PPT-Sterile Neutrino Search Jose Alonso

MIT 1 Outline Neutrino Oscillation Physics Anomalies Indications for Sterile Neutrinos IsoDAR at KamLAND Longer Range Plans Jose Alonso MIT 2 Jose Alonso MIT 3 Jose Alonso MIT. McMahon & Associates is above all a service oriented company, dedicated to the valued customers we have accrued all over the world. We are known for our responsive, courteous staff, our attention to detail, and the legal savvy that comes from working with some of the very best. ALONSO: Much of your work began during the formative period when we were just discovering the Maya. You could have studied sculpture or architecture… DR. RANDS: I studied sculpture. That was m 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.. 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. 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. Alan Bross. N u F a c t 0 9. From . SuperBeams. to Neutrino Factories. Pre-Ramble. Neutrino Factory means different things to different people. Not so much for . SuperBeams. I will be talking about a muon-based Neutrino Factory as opposed to a . 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. MiniBooNE. Robert . Cooper. 3-Flavor Neutrino Mixing Model. Mass . splittings. D. m. 21. 2. . ≅. . 7.6 × 10. -5. e. V. 2. . D. m. 31. 2. . ≅. 2.4 . × 10. -3. e. V. 2. Mixing angles. Pratanu Roy. Arijit Khan. Gustavo Alonso. Systems Group. ETH. Zurich. Nanyang Technical University. Singapore. Systems Group. ETH. Zurich. Data Stream Processing. IP . traffic, phone calls, sensor measurements. *WG co-lead with Ty . DeYoung. IceCube collaboration meeting, . Banff, March . 8. , 2014. 3rd Oscillations Working Group Report:. I. t just got interesting. Atmospheric Neutrino Oscillations. Search for . Bacillussubtilis,severalrecombination-de®cientmutantswithincreasedsensitivitiestoDNA-damagingagentshavebeenisolated.Geneticanalysisofchromosomalandplasmidtransformationshasdemonstratedthattobeef®cie 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 . hopes and failures. From: History of Neutrinos, Paris September 2018. For: La Physique des Neutrinos, Paris September 2022. Why am I giving this talk?. Probably because I’ve been putting out a free monthly ~100 line “long-baseline newsletter” about all things neutrino since 1992.