000192775 001__ 192775
000192775 005__ 20240227162144.0
000192775 0247_ $$2arXiv$$aarXiv:1411.4883
000192775 0247_ $$2altmetric$$aaltmetric:2901907
000192775 0247_ $$2inspire$$ainspire:1328649
000192775 037__ $$aPUBDB-2014-04304
000192775 0881_ $$aIFIC/14-76, arXiv:1411.4883
000192775 088__ $$2Other$$aIFIC/14-76
000192775 088__ $$2arXiv$$aarXiv:1411.4883
000192775 1001_ $$0P:(DE-HGF)0$$aBonilla, Cesar$$b0$$eCorresponding Author
000192775 245__ $$aRelating quarks and leptons with the T7 flavour group
000192775 260__ $$c2014
000192775 3367_ $$2DRIVER$$apreprint
000192775 3367_ $$028$$2EndNote$$aElectronic Article
000192775 3367_ $$0PUB:(DE-HGF)25$$2PUB:(DE-HGF)$$aPreprint$$bpreprint$$mpreprint$$s192775
000192775 3367_ $$2BibTeX$$aARTICLE
000192775 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep
000192775 500__ $$aOA
000192775 520__ $$aIn this letter we present a model for quarks and leptons based on T7 as flavour symmetry, predicting a canonical mass relation between charged leptons and down-type quarks proposed earlier. Neutrino masses are generated through a Type-I seesaw mechanism, with predicted correlations between the atmospheric mixing angle and neutrino masses. Compatibility with oscillation results lead to lower bounds for the lightest neutrino mass as well as for the neutrinoless double beta decay rates, even for normal neutrino mass hierarchy.
000192775 536__ $$0G:(DE-HGF)POF2-523$$a523 - High-energy gamma ray astronomy (POF2-523)$$cPOF2-523$$fPOF II$$x0
000192775 588__ $$aDataset connected to arXivarXiv
000192775 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000192775 7001_ $$0P:(DE-H253)PIP1021630$$aMorisi, Stefano$$b1$$udesy
000192775 7001_ $$0P:(DE-HGF)0$$aPeinado, Eduardo$$b2
000192775 7001_ $$0P:(DE-HGF)0$$aValle, Jose W. F.$$b3
000192775 8564_ $$yRestricted
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.pdf$$yOpenAccess
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.gif?subformat=icon$$xicon$$yOpenAccess
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.jpg?subformat=icon-700$$xicon-700$$yOpenAccess
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000192775 8564_ $$uhttps://bib-pubdb1.desy.de/record/192775/files/PUBDB-2014-04304.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000192775 909CO $$ooai:bib-pubdb1.desy.de:192775$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000192775 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1021630$$aDeutsches Elektronen-Synchrotron$$b1$$kDESY
000192775 9132_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
000192775 9131_ $$0G:(DE-HGF)POF2-523$$1G:(DE-HGF)POF2-520$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$aDE-HGF$$bStruktur der Materie$$lAstroteilchenphysik$$vHigh-energy gamma ray astronomy$$x0
000192775 9141_ $$y2014
000192775 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000192775 915__ $$0StatID:(DE-HGF)0580$$2StatID$$aPublished
000192775 9201_ $$0I:(DE-H253)Z_THAT-20210408$$kZ_THAT$$lTheoretische Astroteilchenphysik$$x0
000192775 980__ $$apreprint
000192775 980__ $$aVDB
000192775 980__ $$aUNRESTRICTED
000192775 980__ $$aFullTexts
000192775 980__ $$aintrep
000192775 980__ $$aI:(DE-H253)Z_THAT-20210408
000192775 9801_ $$aFullTexts