PPT-Cosmic Background Neutrino Decay Search

COBAND Experiment Continuous Spectra l Measurement in FarInfrared Region using STJ ShinHong Kim 　 University of Tsukuba TCHoU for COBAND collaboration. 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. & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. Xiaochuan . Lu and Hitoshi Murayama. NuFact 2013, Aug 22nd. UC Berkeley. 2. Anarchy . approach . applied to neutrino physics . Outline. What is Anarchy Approach. Neutrinoless double beta decay. 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?. . decays. L. Littenberg. (work mainly done by. A.T.Shaikhiev. . INR RAS. ). HQL-2016. 2. Outline. Motivation. Previous heavy neutrino searches. Experiment BNL-E949. Selection criteria. Efficiency and background study. Exclude Light Majorana Neutrinos?. http://. physics.princeton.edu. /~. mcdonald/examples/majorana.pdf. KT . McDonald. Princeton U.. . (October 21, 2016). Sun . Yat. -Sen University. Guangzhou. Beta Decay. Director. . of. ECT* . Trento. . since. . January. . first. 2016. Studies at Univ. Bonn . 1974-79 Dipl. + . Ph. . D. in Jülich/Bonn. 1979-83 . Stony. Brook. 1984-96 Univ. Illinois 1990 . Full.  . The decay rate.  . Lorentz Invariant Phase Space. The decay rate.  . The decay rate.  . Decay amplitude. Describes the interactions during the decay.. The Feynman diagrams. The Feynman diagrams. Krzysztof Panas. Institute of Physics, . Jagiellonian. University in Cracow. , Poland. Majorana mass and . neutrinoless. double beta decay (. 0. νββ. ). GERDA experiment. LEGEND – towards 1 tone germanium . 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. : . universal term for all weak-interaction transitions. . between two neighboring isobars. three different forms. β. -. , . β. +. & . EC. (. capture of an atomic electron. Maurizio . Spurio, . maurizio.spurio@unibo.it. . Università. di Bologna e INFN. 1. M. Spurio - Galactic template neutrino searches. Propagation induces accidents. M. Spurio - Galactic template neutrino searches.