PPT-Future Atmospheric Neutrino Experiments

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. 25/09/2014. Day 1 review. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Good / open presentations. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Points to be discussed further:. Maximum temperature gradients allowed in the sensitive volume. 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. t. elescope . Simone . Biagi. on behalf of the ANTARES collaboration. INFN, . Laboratori. . Nazionali. del . Sud. RICH 2016 – Bled 8 Sept 2016. ANTARES: the largest Northern neutrino telescope. Scientific goals. 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.. Exclude Light Majorana Neutrinos?. http://. physics.princeton.edu. /~. mcdonald/examples/majorana.pdf. KT . McDonald. Princeton U.. . (October 21, 2016). Sun . Yat. -Sen University. Guangzhou. Beta Decay. in collapsing phase. ～. towards comprehensive neutrino studies . Waseda. . univ.. . Yamada lab.. D1 Chinami Kato. Collaboration with . S. Yamada(. Waseda. ), H. . Nagakura. . (Caltech), W. . Iwakami. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Mandate. “Rapid progress in neutrino oscillation physics, with significant European involvement, has established a strong scientific case for a long-baseline neutrino programme exploring CP violation and the mass hierarchy in the neutrino sector. CERN should develop a neutrino program to . PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. 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.. Walter Winter. DESY, Zeuthen. TeVPA 2016. CERN. Sept. 12-16, 2016. Nobel prize 2015: Neutrino oscillations. (. http://www.nobelprize.org. , Oct. 6th, 2015). Manifestation. of a new. paradigm: precision physics in lepton sector. Subtitle: Part 1: Dark Matter and BSM Involving Neutrinos. What is this white paper for?. Document the work we have done here. Establish the benchmark on. Where we are with the two themed BSM areas?. Xiaomei. Zhang. IHEP Computing . Center. Outline. Overview of IHEP experiments. General Challenges . Challenges and practice of software. JUNO Neutrino experiment . Status and challenges of computing. Outline. The 3. n. oscillation framework. The current 4 anomalies that don’t fit this framework. LSND. MiniBoone. The Gallium Anomaly. The Reactor Neutrino Anomaly. Summary . The . majority of experimental results on .