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.

Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter

Identifieur interne : 000083 ( PascalFrancis/Checkpoint ); précédent : 000082; suivant : 000084

Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter

Auteurs : Ram Brustein [Israël, France, Allemagne] ; Dmitri Semikoz [France, Russie]

Source :

RBID : Pascal:12-0224573

Descripteurs français

English descriptors

Abstract

Quantum coherence can significantly increase the strength of the forward scattering of neutrinos propagating through the Earth and interacting with matter. The index of refraction of the neutrinos propagating in a medium and hence their phase velocity is determined by the forward scattering. So, depending on the nature of the interaction of neutrinos with matter, their phase velocity can be larger than the speed of light in vacuum. We show that such effects can explain the apparent superluminal propagation of muon neutrinos found recently by the OPERA experiment. Our proposal explains why the neutrino oscillations and the propagation of neutrinos from supernova 1987A are unaffected. It can be verified by changing the amount of neutrino coherence or by changing the composition of matter in which they propagate.


Affiliations:


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


Links to Exploration step

Pascal:12-0224573

Le document en format XML

<record>
<TEI>
<teiHeader>
<fileDesc>
<titleStmt>
<title xml:lang="en" level="a">Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter</title>
<author>
<name sortKey="Brustein, Ram" sort="Brustein, Ram" uniqKey="Brustein R" first="Ram" last="Brustein">Ram Brustein</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Department of Physics, Ben-Gurion University</s1>
<s2>Beer-Sheva 84105</s2>
<s3>ISR</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Israël</country>
<wicri:noRegion>Beer-Sheva 84105</wicri:noRegion>
</affiliation>
<affiliation wicri:level="3">
<inist:fA14 i1="02">
<s1>APC. 10 rue Alice Domon et Leonie Duquet</s1>
<s2>75205 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Paris</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="03">
<s1>CAS, Ludwig-Maximilians-Universität München</s1>
<s2>80333 München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="1">Bavière</region>
<region type="district" nuts="2">District de Haute-Bavière</region>
<settlement type="city">Munich</settlement>
</placeName>
<orgName type="university">Université Louis-et-Maximilien de Munich</orgName>
</affiliation>
</author>
<author>
<name sortKey="Semikoz, Dmitri" sort="Semikoz, Dmitri" uniqKey="Semikoz D" first="Dmitri" last="Semikoz">Dmitri Semikoz</name>
<affiliation wicri:level="3">
<inist:fA14 i1="02">
<s1>APC. 10 rue Alice Domon et Leonie Duquet</s1>
<s2>75205 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Paris</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="04">
<s1>INR RAS. 60th October Anniversary pr. 7a</s1>
<s2>117312 Moscow</s2>
<s3>RUS</s3>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>Russie</country>
<placeName>
<settlement type="city">Moscou</settlement>
<region>District fédéral central</region>
</placeName>
</affiliation>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">INIST</idno>
<idno type="inist">12-0224573</idno>
<date when="2012">2012</date>
<idno type="stanalyst">PASCAL 12-0224573 INIST</idno>
<idno type="RBID">Pascal:12-0224573</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000094</idno>
<idno type="wicri:Area/PascalFrancis/Curation">000432</idno>
<idno type="wicri:Area/PascalFrancis/Checkpoint">000083</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title xml:lang="en" level="a">Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter</title>
<author>
<name sortKey="Brustein, Ram" sort="Brustein, Ram" uniqKey="Brustein R" first="Ram" last="Brustein">Ram Brustein</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Department of Physics, Ben-Gurion University</s1>
<s2>Beer-Sheva 84105</s2>
<s3>ISR</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Israël</country>
<wicri:noRegion>Beer-Sheva 84105</wicri:noRegion>
</affiliation>
<affiliation wicri:level="3">
<inist:fA14 i1="02">
<s1>APC. 10 rue Alice Domon et Leonie Duquet</s1>
<s2>75205 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Paris</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="03">
<s1>CAS, Ludwig-Maximilians-Universität München</s1>
<s2>80333 München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="1">Bavière</region>
<region type="district" nuts="2">District de Haute-Bavière</region>
<settlement type="city">Munich</settlement>
</placeName>
<orgName type="university">Université Louis-et-Maximilien de Munich</orgName>
</affiliation>
</author>
<author>
<name sortKey="Semikoz, Dmitri" sort="Semikoz, Dmitri" uniqKey="Semikoz D" first="Dmitri" last="Semikoz">Dmitri Semikoz</name>
<affiliation wicri:level="3">
<inist:fA14 i1="02">
<s1>APC. 10 rue Alice Domon et Leonie Duquet</s1>
<s2>75205 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Paris</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="04">
<s1>INR RAS. 60th October Anniversary pr. 7a</s1>
<s2>117312 Moscow</s2>
<s3>RUS</s3>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>Russie</country>
<placeName>
<settlement type="city">Moscou</settlement>
<region>District fédéral central</region>
</placeName>
</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="2012">2012</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>Elementary particles</term>
<term>Forward scattering</term>
<term>Light velocity</term>
<term>Massless particles</term>
<term>Muon neutrinos</term>
<term>Neutrino interactions</term>
<term>Neutrino oscillations</term>
<term>Neutrino scattering</term>
<term>Phase velocity</term>
<term>Quantum coherence</term>
<term>Refractive index</term>
<term>Supernovae</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Neutrino muonique</term>
<term>Cohérence quantique</term>
<term>Diffusion avant</term>
<term>Diffusion neutrino</term>
<term>Indice réfraction</term>
<term>Vitesse phase</term>
<term>Interaction neutrino</term>
<term>Vitesse lumière</term>
<term>Oscillation neutrino</term>
<term>Supernova</term>
<term>Particule sans masse</term>
<term>Particule élémentaire</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Particule élémentaire</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Quantum coherence can significantly increase the strength of the forward scattering of neutrinos propagating through the Earth and interacting with matter. The index of refraction of the neutrinos propagating in a medium and hence their phase velocity is determined by the forward scattering. So, depending on the nature of the interaction of neutrinos with matter, their phase velocity can be larger than the speed of light in vacuum. We show that such effects can explain the apparent superluminal propagation of muon neutrinos found recently by the OPERA experiment. Our proposal explains why the neutrino oscillations and the propagation of neutrinos from supernova 1987A are unaffected. It can be verified by changing the amount of neutrino coherence or by changing the composition of matter in which they propagate.</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>4-5</s2>
</fA06>
<fA08 i1="01" i2="1" l="ENG">
<s1>Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter</s1>
</fA08>
<fA11 i1="01" i2="1">
<s1>BRUSTEIN (Ram)</s1>
</fA11>
<fA11 i1="02" i2="1">
<s1>SEMIKOZ (Dmitri)</s1>
</fA11>
<fA14 i1="01">
<s1>Department of Physics, Ben-Gurion University</s1>
<s2>Beer-Sheva 84105</s2>
<s3>ISR</s3>
<sZ>1 aut.</sZ>
</fA14>
<fA14 i1="02">
<s1>APC. 10 rue Alice Domon et Leonie Duquet</s1>
<s2>75205 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</fA14>
<fA14 i1="03">
<s1>CAS, Ludwig-Maximilians-Universität München</s1>
<s2>80333 München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
</fA14>
<fA14 i1="04">
<s1>INR RAS. 60th October Anniversary pr. 7a</s1>
<s2>117312 Moscow</s2>
<s3>RUS</s3>
<sZ>2 aut.</sZ>
</fA14>
<fA20>
<s1>462-464</s1>
</fA20>
<fA21>
<s1>2012</s1>
</fA21>
<fA23 i1="01">
<s0>ENG</s0>
</fA23>
<fA43 i1="01">
<s1>INIST</s1>
<s2>9425B</s2>
<s5>354000509343070340</s5>
</fA43>
<fA44>
<s0>0000</s0>
<s1>© 2012 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45>
<s0>13 ref.</s0>
</fA45>
<fA47 i1="01" i2="1">
<s0>12-0224573</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>Quantum coherence can significantly increase the strength of the forward scattering of neutrinos propagating through the Earth and interacting with matter. The index of refraction of the neutrinos propagating in a medium and hence their phase velocity is determined by the forward scattering. So, depending on the nature of the interaction of neutrinos with matter, their phase velocity can be larger than the speed of light in vacuum. We show that such effects can explain the apparent superluminal propagation of muon neutrinos found recently by the OPERA experiment. Our proposal explains why the neutrino oscillations and the propagation of neutrinos from supernova 1987A are unaffected. It can be verified by changing the amount of neutrino coherence or by changing the composition of matter in which they propagate.</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 muonique</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG">
<s0>Muon neutrinos</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="X" l="FRE">
<s0>Cohérence quantique</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="ENG">
<s0>Quantum coherence</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="SPA">
<s0>Coherencia cuántica</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="X" l="FRE">
<s0>Diffusion avant</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="X" l="ENG">
<s0>Forward scattering</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="X" l="SPA">
<s0>Difusión hacia adelante</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE">
<s0>Diffusion neutrino</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG">
<s0>Neutrino scattering</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE">
<s0>Indice réfraction</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG">
<s0>Refractive index</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="3" l="FRE">
<s0>Vitesse phase</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="3" l="ENG">
<s0>Phase velocity</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE">
<s0>Interaction neutrino</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG">
<s0>Neutrino interactions</s0>
<s5>32</s5>
</fC03>
<fC03 i1="08" i2="3" l="FRE">
<s0>Vitesse lumière</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="3" l="ENG">
<s0>Light velocity</s0>
<s5>33</s5>
</fC03>
<fC03 i1="09" i2="3" l="FRE">
<s0>Oscillation neutrino</s0>
<s5>34</s5>
</fC03>
<fC03 i1="09" i2="3" l="ENG">
<s0>Neutrino oscillations</s0>
<s5>34</s5>
</fC03>
<fC03 i1="10" i2="3" l="FRE">
<s0>Supernova</s0>
<s5>35</s5>
</fC03>
<fC03 i1="10" i2="3" l="ENG">
<s0>Supernovae</s0>
<s5>35</s5>
</fC03>
<fC03 i1="11" i2="3" l="FRE">
<s0>Particule sans masse</s0>
<s5>36</s5>
</fC03>
<fC03 i1="11" i2="3" l="ENG">
<s0>Massless particles</s0>
<s5>36</s5>
</fC03>
<fC03 i1="12" i2="3" l="FRE">
<s0>Particule élémentaire</s0>
<s5>37</s5>
</fC03>
<fC03 i1="12" i2="3" l="ENG">
<s0>Elementary particles</s0>
<s5>37</s5>
</fC03>
<fN21>
<s1>170</s1>
</fN21>
<fN44 i1="01">
<s1>OTO</s1>
</fN44>
<fN82>
<s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
<affiliations>
<list>
<country>
<li>Allemagne</li>
<li>France</li>
<li>Israël</li>
<li>Russie</li>
</country>
<region>
<li>Bavière</li>
<li>District de Haute-Bavière</li>
<li>District fédéral central</li>
<li>Île-de-France</li>
</region>
<settlement>
<li>Moscou</li>
<li>Munich</li>
<li>Paris</li>
</settlement>
<orgName>
<li>Université Louis-et-Maximilien de Munich</li>
</orgName>
</list>
<tree>
<country name="Israël">
<noRegion>
<name sortKey="Brustein, Ram" sort="Brustein, Ram" uniqKey="Brustein R" first="Ram" last="Brustein">Ram Brustein</name>
</noRegion>
</country>
<country name="France">
<region name="Île-de-France">
<name sortKey="Brustein, Ram" sort="Brustein, Ram" uniqKey="Brustein R" first="Ram" last="Brustein">Ram Brustein</name>
</region>
<name sortKey="Semikoz, Dmitri" sort="Semikoz, Dmitri" uniqKey="Semikoz D" first="Dmitri" last="Semikoz">Dmitri Semikoz</name>
</country>
<country name="Allemagne">
<region name="Bavière">
<name sortKey="Brustein, Ram" sort="Brustein, Ram" uniqKey="Brustein R" first="Ram" last="Brustein">Ram Brustein</name>
</region>
</country>
<country name="Russie">
<region name="District fédéral central">
<name sortKey="Semikoz, Dmitri" sort="Semikoz, Dmitri" uniqKey="Semikoz D" first="Dmitri" last="Semikoz">Dmitri Semikoz</name>
</region>
</country>
</tree>
</affiliations>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Wicri/Musique/explor/OperaV1/Data/PascalFrancis/Checkpoint
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000083 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Checkpoint/biblio.hfd -nk 000083 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Wicri/Musique
   |area=    OperaV1
   |flux=    PascalFrancis
   |étape=   Checkpoint
   |type=    RBID
   |clé=     Pascal:12-0224573
   |texte=   Apparent superluminal neutrino propagation caused by nonlinear coherent interactions in matter
}}

Wicri

This area was generated with Dilib version V0.6.21.
Data generation: Thu Apr 14 14:59:05 2016. Site generation: Thu Jan 4 23:09:23 2024