PPT-The Sudbury Neutrino Observatory: Observation of Flavor Change for Solar Neutrinos.

Art McDonald Professor Emeritus Queens 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. From . Dark Matter . Annihilation. Jason Kumar. University of. H. a. w. a. i. i. collaborators. Jin In. Carsten. . Rott. Pearl Sandick. Jennifer Gaskins. David Yaylali. 1502. 02091, 15xx.xxxxx. dark matter and monoenergetic neutrinos. 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. :. past present future. Heidi Schellman @ Frank Merritt Fest 2015. 1. What we knew in 1971. 2. Neutrinos exist (Cowan, . Reines. 1956). There are two kinds (Lederman, Schwartz, Steinberger - 1962 ). eV. sterile neutrino production in the Early Universe . Based on . : . A. . Mirizzi. , N.S., G. . Miele. , P.D. . Serpico. ; . PRD . 86, 053009 (2012. ). . . Ninetta Saviano. II . Institut. . für. Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. R.Svoboda. Sterile Neutrinos as DM?. As WIMP searches getting well below the weak interaction scale for large range of masses and collider limits now limit smaller masses. What if no . WIMPs. are found to well below weak scale?. and Earth Structures. By . Miriam Aczel. What are neutrinos?. They are almost . massless. —hardly feel the force of gravity. They have no electric charge—don’t feel the electromagnetic force. Have no . Be . Majorana. States?. and Other Puzzlers Inspired by Adrian Melissinos. KT . McDonald. Princeton U. .. (March 7, 2017). Seminar at University . of Rochester. http://physics.princeton.edu/~. mcdonald/examples/majorana_170307.pptx. Ilias. . Savvidis. Aristotle University of Thessaloniki. Collaboration. I Savvidis. 1. , I Giomataris. 2. , E Bougamont. 2. , I Irastorza. 4. , S Aune. 2. , M Chapelier. 2. , Ph Charvin. 2. , P Colas. 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,. Neutrinos. Ghost . Particles . of the . Universe. Georg G. Raffelt. Max-Planck-Institut f. ür Physik, München, Germany. Neutron. Proton. Gravitation (Gravitons?) . Weak . Interaction (W and Z Bosons). Invites applications for SUMMER STUDENT POSITIONS 40 Hours Per Week For 8 weeks starting July $ 14 per hour The Youth in Policing Initiative (YIPI) is an employment program for youth 15 - 18 years of