Superluminal neutrinos and extra dimensions: Constraints from the null energy condition
Identifieur interne : 000106 ( PascalFrancis/Corpus ); précédent : 000105; suivant : 000107Superluminal neutrinos and extra dimensions: Constraints from the null energy condition
Auteurs : Steven S. GubserSource :
- Physics letters. Section B [ 0370-2693 ] ; 2011.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
In light of the recent results from the OPERA Collaboration, indicating that neutrinos can travel superluminally, I review a simple extra-dimensional strategy for accommodating such behavior; and I also explain why it is hard in this strategy to avoid violating the null energy condition somewhere in the extra dimensions.
Notice en format standard (ISO 2709)
Pour connaître la documentation sur le format Inist Standard.
pA |
|
---|
Format Inist (serveur)
NO : | PASCAL 12-0146163 INIST |
---|---|
ET : | Superluminal neutrinos and extra dimensions: Constraints from the null energy condition |
AU : | GUBSER (Steven S.) |
AF : | Joseph Henry Laboratories, Princeton University/Princeton, NJ 08544/Etats-Unis (1 aut.) |
DT : | Publication en série; Niveau analytique |
SO : | Physics letters. Section B; ISSN 0370-2693; Coden PYLBAJ; Royaume-Uni; Da. 2011; Vol. 705; No. 3; Pp. 279-281; Bibl. 29 ref. |
LA : | Anglais |
EA : | In light of the recent results from the OPERA Collaboration, indicating that neutrinos can travel superluminally, I review a simple extra-dimensional strategy for accommodating such behavior; and I also explain why it is hard in this strategy to avoid violating the null energy condition somewhere in the extra dimensions. |
CC : | 001B00; 001B20; 001B10 |
FD : | Neutrino; Particule sans masse; Particule élémentaire |
ED : | Neutrinos; Massless particles; Elementary particles |
LO : | INIST-9425B.354000509225590210 |
ID : | 12-0146163 |
Links to Exploration step
Pascal:12-0146163Le document en format XML
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Superluminal neutrinos and extra dimensions: Constraints from the null energy condition</title>
<author><name sortKey="Gubser, Steven S" sort="Gubser, Steven S" uniqKey="Gubser S" first="Steven S." last="Gubser">Steven S. Gubser</name>
<affiliation><inist:fA14 i1="01"><s1>Joseph Henry Laboratories, Princeton University</s1>
<s2>Princeton, NJ 08544</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">12-0146163</idno>
<date when="2011">2011</date>
<idno type="stanalyst">PASCAL 12-0146163 INIST</idno>
<idno type="RBID">Pascal:12-0146163</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000106</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Superluminal neutrinos and extra dimensions: Constraints from the null energy condition</title>
<author><name sortKey="Gubser, Steven S" sort="Gubser, Steven S" uniqKey="Gubser S" first="Steven S." last="Gubser">Steven S. Gubser</name>
<affiliation><inist:fA14 i1="01"><s1>Joseph Henry Laboratories, Princeton University</s1>
<s2>Princeton, NJ 08544</s2>
<s3>USA</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>Elementary particles</term>
<term>Massless particles</term>
<term>Neutrinos</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Neutrino</term>
<term>Particule sans masse</term>
<term>Particule élémentaire</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">In light of the recent results from the OPERA Collaboration, indicating that neutrinos can travel superluminally, I review a simple extra-dimensional strategy for accommodating such behavior; and I also explain why it is hard in this strategy to avoid violating the null energy condition somewhere in the extra dimensions.</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>705</s2>
</fA05>
<fA06><s2>3</s2>
</fA06>
<fA08 i1="01" i2="1" l="ENG"><s1>Superluminal neutrinos and extra dimensions: Constraints from the null energy condition</s1>
</fA08>
<fA11 i1="01" i2="1"><s1>GUBSER (Steven S.)</s1>
</fA11>
<fA14 i1="01"><s1>Joseph Henry Laboratories, Princeton University</s1>
<s2>Princeton, NJ 08544</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
</fA14>
<fA20><s1>279-281</s1>
</fA20>
<fA21><s1>2011</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA43 i1="01"><s1>INIST</s1>
<s2>9425B</s2>
<s5>354000509225590210</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>12-0146163</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>In light of the recent results from the OPERA Collaboration, indicating that neutrinos can travel superluminally, I review a simple extra-dimensional strategy for accommodating such behavior; and I also explain why it is hard in this strategy to avoid violating the null energy condition somewhere in the extra dimensions.</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>Particule sans masse</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="3" l="ENG"><s0>Massless particles</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE"><s0>Particule élémentaire</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG"><s0>Elementary particles</s0>
<s5>28</s5>
</fC03>
<fN21><s1>114</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
<server><NO>PASCAL 12-0146163 INIST</NO>
<ET>Superluminal neutrinos and extra dimensions: Constraints from the null energy condition</ET>
<AU>GUBSER (Steven S.)</AU>
<AF>Joseph Henry Laboratories, Princeton University/Princeton, NJ 08544/Etats-Unis (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. 705; No. 3; Pp. 279-281; Bibl. 29 ref.</SO>
<LA>Anglais</LA>
<EA>In light of the recent results from the OPERA Collaboration, indicating that neutrinos can travel superluminally, I review a simple extra-dimensional strategy for accommodating such behavior; and I also explain why it is hard in this strategy to avoid violating the null energy condition somewhere in the extra dimensions.</EA>
<CC>001B00; 001B20; 001B10</CC>
<FD>Neutrino; Particule sans masse; Particule élémentaire</FD>
<ED>Neutrinos; Massless particles; Elementary particles</ED>
<LO>INIST-9425B.354000509225590210</LO>
<ID>12-0146163</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 000106 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Corpus/biblio.hfd -nk 000106 | 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:12-0146163 |texte= Superluminal neutrinos and extra dimensions: Constraints from the null energy condition }}
![]() | This area was generated with Dilib version V0.6.21. | ![]() |