PPT-Status of the ESSnuSB neutrino beam and detector project

1 Particle Physics with Neutrino Telescopes Uppsala 7 October 2019 T or d E k e löf Upp s a l a Un i v e rs i t y 20191007 PPNT in Uppsala Tord Ekelof Uppsala University . 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 . 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. 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?. M. Sullivan. Mini-workshop on the MEIC design. Nov 2, 2012. Introduction. Accelerator Parameters. Previous Synchrotron . R. adiation estimates. Other SR issues. Other detector backgrounds. Points of Interest. C. Weiss. 28.11.2013. EAR2 Beam Line - Report on the Status. 1. 28.11.2013. EAR2 Beam Line - Report on the Status. 2. Beam Dump. EAR-2 Exp. Hall. 2. nd. Collimator. Magnet. Pit Shielding. Target. New Area. 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. Neutrino Oscillations in Susan Cartwright Neutrino Oscillations Principles Experimental techniques Neutrino oscillations: Principles The Standard Model contains three neutrinos These can be labelled by flavour as 1. The basis of the potential of . muon. beams. Muon. mass:. 200. . m. e. ~ . m. m. ~ 0.1. . m. p. Muon. decay:. n. e. , . n. m. Precisely known energy spectrum. Energy frontier:. No . brem. -/beam-. 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 . in Japan. T. Ishida. Neutrino Section, J-PARC Center, KEK. on behalf of the neutrino beam group . 1. Contents. Neutrino experimental facility at J-PARC. S. tatus of the facility since NBI2012. . Physics reach of T2K / J-PARC to Hyper-K. IceCube. Justin Vandenbroucke, June 9, 2021. IceCube. Bootcamp, WIPAC, UW–Madison. Outline. Neutrino interactions and cross sections. Muon lifetime. Charged particles losing energy in matter. Ionization. Mike Sullivan. EICUG 2019. July 22-26. Paris, France . 1. Outline. Introduction. Detector Issues. Machine Issues. Unique features of the EIC. Some general questions for the detector and accelerator teams. 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.