PPT-Are we close to measuring the neutrino hierarchy?
Author : briana-ranney | Published Date : 2020-01-14
Are we close to measuring the neutrino hierarchy Filipe B Abdalla ν Loureiro Moraes Abdalla et al arXiv180907204 Loureiro Cuceu Abdalla et al arXiv181102578
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Are we close to measuring the neutrino hierarchy?: Transcript
Are we close to measuring the neutrino hierarchy Filipe B Abdalla ν Loureiro Moraes Abdalla et al arXiv180907204 Loureiro Cuceu Abdalla et al arXiv181102578 Outline Cosmology background. Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. 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 . Direct Influence. Three Degrees of Influence. Alter Influence Persists. Alter. ’. s Alter Influence Persists. Period 1. Eleni. Lucas. Lucas. Lysander. Erika. Erika. Harla. Erika. James. Jay. Brecken. :. 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 ). Satoshi Nakamura. Osaka University, Japan. Collaborators : H. . Kamano. (RCNP, Osaka Univ.), T. Sato (Osaka Univ.). T.-S.H. Lee (Argonne Nat’l Lab). Contents. Introduction . J. Brunner. 17/04/2013. APC. Outline. Oscillation Probabilities. Neutrino Cross Sections. The Proton Accelerator . The Neutrino Beam. Detector Performance. Event Rates / Result. Oscillation Probabilities. 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). COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HANNESTAD, Aarhus . University. NuHorizons. 2011. n. e. n. m. n. t. Fermion Mass Spectrum. 10. 100. 1. 10. 100. 1. 10. 100. 1. 10. 100. 1. . . 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?. 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.. :. 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 ). Jun Cao. Institute of High Energy Physics. Gordon Research Conference on “New . Tools for the Next Generation of Particle Physics and . Cosmology”, HKUST, Hong Kong, Jun.30-Jul.4, 2019. Neutrino Mixing. 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. Kavli. IPMU, Univ. of Tokyo. for Super-K collaboration . Recent results from. Super-. Kamiokande. Neutrinos and Dark Matter in Nuclear Physics 2015, June 1st, . 2015. 1. Neutrinos and Dark Matter in Nuclear Physics 2015, June 1st, .
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