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. 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. Early Cosmologies. Sections 1.1-1.2. Reminders. Reading quiz for Chapter 1, Sections 3 and 4, due on Mallard prior to start of next class.. Weekly reflection #1 will be sent via email later today and will be due via email prior to start of class on Tuesday.. 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). .  . By Isabella . Ferrufino. William . Sinz. . Zixuan. . Zhao. Monica . Raubusch. Abstract. For Disability and Safety . Existing condition . Preferred condition . Methodology. Data analysis . mass. Stuart . Freedman memorial symposium. Berkeley, Jan 11, 2014. Hamish Robertson, University of Washington. a long wait for a little weight. 2. Neutrinos oscillate, have mass. Super-. Kamiokande. Portfolios with Seesaw. Kirsten Lofton. kyhatch@episd.org. Twitter: @kirstenteaches. QR Code Link to Presentation. http://tinyurl.com/TCEA2016Seesaw. About Me. My Family. 18th year in education. Taught K, 1, 2, 6, 7. 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 . 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,. Members include:. B.J. Byers, Matt “Brown” Brown and Thomas Thurman. Dumbo’s. Light Switch. Energy Conversions. Book starts at a rested position falls on 1. st. seesaw. Mass of falling book raises Flying elephant on 1. The Digital Learning Journal. Seesaw allows students of any age the ability to document their learning.. What’s this presentation about? Use this slide to introduce yourself and give a high level overview of the topic you’re about to explain.. 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.. http://www.darkenergysurvey.org. . . . Outline. DES: what is it and update + probes used. Dark energy from DES.. Neutrino masses from DES. Filipe . Batoni. . Abdalla. Future Dark Energy Surveys.