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New and Improved Models of Radiative Neutrino Masses. K.S. Babu Oklahoma State University. From Majorana to LHC: Workshop on the Origin of Neutrino Mass ICTP, Trieste October 2-5, 2013. Outline. Minimal SO(10) as a theory of neutrino mass.
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New and Improved Models of Radiative Neutrino Masses K.S. Babu Oklahoma State University From Majorana to LHC: Workshop on the Origin of Neutrino Mass ICTP, Trieste October 2-5, 2013
Minimal SO(10) as a theory of neutrino mass Model has only 11 real parameters plus 7 phases Babu, Mohapatra (1993) Bajc, Senjanovic, Vissani (2002) Fukuyama, Okada (2002) Goh, Mohapatra, Ng (2003) Babu, Macesanu (2005) Bertolini, Malinsky, Schwetz (2006) Bajc, Dorsner, Nemevsek (2009) Joshipura, Patel (2012)
Testing SO(10) via Proton Decay Pati-Salam symmetry Mohapatra, Parida (1993) Deshpande, Keith, Pal (1995) Lee, Mohapatra, Parida, Rani (1995) Bertolini, Luzio, Malinsky (2012) Altarelli, Meloni (2013) Babu, Khan (2013)
Gauge coupling evolution in non-SUSY SO(10) Babu, Khan (2013)
Proton Lifetime in non-SUSY SO(10) Babu, Khan (2013)
S. Weinberg (1979) C.N. Leung, KSB (2003) For applications see: De Gouvea, Jenkins (2008) Angel, Rodd, Volkas (2012) Bonnet, Hirsch, Ota, Winter (2013)
Zee Model of Neutrino Mass A. Zee (1980)
L. Wolfenstein (1980) Smirnov, Tanimoto (1997) Jarlskog, Matsuda, Skaldhauge, Tanimoto (1999) Frampton, Glashow (1999)
Koide (2001) X.G. He (2004)
New Predictive Realization Babu, Julio (2013)
Gonzalez-Garcia et al (2012) Fogli et al (2012)
Zee, (1985) • Babu (1988)
Renormalization of the two—loop model K.S. Babu, J. Julio (2013)
LFV Predictions of Radiative Neutrino Mass Model K.S. Babu, J. Julio (2013)