CERN Accélérateur de science

002315300 001__ 2315300
002315300 003__ SzGeCERN
002315300 005__ 20180427220015.0
002315300 0248_ $$aoai:inspirehep.net:1666759$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002315300 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1666759$$d2018-04-26T13:43:31Z$$h2018-04-27T04:00:10Z$$mmarcxml
002315300 035__ $$9Inspire$$a1666759
002315300 041__ $$aeng
002315300 100__ $$aFuentes-Martin, Javier$$uValencia U., IFIC$$vUniversitat deVaì encia – CSIC
002315300 245__ $$ab → ss + − anomalies from dynamical Yukawas
002315300 260__ $$c2017
002315300 300__ $$a4 p
002315300 520__ $$9Grobid$$aThe LHCb Collaboration has recently reported hints for New Physics in b → ss + −
transitions that point to a large violation of flavor universality in the lepton
sector. Motivated by them, we present a framework able to accommodate the
experimental anomalies while, at the same time, addressing the flavor puzzle of
the Standard Model. This framework is based on the hypothesis of dynamical
Yukawas, where it is assumed that these couplings are generated by the vacuum
expectation value of dynamical fields charged under a local non-Abelian flavor
symmetry. The proposed framework has a rich phenomenology and predicts striking
collider signatures that will be tested in the near future.
002315300 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002315300 690C_ $$aCERN
002315300 773__ $$01643132$$c461-464$$wC17-03-18$$y2017$$z9791096879021
002315300 8564_ $$81399840$$s865472$$uhttps://cds.cern.ch/record/2315300/files/1643132_461-464.pdf$$yFulltext
002315300 960__ $$a13
002315300 962__ $$b2232276$$k461-464$$nlathuile20170318
002315300 980__ $$aARTICLE
002315300 980__ $$aConferencePaper
002315300 999C6 $$a0-1-0-0-0-0-0$$t2018-04-09 18:32:53$$vcontent.pdf;1$$vInvenio/1.1.2.1260-aa76f refextract/1.5.44
002315300 999C5 $$01409497$$hR. Aaij et al.$$m[LHCb Collaboration]$$o1$$rarXiv:1512.04442 [hep-ex]$$sJHEP,1602,104$$y2016
002315300 999C5 $$01504055$$cBelle Collaboration$$hS. Wehle et al.$$o2$$rarXiv:1612.05014 [hep-ex]$$sPhys.Rev.Lett.,118,111801$$y2017
002315300 999C5 $$01380188$$hR. Aaij et al.$$m[LHCb Collaboration]$$o3$$rarXiv:1506.08777 [hep-ex]$$sJHEP,1509,179$$y2015
002315300 999C5 $$01303108$$hR. Aaij et al.$$m[LHCb Collaboration]$$o4$$rarXiv:1406.6482 [hep-ex]$$sPhys.Rev.Lett.,113,151601$$y2014
002315300 999C5 $$01465646$$hM. Bordone, G. Isidori and A. Pattori$$o5$$rarXiv:1605.07633 [hep-ph]$$sEur.Phys.J.,C76,440$$y2016
002315300 999C5 $$01599846$$hR. Aaij et al.$$m[LHCb Collaboration]$$o6$$rarXiv:1705.05802 [hep-ex]
002315300 999C5 $$01591975$$hB. Capdevila, A. Crivellin, S. Descotes-Genon, J. Matias and J. Virto$$o7$$rarXiv:1704.05340 [hep-ph]
002315300 999C5 $$01592392$$hA. Celis, J. Fuentes-Martin, A. Vicente and J. Virto$$o8$$rarXiv:1704.05672 [hep-ph]
002315300 999C5 $$01369342$$hA. Celis, J. Fuentes-Martin, M. Jung and H. Serodio$$o9$$rarXiv:1505.03079 [hep-ph]$$sPhys.Rev.,D92,015007$$y2015
002315300 999C5 $$01496640$$hA. Crivellin, J. Fuentes-Martin, A. Greljo and G. Isidori$$o10$$rarXiv:1611.02703 [hep-ph]$$sPhys.Lett.,B766,77$$y2017
002315300 999C5 $$01239849$$hR. Alonso, M. B. Gavela, G. Isidori and L. Maiani$$o11$$rarXiv:1306.5927 [hep-ph]$$sJHEP,1311,187$$y2013
002315300 999C5 $$0892710$$hR. Alonso, M. B. Gavela, L. Merlo and S. Rigolin$$o12$$rarXiv:1103.2915 [hep-ph]$$sJHEP,1107,012$$y2011
002315300 999C5 $$01243170$$hC. S. Fong and E. Nardi$$o13$$rarXiv:1307.4412 [hep-ph]$$sPhys.Rev.,D89,036008$$y2014
002315300 999C5 $$0313939$$hS. R. Mishra et al.$$m[CCFR Collaboration]$$o14$$sPhys.Rev.Lett.,66,3117$$y1991
002315300 999C5 $$01296830$$cATLAS Collaboration$$hG. Aad et al.$$o15$$rarXiv:1405.4123 [hep-ex]$$sPhys.Rev.,D90,052005$$y2014
002315300 999C5 $$01480025$$cATLAS collaboration$$o16$$rATLAS-CONF-2016-045