PPT-NEUTRINO PHYSICS FROM

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. 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. 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 . 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.. 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,. –. . COBAND. . Experiment –. Continuous. . Spectra. l. . Measurement. . in Far-Infrared Region using STJ. Shin-Hong Kim. 　. （. University of Tsukuba, . TCHoU. ）. for COBAND collaboration. Are we close to measuring the neutrino hierarchy? Filipe B. Abdalla ν Loureiro , Moraes , Abdalla et al. arXiv:1809.07204 Loureiro , Cuceu , Abdalla et al. arXiv:1811.02578 Outline Cosmology background General Presentation – Zagreb (Croatia) – 23. rd. of October – 11h00 - 12h30. The Chair, Tord Ekelöf. Aysel. . Kayis. . Topaksu. Marcos Dracos. Georgios . Fanourakis. Eliane Bouquerel. Marie-Laure Schneider. 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. 1. John Beacom, The Ohio State University. High Energy . Neutrino . Astronomy. Topic: Impossible. Requires. : sources that reach high energies. . sources that are luminous. . sources of different types. 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?. 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.