PPT-Seesaw neutrino models and their motions in lepton flavor space

Rome Samanta University of Southampton Neutrino masses and mixing SM heavy RH neutrinos Matter anti matter asymmetry Baryogenesis via leptogenesis Seesaw. YASAMAN FARZAN. IPM, Tehran. This talk is based on. Y. F., JHEP 0707 (07) 54 . ;. Ayazi. and . Farzan. , JHEP 0901:022,2009. ;. Y.F. , PLB677. ;. Y.F. And . Saereh. . Najjari. , . arXiv. : 1001.3207 , to appear in PLB. Oscillations. Collective Neutrino Oscillations. Georg G. Raffelt. 3. rd. Schr. ödinger Lecture, Thursday 19 May 2011. Neutrino Oscillations in Matter. 3300 citations. Lincoln Wolfenstein. Neutrinos in a medium suffer . Neutrino . L. imits. Georg G. Raffelt, Max-Planck-Institut f. ür Physik, München. Sun. Globular Cluster. Supernova 1987A. Cosmology. Questions about Neutrinos. Standard properties of active neutrinos. (photoelectric effect), . light scattered . (Compton) . like particle →Photon . γ. Elecrodynamics. : field →. exchage. particle. . (mediator; . photon. ). 뉴트리노에. and. PAMELA/Fermi LAT Signals. Toshifumi Yamada. Sokendai, KEK. In collaboration with . Ilia. Gogoladze, Qaisar Shafi (Univ. of Delaware) and Nobuchika Okada (Univ. of Alabama). Atsushi WATANABE. Niigata Univ. & . The . Max-Planck-Institute . for Nuclear Physics. 23. rd. February 2011 @. HRI, Allahabad. . Based on the work with . K. Yoshioka (Kyoto Univ.). , . H. . Ishimori. epton asymmetry in. . the. . 3-3-1 . model. . with. . right-handed. neutrinos. N. T. . Thuy. Yonsei. University. Jindo. Workshop. , Sep . 20~23, . 2012. 1. O. utline. I. . Introduction. II. . A review of the model. Neutrino Flavor Conversion. in Supernovae. Georg Raffelt, Max-Planck-Institut . f. ür Physik, . München. Core-Collapse Supernova Explosion. Neutrino. cooling by. diffusion. End state of a. massive star. R. e. l. d. The. d. i. A. Yu. Smirnov. Max-Planck Institute. for Nuclear Physics,. Heidelberg, Germany . NOW 2014 . September 8– 13, 2014 . . The riddle of neutrino mass:. strongly suppresses . Leptogenesis. University of Maryland. Department of Physics. Chang-Hun Lee. P.S. . Bhupal. Dev, C.-H. Lee, R.N. . Mohapatra. , . Phys.Rev. . D90 (2014) 9, . 095012. P.S. . Bhupal. Dev, C.-H. Lee, R.N. . Art McDonald, Professor Emeritus. Queen’s University, Kingston, . Ontario, Canada. T. he middle of the sun is so hot that the centers of the atoms (nuclei). f. use together, giving off lots of energy and neutrinos. The neutrinos penetrate easily through the dense material in the Sun and reach the earth.. ass: Facts and Fancy. Francesco Vissani. LNGS and GSSI. Introduction. Baryon and lepton numbers and their status in the standard model of particles and interactions. L. epton and baryon number. In all known transformations among particles,. Michael Schmitt. Northwestern University. COFI Workshop. May 22, 2018. May 22, 2018. LFV at the LHC. 1. May 22, 2018. LFV at the LHC. 2. This talk is not about the fascinating observations in B decays.. will we ever know?. Ray Volkas. School of Physics. The University of Melbourne. CERN Theory Colloquium at “Neutrinos: the quest for a new physics scale”, 29 March 2017.. What we know, don’t know and want to know..