluminal vμ) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between ve and vμ, vτ) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERA-CERN 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 graviton-neutrino split time delay among the gravity burst and neutronization neutrino peak in any future supernova explosion in Andromeda recordable in the Megaton neutrino detector.
C02 01  3    @0 001B20
C02 02  3    @0 001B10
C03 01  3  FRE  @0 CERN @5 26
C03 01  3  ENG  @0 CERN @5 26
C03 02  3  FRE  @0 Neutrino @5 27
C03 02  3  ENG  @0 Neutrinos @5 27
C03 03  3  FRE  @0 Mélangeage @5 28
C03 03  3  ENG  @0 Mixing @5 28
C03 04  3  FRE  @0 Masse neutrino @5 29
C03 04  3  ENG  @0 Neutrino mass @5 29
C03 05  3  FRE  @0 Supernova @5 30
C03 05  3  ENG  @0 Supernovae @5 30
C03 06  3  FRE  @0 Oscillation neutrino @5 31
C03 06  3  ENG  @0 Neutrino oscillations @5 31
C03 07  3  FRE  @0 Flaveur @5 32
C03 07  3  ENG  @0 Flavor @5 32
C03 08  3  FRE  @0 Tachyon @5 33
C03 08  3  ENG  @0 Tachyons @5 33
C03 09  3  FRE  @0 Timing @5 34
C03 09  3  ENG  @0 Timing @5 34
C03 10  X  FRE  @0 Modèle @5 35
C03 10  X  ENG  @0 Models @5 35
C03 10  X  SPA  @0 Modelo @5 35
C03 11  3  FRE  @0 Détection neutrino @5 36
C03 11  3  ENG  @0 Neutrino detection @5 36
C03 12  3  FRE  @0 Graviton @5 37
C03 12  3  ENG  @0 Gravitons @5 37
C03 13  3  FRE  @0 Temps retard @5 38
C03 13  3  ENG  @0 Time delay @5 38
C03 14  3  FRE  @0 Gravité @5 39
C03 14  3  ENG  @0 Gravity @5 39
C03 15  3  FRE  @0 Neutronisation @5 40
C03 15  3  ENG  @0 Neutronization @5 40
C03 16  X  FRE  @0 Explosion supernova @5 41
C03 16  X  ENG  @0 Supernovae explosion @5 41
C03 16  X  SPA  @0 Explosión supernova @5 41
C03 17  3  FRE  @0 Physique mathématique @5 42
C03 17  3  ENG  @0 Mathematical physics @5 42
C03 18  3  FRE  @0 Physique nucléaire @5 43
C03 18  3  ENG  @0 Nuclear physics @5 43
C03 19  3  FRE  @0 Particule sans masse @5 44
C03 19  3  ENG  @0 Massless particles @5 44
C03 20  3  FRE  @0 Masse particule élémentaire @5 45
C03 20  3  ENG  @0 Elementary particle mass @5 45
C03 21  3  FRE  @0 Particule élémentaire @5 46
C03 21  3  ENG  @0 Elementary particles @5 46
N21       @1 247
N44 01      @1 OTO
N82       @1 OTO

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Pascal:12-0326865

Le document en format XML

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<div type="abstract" xml:lang="en">We tried to fit in any way the recent OPERA-CERN claims of a neutrino superluminal 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 IMB-Kamiokande 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 CERN-OPERA super-luminal speed. (3) A split neutrino flavor speed (among a common real mass relativistic v
<sub>e</sub>
component and a superluminal v
<sub>μ</sub>
) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between v
<sub>e</sub>
and v
<sub>μ</sub>
, v
<sub>τ</sub>
) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERA-CERN 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 graviton-neutrino 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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<sub>e</sub>
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<sub>μ</sub>
) in an ad hoc frozen speed scenario that leads to the prompt neutrino de-coherence and rapid flavor mixing (between v
<sub>e</sub>
and v
<sub>μ</sub>
, v
<sub>τ</sub>
) that are in conflict with most oscillation records. Therefore, we concluded that an error must be hidden in OPERA-CERN 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 graviton-neutrino split time delay among the gravity burst and neutronization neutrino peak in any future supernova explosion in Andromeda recordable in the Megaton neutrino detector.</s0>
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   |texte=   Inconsistency in super-luminal CERN-OPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass
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