PPT-Reactor Neutrino Results

Jun Cao Institute of High Energy Physics ICHEP Melbourne July 11 2012 Neutrino Mixing 23 45 Atmospheric Accelerator 1 2 34 Solar Reactor 0 1 3. الجمهور: هو احنا هناخد إيه النهاردة؟. أنا: هناخد . Reactor. الجمهور: بس؟. أنا: آه بس. الجمهور: هو السكشن طويل . أنا: آه. Neutrinos. Ghost . Particles . of the . Universe. Georg G. Raffelt. Max-Planck-Institut f. ür Physik, München, Germany. Neutron. Proton. Gravitation (Gravitons?) . Weak . Interaction (W and Z Bosons). in collapsing phase. ～. towards comprehensive neutrino studies . Waseda. . univ.. . Yamada lab.. D1 Chinami Kato. Collaboration with . S. Yamada(. Waseda. ), H. . Nagakura. . (Caltech), W. . Iwakami. antimatter. ?. Susan Cartwright. The Standard Model of particle . physics contains 12 fundamental . particles. 9 of these have electric charge. It turns out that each of these particles has a corresponding antiparticle. 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 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 Roma International Conference on . Astroparticle. Physics. September 2018. Juande Zornoza (IFIC, UV-CSIC). Disclaimer. ~. 3. 0 plenary talks . on these topics… big challenge to . summarize .  rather personal thoughts. 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. Past and Present. Art McDonald. Queen’s University. And. SNOLAB. 1940’s to 1960’s:. Neutrino oscillations were proposed by . Pontecorvo. in 1957 motivated by initial reports of measurements by Davis with a Chlorine detector at a reactor. At that point, the transitions being considered were electron neutrino to electron anti-neutrino.. Alfons Weber. University of Oxford & STFC/RAL. For the T2K Collaboration. Content. Neutrino Oscillations. I. ntroduction. The T2K Experiment. Beam . Near Detector. Far Detector. Results . Disappearance analysis. 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?. 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 . with. . reactor. . experiments. Jonathan . Gaffiot. , . Ph.D. .. CEA . Saclay: IRFU – Service de Physique Nucléaire. Nucifer. . project. . - STEREO . project. 09/15/2012. - Jonathan Gaffiot - Reactor experiments to test sterile nu's.