OperaV1, PascalFrancis, Corpus, bibRecord, 000102

Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity

Identifieur interne : 000102 ( PascalFrancis/Corpus ); précédent : 000101; suivant : 000103

Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity

Auteurs : ZHECHANG ; XIN LI ; SAI WANG

Source :

Physics letters. Section B [ 0370-2693 ] ; 2012.

RBID : Pascal:12-0177136

Descripteurs français

Pascal (Inist)
- Neutrino, Relativité restreinte, Principe relativité, Causalité, Conservation énergie, Particule sans masse, Particule élémentaire.

English descriptors

KwdEn :
- Causality, Elementary particles, Energy conservation, Massless particles, Neutrinos, Relativity principle, Special relativity.

Abstract

Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

A01	`01`	`1`		`@0 0370-2693`
A02	`01`			`@0 PYLBAJ`
A03		`1`		`@0 Phys. lett., Sect. B`
A05				`@2 710`
A06				`@2 3`
A08	`01`	`1`	`ENG`	`@1 Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity`
A11	`01`	`1`		`@1 ZHECHANG`
A11	`02`	`1`		`@1 XIN LI`
A11	`03`	`1`		`@1 SAI WANG`
A14	`01`			`@1 Institute of High Energy Physics, Chinese Academy of Sciences @2 100049 Beijing @3 CHN @Z 1 aut. @Z 2 aut. @Z 3 aut.`
A14	`02`			`@1 Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences @2 100049 Beijing @3 CHN @Z 1 aut. @Z 2 aut. @Z 3 aut.`
A20				`@1 430-434`
A21				`@1 2012`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 9425B @5 354000509647830050`
A44				`@0 0000 @1 © 2012 INIST-CNRS. All rights reserved.`
A45				`@0 26 ref.`
A47	`01`	`1`		`@0 12-0177136`
A60				`@1 P`
A61				`@0 A`
A64	`01`	`1`		`@0 Physics letters. Section B`
A66	`01`			`@0 GBR`
C01	`01`		`ENG`	@0 Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.
C02	`01`	`3`		`@0 001B00`
C02	`02`	`3`		`@0 001B20`
C02	`03`	`3`		`@0 001B10`
C03	`01`	`3`	`FRE`	`@0 Neutrino @5 26`
C03	`01`	`3`	`ENG`	`@0 Neutrinos @5 26`
C03	`02`	`3`	`FRE`	`@0 Relativité restreinte @5 27`
C03	`02`	`3`	`ENG`	`@0 Special relativity @5 27`
C03	`03`	`X`	`FRE`	`@0 Principe relativité @5 28`
C03	`03`	`X`	`ENG`	`@0 Relativity principle @5 28`
C03	`03`	`X`	`SPA`	`@0 Principio relatividad @5 28`
C03	`04`	`3`	`FRE`	`@0 Causalité @5 29`
C03	`04`	`3`	`ENG`	`@0 Causality @5 29`
C03	`05`	`3`	`FRE`	`@0 Conservation énergie @5 30`
C03	`05`	`3`	`ENG`	`@0 Energy conservation @5 30`
C03	`06`	`3`	`FRE`	`@0 Particule sans masse @5 31`
C03	`06`	`3`	`ENG`	`@0 Massless particles @5 31`
C03	`07`	`3`	`FRE`	`@0 Particule élémentaire @5 32`
C03	`07`	`3`	`ENG`	`@0 Elementary particles @5 32`
N21				`@1 135`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

Format Inist (serveur)

NO :	PASCAL 12-0177136 INIST
ET :	Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity
AU :	ZHECHANG; XIN LI; SAI WANG
AF :	Institute of High Energy Physics, Chinese Academy of Sciences/100049 Beijing/Chine (1 aut., 2 aut., 3 aut.); Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences/100049 Beijing/Chine (1 aut., 2 aut., 3 aut.)
DT :	Publication en série; Niveau analytique
SO :	Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2012; Vol. 710; No. 3; Pp. 430-434; Bibl. 26 ref.
LA :	Anglais
EA :	Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.
CC :	001B00; 001B20; 001B10
FD :	Neutrino; Relativité restreinte; Principe relativité; Causalité; Conservation énergie; Particule sans masse; Particule élémentaire
ED :	Neutrinos; Special relativity; Relativity principle; Causality; Energy conservation; Massless particles; Elementary particles
SD :	Principio relatividad
LO :	INIST-9425B.354000509647830050
ID :	12-0177136

Links to Exploration step

Pascal:12-0177136

Le document en format XML

<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity</title>
<author><name sortKey="Zhechang" sort="Zhechang" uniqKey="Zhechang" last="Zhechang">ZHECHANG</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Xin Li" sort="Xin Li" uniqKey="Xin Li" last="Xin Li">XIN LI</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Sai Wang" sort="Sai Wang" uniqKey="Sai Wang" last="Sai Wang">SAI WANG</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">12-0177136</idno>
<date when="2012">2012</date>
<idno type="stanalyst">PASCAL 12-0177136 INIST</idno>
<idno type="RBID">Pascal:12-0177136</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000102</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity</title>
<author><name sortKey="Zhechang" sort="Zhechang" uniqKey="Zhechang" last="Zhechang">ZHECHANG</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Xin Li" sort="Xin Li" uniqKey="Xin Li" last="Xin Li">XIN LI</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Sai Wang" sort="Sai Wang" uniqKey="Sai Wang" last="Sai Wang">SAI WANG</name>
<affiliation><inist:fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
<affiliation><inist:fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 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="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>Causality</term>
<term>Elementary particles</term>
<term>Energy conservation</term>
<term>Massless particles</term>
<term>Neutrinos</term>
<term>Relativity principle</term>
<term>Special relativity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Neutrino</term>
<term>Relativité restreinte</term>
<term>Principe relativité</term>
<term>Causalité</term>
<term>Conservation énergie</term>
<term>Particule sans masse</term>
<term>Particule élémentaire</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.</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>710</s2>
</fA05>
<fA06><s2>3</s2>
</fA06>
<fA08 i1="01" i2="1" l="ENG"><s1>Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity</s1>
</fA08>
<fA11 i1="01" i2="1"><s1>ZHECHANG</s1>
</fA11>
<fA11 i1="02" i2="1"><s1>XIN LI</s1>
</fA11>
<fA11 i1="03" i2="1"><s1>SAI WANG</s1>
</fA11>
<fA14 i1="01"><s1>Institute of High Energy Physics, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</fA14>
<fA14 i1="02"><s1>Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences</s1>
<s2>100049 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</fA14>
<fA20><s1>430-434</s1>
</fA20>
<fA21><s1>2012</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA43 i1="01"><s1>INIST</s1>
<s2>9425B</s2>
<s5>354000509647830050</s5>
</fA43>
<fA44><s0>0000</s0>
<s1>© 2012 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45><s0>26 ref.</s0>
</fA45>
<fA47 i1="01" i2="1"><s0>12-0177136</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>Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.</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="3" l="FRE"><s0>Relativité restreinte</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="3" l="ENG"><s0>Special relativity</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="X" l="FRE"><s0>Principe relativité</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="X" l="ENG"><s0>Relativity principle</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="X" l="SPA"><s0>Principio relatividad</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE"><s0>Causalité</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG"><s0>Causality</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE"><s0>Conservation énergie</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG"><s0>Energy conservation</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="3" l="FRE"><s0>Particule sans masse</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="3" l="ENG"><s0>Massless particles</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE"><s0>Particule élémentaire</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG"><s0>Elementary particles</s0>
<s5>32</s5>
</fC03>
<fN21><s1>135</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
<server><NO>PASCAL 12-0177136 INIST</NO>
<ET>Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity</ET>
<AU>ZHECHANG; XIN LI; SAI WANG</AU>
<AF>Institute of High Energy Physics, Chinese Academy of Sciences/100049 Beijing/Chine (1 aut., 2 aut., 3 aut.); Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences/100049 Beijing/Chine (1 aut., 2 aut., 3 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2012; Vol. 710; No. 3; Pp. 430-434; Bibl. 26 ref.</SO>
<LA>Anglais</LA>
<EA>Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. 107 (2011) 181803] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The Cherenkov-like process for the superluminal particles would be forbidden if the principle of special relativity holds in any frame instead violated with a preferred frame. We have proposed that the Finslerian special relativity could account for the data of the neutrino superluminality (arXiv:1110.6673 [hep-ph]). The Finslerian special relativity preserves the principle of special relativity and involves a preferred direction while consists with the causality. In this Letter, we prove that the energy-momentum conservation is preserved and the energy-momentum is well defined in Finslerian special relativity. The Cherenkov-like process is forbidden in the Finslerian special relativity. Thus, the superluminal neutrinos would not lose energy in their distant propagation.</EA>
<CC>001B00; 001B20; 001B10</CC>
<FD>Neutrino; Relativité restreinte; Principe relativité; Causalité; Conservation énergie; Particule sans masse; Particule élémentaire</FD>
<ED>Neutrinos; Special relativity; Relativity principle; Causality; Energy conservation; Massless particles; Elementary particles</ED>
<SD>Principio relatividad</SD>
<LO>INIST-9425B.354000509647830050</LO>
<ID>12-0177136</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 000102 | SxmlIndent | more

HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Corpus/biblio.hfd -nk 000102 | 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:12-0177136
   |texte=   Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity
}}

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

	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.

Serveur d'exploration sur l'opéra

Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity

Neutrino superluminality without Cherenkov-like processes in Finslerian special relativity

Source :

Descripteurs français

English descriptors

Abstract

Notice en format standard (ISO 2709)

Format Inist (serveur)

Links to Exploration step

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri