Serveur d'exploration sur l'opéra

Attention, ce site est en cours de développement !
Attention, site généré par des moyens informatiques à partir de corpus bruts.
Les informations ne sont donc pas validées.

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

Identifieur interne : 000002 ( Istex/Curation ); précédent : 000001; suivant : 000003

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 :

RBID : ISTEX:73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14

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

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


Links to Exploration step

ISTEX:73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14

Le document en format XML

<record>
<TEI wicri:istexFullTextTei="biblStruct">
<teiHeader>
<fileDesc>
<titleStmt>
<title>Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass</title>
<author>
<name sortKey="Fargion, Daniele" sort="Fargion, Daniele" uniqKey="Fargion D" first="Daniele" last="Fargion">Daniele Fargion</name>
<affiliation wicri:level="1">
<mods:affiliation>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome, Italy</mods:affiliation>
<country xml:lang="fr">Italie</country>
<wicri:regionArea>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1">
<mods:affiliation>E-mail: daniele.fargion@roma1.infn.it</mods:affiliation>
<country wicri:rule="url">Italie</country>
</affiliation>
</author>
<author>
<name sortKey="D Armiento, Daniele" sort="D Armiento, Daniele" uniqKey="D Armiento D" first="Daniele" last="D'Armiento">Daniele D'Armiento</name>
<affiliation wicri:level="1">
<mods:affiliation>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome, Italy</mods:affiliation>
<country xml:lang="fr">Italie</country>
<wicri:regionArea>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome</wicri:regionArea>
</affiliation>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14</idno>
<date when="2012" year="2012">2012</date>
<idno type="doi">10.1088/0954-3899/39/8/085002</idno>
<idno type="url">https://api.istex.fr/document/73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14/fulltext/pdf</idno>
<idno type="wicri:Area/Istex/Corpus">000002</idno>
<idno type="wicri:Area/Istex/Curation">000002</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title level="a">Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass</title>
<author>
<name sortKey="Fargion, Daniele" sort="Fargion, Daniele" uniqKey="Fargion D" first="Daniele" last="Fargion">Daniele Fargion</name>
<affiliation wicri:level="1">
<mods:affiliation>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome, Italy</mods:affiliation>
<country xml:lang="fr">Italie</country>
<wicri:regionArea>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome</wicri:regionArea>
</affiliation>
<affiliation wicri:level="1">
<mods:affiliation>E-mail: daniele.fargion@roma1.infn.it</mods:affiliation>
<country wicri:rule="url">Italie</country>
</affiliation>
</author>
<author>
<name sortKey="D Armiento, Daniele" sort="D Armiento, Daniele" uniqKey="D Armiento D" first="Daniele" last="D'Armiento">Daniele D'Armiento</name>
<affiliation wicri:level="1">
<mods:affiliation>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome, Italy</mods:affiliation>
<country xml:lang="fr">Italie</country>
<wicri:regionArea>Physics Department, Rome University 1, Sapienza and INFN, Roma1 Pl A Moro 2, 00185 Rome</wicri:regionArea>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series>
<title level="j">Journal of Physics G Nuclear and Particle Physics</title>
<idno type="ISSN">0954-3899</idno>
<idno type="eISSN">1361-6471</idno>
<imprint>
<publisher>IOP Publishing</publisher>
<date type="published" when="2012-08">2012-08</date>
<biblScope unit="volume">39</biblScope>
<biblScope unit="issue">8</biblScope>
</imprint>
<idno type="ISSN">0954-3899</idno>
</series>
<idno type="istex">73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14</idno>
<idno type="DOI">10.1088/0954-3899/39/8/085002</idno>
<idno type="href">http://stacks.iop.org/JPhysG/39/085002</idno>
<idno type="ArticleID">jpg410574</idno>
</biblStruct>
</sourceDesc>
<seriesStmt>
<idno type="ISSN">0954-3899</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass></textClass>
<langUsage>
<language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<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>
</front>
</TEI>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Wicri/Musique/explor/OperaV1/Data/Istex/Curation
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000002 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/Istex/Curation/biblio.hfd -nk 000002 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Wicri/Musique
   |area=    OperaV1
   |flux=    Istex
   |étape=   Curation
   |type=    RBID
   |clé=     ISTEX:73662B5D28EDD5B0F28896AE8C5B9FF7C3890B14
   |texte=   Inconsistency in super-luminal CERNOPERA neutrino speed with the observed SN1987A burst and neutrino mixing for any imaginary neutrino mass
}}

Wicri

This area was generated with Dilib version V0.6.21.
Data generation: Thu Apr 14 14:59:05 2016. Site generation: Thu Oct 8 06:48:41 2020