Superluminal velocity through near-maximal neutrino oscillations or by being off shell
Identifieur interne : 000853 ( Main/Curation ); précédent : 000852; suivant : 000854Superluminal velocity through near-maximal neutrino oscillations or by being off shell
Auteurs : Tim R. Morris [Royaume-Uni]Source :
- Journal of Physics G Nuclear and Particle Physics [ 0954-3899 ] ; 2012-04.
Descripteurs français
- Pascal (Inist)
- Wicri :
- topic : Particule élémentaire, Physique nucléaire.
English descriptors
- KwdEn :
Abstract
Recently it was suggested that the observation of superluminal neutrinos by the OPERA collaboration may be due to group velocity effects resulting from close-to-maximal oscillation between neutrino mass eigenstates, in analogy to known effects in optics. We show that superluminal propagation does occur through this effect for a series of very narrow energy ranges, but this phenomenon cannot explain the OPERA measurement. Superluminal propagation can also occur if one of the neutrino masses is extremely small. However the effect only has appreciable amplitude at energies of order this mass and thus has negligible overlap with the multi-GeV scale of the experiment.
Url:
DOI: 10.1088/0954-3899/39/4/045010
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: Pour aller vers cette notice dans l'étape Curation :000104
- to stream Istex, to step Curation: Pour aller vers cette notice dans l'étape Curation :000104
- to stream Istex, to step Checkpoint: Pour aller vers cette notice dans l'étape Curation :000031
- to stream Main, to step Merge: Pour aller vers cette notice dans l'étape Curation :000849
- to stream PascalFrancis, to step Corpus: Pour aller vers cette notice dans l'étape Curation :000100
- to stream PascalFrancis, to step Curation: Pour aller vers cette notice dans l'étape Curation :000426
- to stream PascalFrancis, to step Checkpoint: Pour aller vers cette notice dans l'étape Curation :000054
- to stream Main, to step Merge: Pour aller vers cette notice dans l'étape Curation :000899
Links to Exploration step
ISTEX:018F1A8D7E43B5791309459D40767777B8531BBCLe document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title>Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author wicri:is="90%"><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R" last="Morris">Tim R. Morris</name>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:018F1A8D7E43B5791309459D40767777B8531BBC</idno>
<date when="2012" year="2012">2012</date>
<idno type="doi">10.1088/0954-3899/39/4/045010</idno>
<idno type="url">https://api.istex.fr/document/018F1A8D7E43B5791309459D40767777B8531BBC/fulltext/pdf</idno>
<idno type="wicri:Area/Istex/Corpus">000104</idno>
<idno type="wicri:Area/Istex/Curation">000104</idno>
<idno type="wicri:Area/Istex/Checkpoint">000031</idno>
<idno type="wicri:doubleKey">0954-3899:2012:Morris T:superluminal:velocity:through</idno>
<idno type="wicri:Area/Main/Merge">000849</idno>
<idno type="wicri:source">INIST</idno>
<idno type="RBID">Pascal:12-0189172</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000100</idno>
<idno type="wicri:Area/PascalFrancis/Curation">000426</idno>
<idno type="wicri:Area/PascalFrancis/Checkpoint">000054</idno>
<idno type="wicri:doubleKey">0954-3899:2012:Morris T:superluminal:velocity:through</idno>
<idno type="wicri:Area/Main/Merge">000899</idno>
<idno type="wicri:Area/Main/Curation">000853</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title level="a">Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author wicri:is="90%"><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R" last="Morris">Tim R. Morris</name>
<affiliation wicri:level="1"><country xml:lang="fr">Royaume-Uni</country>
<wicri:regionArea>School of Physics and Astronomy, University of Southampton Highfield, Southampton, SO17 1BJ</wicri:regionArea>
<wicri:noRegion>SO17 1BJ</wicri:noRegion>
</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="2012-04">2012-04</date>
<biblScope unit="volume">39</biblScope>
<biblScope unit="issue">4</biblScope>
</imprint>
<idno type="ISSN">0954-3899</idno>
</series>
<idno type="istex">018F1A8D7E43B5791309459D40767777B8531BBC</idno>
<idno type="DOI">10.1088/0954-3899/39/4/045010</idno>
<idno type="href">http://stacks.iop.org/JPhysG/39/045010</idno>
<idno type="ArticleID">jpg417154</idno>
</biblStruct>
</sourceDesc>
<seriesStmt><idno type="ISSN">0954-3899</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Eigenstates</term>
<term>Elementary particle mass</term>
<term>Elementary particles</term>
<term>Group velocity</term>
<term>Massless particles</term>
<term>Mathematical physics</term>
<term>Neutrino mass</term>
<term>Neutrino oscillations</term>
<term>Neutrinos</term>
<term>Nuclear physics</term>
<term>Superluminal velocity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Etat propre</term>
<term>Masse neutrino</term>
<term>Masse particule élémentaire</term>
<term>Neutrino</term>
<term>Oscillation neutrino</term>
<term>Particule sans masse</term>
<term>Particule élémentaire</term>
<term>Physique mathématique</term>
<term>Physique nucléaire</term>
<term>Vitesse groupe</term>
<term>Vitesse superluminique</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Particule élémentaire</term>
<term>Physique nucléaire</term>
</keywords>
</textClass>
<langUsage><language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front><div type="abstract">Recently it was suggested that the observation of superluminal neutrinos by the OPERA collaboration may be due to group velocity effects resulting from close-to-maximal oscillation between neutrino mass eigenstates, in analogy to known effects in optics. We show that superluminal propagation does occur through this effect for a series of very narrow energy ranges, but this phenomenon cannot explain the OPERA measurement. Superluminal propagation can also occur if one of the neutrino masses is extremely small. However the effect only has appreciable amplitude at energies of order this mass and thus has negligible overlap with the multi-GeV scale of the experiment.</div>
</front>
</TEI>
<double idat="0954-3899:2012:Morris T:superluminal:velocity:through"><INIST><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R." last="Morris">Tim R. Morris</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>School of Physics and Astronomy, University of Southampton Highfield</s1>
<s2>Southampton, SO17 1BJ</s2>
<s3>GBR</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Southampton, SO17 1BJ</wicri:noRegion>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">12-0189172</idno>
<date when="2012">2012</date>
<idno type="stanalyst">PASCAL 12-0189172 INIST</idno>
<idno type="RBID">Pascal:12-0189172</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000100</idno>
<idno type="wicri:Area/PascalFrancis/Curation">000426</idno>
<idno type="wicri:Area/PascalFrancis/Checkpoint">000054</idno>
<idno type="wicri:doubleKey">0954-3899:2012:Morris T:superluminal:velocity:through</idno>
<idno type="wicri:Area/Main/Merge">000899</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R." last="Morris">Tim R. Morris</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>School of Physics and Astronomy, University of Southampton Highfield</s1>
<s2>Southampton, SO17 1BJ</s2>
<s3>GBR</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Southampton, SO17 1BJ</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series><title level="j" type="main">Journal of physics. G. Nuclear and particle physics : (Print)</title>
<title level="j" type="abbreviated">J. phys., G, Nucl. part. phys. : (Print)</title>
<idno type="ISSN">0954-3899</idno>
<imprint><date when="2012">2012</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><title level="j" type="main">Journal of physics. G. Nuclear and particle physics : (Print)</title>
<title level="j" type="abbreviated">J. phys., G, Nucl. part. phys. : (Print)</title>
<idno type="ISSN">0954-3899</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Eigenstates</term>
<term>Elementary particle mass</term>
<term>Elementary particles</term>
<term>Group velocity</term>
<term>Massless particles</term>
<term>Mathematical physics</term>
<term>Neutrino mass</term>
<term>Neutrino oscillations</term>
<term>Neutrinos</term>
<term>Nuclear physics</term>
<term>Superluminal velocity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Vitesse superluminique</term>
<term>Oscillation neutrino</term>
<term>Neutrino</term>
<term>Vitesse groupe</term>
<term>Etat propre</term>
<term>Masse neutrino</term>
<term>Physique mathématique</term>
<term>Physique nucléaire</term>
<term>Particule sans masse</term>
<term>Masse particule élémentaire</term>
<term>Particule élémentaire</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Physique nucléaire</term>
<term>Particule élémentaire</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">Recently it was suggested that the observation of superluminal neutrinos by the OPERA collaboration may be due to group velocity effects resulting from close-to-maximal oscillation between neutrino mass eigenstates, in analogy to known effects in optics. We show that superluminal propagation does occur through this effect for a series of very narrow energy ranges, but this phenomenon cannot explain the OPERA measurement. Superluminal propagation can also occur if one of the neutrino masses is extremely small. However the effect only has appreciable amplitude at energies of order this mass and thus has negligible overlap with the multi-GeV scale of the experiment.</div>
</front>
</TEI>
</INIST>
<ISTEX><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title>Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author wicri:is="90%"><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R" last="Morris">Tim R. Morris</name>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:018F1A8D7E43B5791309459D40767777B8531BBC</idno>
<date when="2012" year="2012">2012</date>
<idno type="doi">10.1088/0954-3899/39/4/045010</idno>
<idno type="url">https://api.istex.fr/document/018F1A8D7E43B5791309459D40767777B8531BBC/fulltext/pdf</idno>
<idno type="wicri:Area/Istex/Corpus">000104</idno>
<idno type="wicri:Area/Istex/Curation">000104</idno>
<idno type="wicri:Area/Istex/Checkpoint">000031</idno>
<idno type="wicri:doubleKey">0954-3899:2012:Morris T:superluminal:velocity:through</idno>
<idno type="wicri:Area/Main/Merge">000849</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title level="a">Superluminal velocity through near-maximal neutrino oscillations or by being off shell</title>
<author wicri:is="90%"><name sortKey="Morris, Tim R" sort="Morris, Tim R" uniqKey="Morris T" first="Tim R" last="Morris">Tim R. Morris</name>
<affiliation wicri:level="1"><country xml:lang="fr">Royaume-Uni</country>
<wicri:regionArea>School of Physics and Astronomy, University of Southampton Highfield, Southampton, SO17 1BJ</wicri:regionArea>
<wicri:noRegion>SO17 1BJ</wicri:noRegion>
</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="2012-04">2012-04</date>
<biblScope unit="volume">39</biblScope>
<biblScope unit="issue">4</biblScope>
</imprint>
<idno type="ISSN">0954-3899</idno>
</series>
<idno type="istex">018F1A8D7E43B5791309459D40767777B8531BBC</idno>
<idno type="DOI">10.1088/0954-3899/39/4/045010</idno>
<idno type="href">http://stacks.iop.org/JPhysG/39/045010</idno>
<idno type="ArticleID">jpg417154</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">Recently it was suggested that the observation of superluminal neutrinos by the OPERA collaboration may be due to group velocity effects resulting from close-to-maximal oscillation between neutrino mass eigenstates, in analogy to known effects in optics. We show that superluminal propagation does occur through this effect for a series of very narrow energy ranges, but this phenomenon cannot explain the OPERA measurement. Superluminal propagation can also occur if one of the neutrino masses is extremely small. However the effect only has appreciable amplitude at energies of order this mass and thus has negligible overlap with the multi-GeV scale of the experiment.</div>
</front>
</TEI>
</ISTEX>
</double>
</record>
Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Musique/explor/OperaV1/Data/Main/Curation
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000853 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Curation/biblio.hfd -nk 000853 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien |wiki= Wicri/Musique |area= OperaV1 |flux= Main |étape= Curation |type= RBID |clé= ISTEX:018F1A8D7E43B5791309459D40767777B8531BBC |texte= Superluminal velocity through near-maximal neutrino oscillations or by being off shell }}
![]() | This area was generated with Dilib version V0.6.21. | ![]() |