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. Susan Cartwright. University of Sheffield. Introduction: . Massive neutrinos in the Standard Model. Dirac and . Majorana. masses. The mixing matrix and neutrino oscillations . Massive neutrinos in the . the LENA Detector. Epiphany Conference. Cracow. January 8, 2010. Michael Wurm. Technische Universität München. Michael Wurm, TUM Physics with LENA . 1. /24 . LENA. L. ow-. E. nergy. Zachary Robinson. Phys 406. What creates the sun’s energy?. Composition of Sun. Fusion in the Sun (and other stars). Creation of the elements. Studying the sun with . helioseismology. What is it?. How is it used?. 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 . . . 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?. 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,. 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 1 Methods of Experimental Particle Physics Alexei Safonov Lecture #7 Last Time… We wrote the electroweak lagrangian Found a way to introduce the asymmetry between left handed and right handed interactions imposed on us by W interactions 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 . 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. 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.. 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?. Joint Session, Snowmass Energy Frontier. Jonathan Feng, UC Irvine, 8 July 2020. F. ORWARD . P. HYSICS . F. ACILITY. As the LHC extends the energy frontier to higher energies and much higher luminosities in the coming 15 years, how can its physics potential be maximally exploited?. 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.