Do high-energy neutrinos travel faster than photons in a discrete space-time?
Identifieur interne : 000110 ( PascalFrancis/Corpus ); précédent : 000109; suivant : 000111Do high-energy neutrinos travel faster than photons in a discrete space-time?
Auteurs : She-Sheng XueSource :
- Physics letters. Section B [ 0370-2693 ] ; 2011.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.
Notice en format standard (ISO 2709)
Pour connaître la documentation sur le format Inist Standard.
pA |
|
---|
Format Inist (serveur)
NO : | PASCAL 12-0093165 INIST |
---|---|
ET : | Do high-energy neutrinos travel faster than photons in a discrete space-time? |
AU : | XUE (She-Sheng) |
AF : | ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza/Rome/Italie (1 aut.) |
DT : | Publication en série; Niveau analytique |
SO : | Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2011; Vol. 706; No. 2-3; Pp. 213-218; Bibl. 29 ref. |
LA : | Anglais |
EA : | The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons. |
CC : | 001B00; 001B20; 001B10 |
FD : | Neutrino; Espace temps discret; Gravitation quantique; Parité; Symétrie jauge; Champ local; Théorie quantique champ; Opérateur; Interaction neutrino; Oscillation neutrino; Conservation parité; Asymétrie; Electron polarisé; Particule sans masse; Particule élémentaire |
ED : | Neutrinos; Discrete space time; Quantum gravity; Parity; Gauge symmetry; Local field; Quantum field theory; Operator; Neutrino interactions; Neutrino oscillations; Parity conservation; Asymmetry; Polarized electron; Massless particles; Elementary particles |
SD : | Espacio tiempo discreto; Simetría galga; Campo local; Operador; Conservación paridad; Electrón polarizado |
LO : | INIST-9425B.354000508895920140 |
ID : | 12-0093165 |
Links to Exploration step
Pascal:12-0093165Le document en format XML
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Do high-energy neutrinos travel faster than photons in a discrete space-time?</title>
<author><name sortKey="Xue, She Sheng" sort="Xue, She Sheng" uniqKey="Xue S" first="She-Sheng" last="Xue">She-Sheng Xue</name>
<affiliation><inist:fA14 i1="01"><s1>ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza</s1>
<s2>Rome</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">12-0093165</idno>
<date when="2011">2011</date>
<idno type="stanalyst">PASCAL 12-0093165 INIST</idno>
<idno type="RBID">Pascal:12-0093165</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000110</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Do high-energy neutrinos travel faster than photons in a discrete space-time?</title>
<author><name sortKey="Xue, She Sheng" sort="Xue, She Sheng" uniqKey="Xue S" first="She-Sheng" last="Xue">She-Sheng Xue</name>
<affiliation><inist:fA14 i1="01"><s1>ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza</s1>
<s2>Rome</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</analytic>
<series><title level="j" type="main">Physics letters. Section B</title>
<title level="j" type="abbreviated">Phys. lett., Sect. B</title>
<idno type="ISSN">0370-2693</idno>
<imprint><date when="2011">2011</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><title level="j" type="main">Physics letters. Section B</title>
<title level="j" type="abbreviated">Phys. lett., Sect. B</title>
<idno type="ISSN">0370-2693</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Asymmetry</term>
<term>Discrete space time</term>
<term>Elementary particles</term>
<term>Gauge symmetry</term>
<term>Local field</term>
<term>Massless particles</term>
<term>Neutrino interactions</term>
<term>Neutrino oscillations</term>
<term>Neutrinos</term>
<term>Operator</term>
<term>Parity</term>
<term>Parity conservation</term>
<term>Polarized electron</term>
<term>Quantum field theory</term>
<term>Quantum gravity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Neutrino</term>
<term>Espace temps discret</term>
<term>Gravitation quantique</term>
<term>Parité</term>
<term>Symétrie jauge</term>
<term>Champ local</term>
<term>Théorie quantique champ</term>
<term>Opérateur</term>
<term>Interaction neutrino</term>
<term>Oscillation neutrino</term>
<term>Conservation parité</term>
<term>Asymétrie</term>
<term>Electron polarisé</term>
<term>Particule sans masse</term>
<term>Particule élémentaire</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.</div>
</front>
</TEI>
<inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0370-2693</s0>
</fA01>
<fA02 i1="01"><s0>PYLBAJ</s0>
</fA02>
<fA03 i2="1"><s0>Phys. lett., Sect. B</s0>
</fA03>
<fA05><s2>706</s2>
</fA05>
<fA06><s2>2-3</s2>
</fA06>
<fA08 i1="01" i2="1" l="ENG"><s1>Do high-energy neutrinos travel faster than photons in a discrete space-time?</s1>
</fA08>
<fA11 i1="01" i2="1"><s1>XUE (She-Sheng)</s1>
</fA11>
<fA14 i1="01"><s1>ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza</s1>
<s2>Rome</s2>
<s3>ITA</s3>
<sZ>1 aut.</sZ>
</fA14>
<fA20><s1>213-218</s1>
</fA20>
<fA21><s1>2011</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA43 i1="01"><s1>INIST</s1>
<s2>9425B</s2>
<s5>354000508895920140</s5>
</fA43>
<fA44><s0>0000</s0>
<s1>© 2012 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45><s0>29 ref.</s0>
</fA45>
<fA47 i1="01" i2="1"><s0>12-0093165</s0>
</fA47>
<fA60><s1>P</s1>
</fA60>
<fA61><s0>A</s0>
</fA61>
<fA64 i1="01" i2="1"><s0>Physics letters. Section B</s0>
</fA64>
<fA66 i1="01"><s0>GBR</s0>
</fA66>
<fC01 i1="01" l="ENG"><s0>The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.</s0>
</fC01>
<fC02 i1="01" i2="3"><s0>001B00</s0>
</fC02>
<fC02 i1="02" i2="3"><s0>001B20</s0>
</fC02>
<fC02 i1="03" i2="3"><s0>001B10</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE"><s0>Neutrino</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG"><s0>Neutrinos</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="X" l="FRE"><s0>Espace temps discret</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="ENG"><s0>Discrete space time</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="SPA"><s0>Espacio tiempo discreto</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE"><s0>Gravitation quantique</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG"><s0>Quantum gravity</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE"><s0>Parité</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG"><s0>Parity</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="X" l="FRE"><s0>Symétrie jauge</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="X" l="ENG"><s0>Gauge symmetry</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="X" l="SPA"><s0>Simetría galga</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="X" l="FRE"><s0>Champ local</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="X" l="ENG"><s0>Local field</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="X" l="SPA"><s0>Campo local</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE"><s0>Théorie quantique champ</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG"><s0>Quantum field theory</s0>
<s5>32</s5>
</fC03>
<fC03 i1="08" i2="X" l="FRE"><s0>Opérateur</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="X" l="ENG"><s0>Operator</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="X" l="SPA"><s0>Operador</s0>
<s5>33</s5>
</fC03>
<fC03 i1="09" i2="3" l="FRE"><s0>Interaction neutrino</s0>
<s5>34</s5>
</fC03>
<fC03 i1="09" i2="3" l="ENG"><s0>Neutrino interactions</s0>
<s5>34</s5>
</fC03>
<fC03 i1="10" i2="3" l="FRE"><s0>Oscillation neutrino</s0>
<s5>35</s5>
</fC03>
<fC03 i1="10" i2="3" l="ENG"><s0>Neutrino oscillations</s0>
<s5>35</s5>
</fC03>
<fC03 i1="11" i2="X" l="FRE"><s0>Conservation parité</s0>
<s5>36</s5>
</fC03>
<fC03 i1="11" i2="X" l="ENG"><s0>Parity conservation</s0>
<s5>36</s5>
</fC03>
<fC03 i1="11" i2="X" l="SPA"><s0>Conservación paridad</s0>
<s5>36</s5>
</fC03>
<fC03 i1="12" i2="3" l="FRE"><s0>Asymétrie</s0>
<s5>37</s5>
</fC03>
<fC03 i1="12" i2="3" l="ENG"><s0>Asymmetry</s0>
<s5>37</s5>
</fC03>
<fC03 i1="13" i2="X" l="FRE"><s0>Electron polarisé</s0>
<s5>38</s5>
</fC03>
<fC03 i1="13" i2="X" l="ENG"><s0>Polarized electron</s0>
<s5>38</s5>
</fC03>
<fC03 i1="13" i2="X" l="SPA"><s0>Electrón polarizado</s0>
<s5>38</s5>
</fC03>
<fC03 i1="14" i2="3" l="FRE"><s0>Particule sans masse</s0>
<s5>39</s5>
</fC03>
<fC03 i1="14" i2="3" l="ENG"><s0>Massless particles</s0>
<s5>39</s5>
</fC03>
<fC03 i1="15" i2="3" l="FRE"><s0>Particule élémentaire</s0>
<s5>40</s5>
</fC03>
<fC03 i1="15" i2="3" l="ENG"><s0>Elementary particles</s0>
<s5>40</s5>
</fC03>
<fN21><s1>072</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
<server><NO>PASCAL 12-0093165 INIST</NO>
<ET>Do high-energy neutrinos travel faster than photons in a discrete space-time?</ET>
<AU>XUE (She-Sheng)</AU>
<AF>ICRANeT, Piazzale della Repubblica, 10-65122, Pescara, Physics Department, University of Rome "La Sapienza/Rome/Italie (1 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2011; Vol. 706; No. 2-3; Pp. 213-218; Bibl. 29 ref.</SO>
<LA>Anglais</LA>
<EA>The recent OPERA measurement of high-energy neutrino velocity, once independently verified, implies new physics in the neutrino sector. We revisit the theoretical inconsistency of the fundamental high-energy cutoff attributing to quantum gravity with the parity-violating gauge symmetry of local quantum field theory describing neutrinos. This inconsistency suggests high-dimension operators of neutrino interactions. Based on these studies, we try to view the OPERA result, high-energy neutrino oscillations and indicate to observe the restoration of parity conservation by measuring the asymmetry of high-energy neutrinos colliding with left- and right-handed polarized electrons.</EA>
<CC>001B00; 001B20; 001B10</CC>
<FD>Neutrino; Espace temps discret; Gravitation quantique; Parité; Symétrie jauge; Champ local; Théorie quantique champ; Opérateur; Interaction neutrino; Oscillation neutrino; Conservation parité; Asymétrie; Electron polarisé; Particule sans masse; Particule élémentaire</FD>
<ED>Neutrinos; Discrete space time; Quantum gravity; Parity; Gauge symmetry; Local field; Quantum field theory; Operator; Neutrino interactions; Neutrino oscillations; Parity conservation; Asymmetry; Polarized electron; Massless particles; Elementary particles</ED>
<SD>Espacio tiempo discreto; Simetría galga; Campo local; Operador; Conservación paridad; Electrón polarizado</SD>
<LO>INIST-9425B.354000508895920140</LO>
<ID>12-0093165</ID>
</server>
</inist>
</record>
Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Musique/explor/OperaV1/Data/PascalFrancis/Corpus
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000110 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Corpus/biblio.hfd -nk 000110 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien |wiki= Wicri/Musique |area= OperaV1 |flux= PascalFrancis |étape= Corpus |type= RBID |clé= Pascal:12-0093165 |texte= Do high-energy neutrinos travel faster than photons in a discrete space-time? }}
![]() | This area was generated with Dilib version V0.6.21. | ![]() |