BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Golden Elements of Flavor DTSTART;VALUE=DATE-TIME:20070718T080000Z DTEND;VALUE=DATE-TIME:20070718T090000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-18472@cern.ch DESCRIPTION:I argue that the observed flavour mixings in the quark and lep ton sector can be\nconstructed from a small number of textures - the eleme nts of flavour. The\nelements explaining the first two generation flavour physics are related to the\ngolden ratio. Consequently the solar neutrino and the Cabibbo mixing angles are\nnot arbitrary and can be predicted with high accuracy. The final KamLAND and SNO\nresults (expected to be releare d this summer) may prove/disprove this scenario.\n\nhttp://indico.cern.ch/ conferenceDisplay.py?confId=18472 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=18472 END:VEVENT BEGIN:VEVENT SUMMARY:Leptogenesis and low energy neutrino physics DTSTART;VALUE=DATE-TIME:20070925T090000Z DTEND;VALUE=DATE-TIME:20070925T100000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-21649@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=21649 LOCATION:CERN TH Theory Conference Room URL:http://indico.cern.ch/conferenceDisplay.py?confId=21649 END:VEVENT BEGIN:VEVENT SUMMARY:Probing non-standard neutrino interactions with supernova neutrino s DTSTART;VALUE=DATE-TIME:20071109T100000Z DTEND;VALUE=DATE-TIME:20071109T110000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-23316@cern.ch DESCRIPTION:Part 1: discussion of news in neutrino physics\nPart 2: prese ntation by Andreu Esteban-Pretel on "Probing non-standard neutrino interac tions with supernova neutrinos" \, arXiv:0704.0032\n\nhttp://indico.cern.c h/conferenceDisplay.py?confId=23316 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=23316 END:VEVENT BEGIN:VEVENT SUMMARY:Sensitivity of CNGS and J-PARC Beams to Quantum-Gravity Decoherenc e in Neutrino Oscillations DTSTART;VALUE=DATE-TIME:20080129T100000Z DTEND;VALUE=DATE-TIME:20080129T110000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-27418@cern.ch DESCRIPTION:Quantum decoherence\, the evolution of pure states into mixed states\, may\nbe a feature of quantum-gravity models. In most cases\, such models lead to\nfewer neutrinos of all active flavours being detected in a long baseline\nexperiment as compared to three-flavour standard neutrino oscillations. We\ndiscuss the potential of the CNGS and J-PARC beams in c onstraining models\nof quantum-gravity induced decoherence using neutrino oscillations as a\nprobe.\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=27418 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=27418 END:VEVENT BEGIN:VEVENT SUMMARY:A New class of invariants in the lepton sector DTSTART;VALUE=DATE-TIME:20080314T100000Z DTEND;VALUE=DATE-TIME:20080314T110000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-30394@cern.ch DESCRIPTION:1) discussion of neutrino related issues\n2) presentation by A rman Esmaili\, "A New class of invariants in the lepton sector"\n arXiv :0711.0448 [hep-ph]\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=3 0394 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=30394 END:VEVENT BEGIN:VEVENT SUMMARY:Testing dark matter with neutrino detectors DTSTART;VALUE=DATE-TIME:20080407T093000Z DTEND;VALUE=DATE-TIME:20080407T103000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-31781@cern.ch DESCRIPTION:1) discussion on neutrino related issues\;\n2) presentation by Sergio Palomares Ruiz on "Testing dark matter with neutrino detectors".\n \nhttp://indico.cern.ch/conferenceDisplay.py?confId=31781 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=31781 END:VEVENT BEGIN:VEVENT SUMMARY:NuSOnG DTSTART;VALUE=DATE-TIME:20080429T090000Z DTEND;VALUE=DATE-TIME:20080429T100000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-32667@cern.ch DESCRIPTION:1) discussion of various neutrino topics\n2) presentation of F . Olness on the NuSOnG proposal\, for a high-statistics TeV scale neutrino scattering experiment at Fermilab\, arXiv:0803.0354\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=32667 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=32667 END:VEVENT BEGIN:VEVENT SUMMARY:MiniBooNE Neutrino Oscillation Analyses DTSTART;VALUE=DATE-TIME:20080521T090000Z DTEND;VALUE=DATE-TIME:20080521T100000Z DTSTAMP;VALUE=DATE-TIME:20130525T185549Z UID:indico-event-34064@cern.ch DESCRIPTION:The LSND neutrino oscillation experiment\, performed in the 19 90s at Los Alamos National\nLaboratory\, USA\, observed an excess of elect ron anti-neutrino events best fit by a 2-neutrinooscillation hypothesis. This result\, in combination with the solar and atmospheric oscillation re sults\, cannot be accommodated by the Standard Model. MiniBooNE is an ex periment designed to confirm or refute the high-delta m^2 oscillations cla imed by LSND. InMarch\, 2007\, MiniBooNE presented the oscillation analys is result\, performed using a neutrino data sample. MiniBooNE's oscillati on result employed two complementary analyses. MiniBooNE found no evidenc e for oscillations from 475 MeV to 3 GeV in reconstructed neutrino energy. This talk will review the oscillation result and present two new oscillat ion analyses: one which combines the two complementary analyses for a stro nger limit\, and one which combines the LSND result with the three null se arches (MiniBooNE\, KARMEN2\, and Bugey).\n\nhttp://indico.cern.ch/confere nceDisplay.py?confId=34064 LOCATION:CERN 1-1-025 URL:http://indico.cern.ch/conferenceDisplay.py?confId=34064 END:VEVENT END:VCALENDAR