PPT-US-Japan Collaboration on high intensity neutrino beams

Laser manipulation of H beams Brief status at JPARC amp Progress of 400 MeV H striping to protons by using only lasers Pranab K Saha On behalf of JPARC laser stripping group. 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.. Kai Classic Premier Kaji Reserve Blue Dual Core Hiro Fuji Made In China Japan Japan Japan Japan Japan Japan Japan Japan Steel Blades VG-Max Core VG-Max Core SG-11 Clad Core SG-11 Clad Core Blue II Car 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. 1. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. Neutrino. 2. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. 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?. 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-. 0. Accelerators for neutrino physics:. The Beta. . Beam. . . . Elena Wildner, . BE. /. ABP. 0. 2015-11-26. 2015-11-26. Elena Wildner: Beta Beams, ATS Seminar. 1. Outline. General: . Neutrinos. 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.. 12 December 2014. Physics and Friendships, . A Symposium in honor of David . Leith. 1. With . thanks to David and to . all,. I . would like to - . talk to you about . the roles played by, and contributions made by David in the Japan-US cooperation in the field of high energy physics. properties from COHERENT elastic neutrino-nucleus scatteringSpeakerYiyu ZhangInstitute of High Energy Physics CAS2021/2/19Yiyu Zhang IHEP 1M Cadedduet al PhysRevD10220201015030Based on a work in 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.