Slide 1Application of neutrino spectrometry 1) Solar neutrino detection 2) Supernovae neutrino detection 3) Cosmic and atmospheric neutrino detection 4) Neutrino oscillation…

Slide 1 PHYS 1621 Supernova and Neutron Stars For heavy white dwarves with a companion star acquire mass, if becomes > 1.4 M(Sun) SUPERNOVA (Ia). p + e  n + neutrino…

Slide 1 The ANTARES Neutrino Telescope Mieke Bouwhuis 27/03/2006 Slide 2 Broadband light source 1’ radio 10 -8 eV optical 10 eVx rays 10 4 eV gamma rays10 12 eV The pulsar…

Some Canadian History In Two Parts PEngineering Education - the Beginnings PThe Millennium Project The Origins of Engineering Education in Canada With Ray Findlay King's…

PHYS 162 * Supernova and Neutron Stars For heavy white dwarves with a companion star acquire mass, if becomes > 1.4 M(Sun) SUPERNOVA (Ia). p + e  n + neutrino Usually…

PowerPoint Presentation ANtarctic Impulsive Transient Antenna University of Hawaii at Manoa Peter Gorham, PI John Learned and Gary S. Varner Ohio-State University Jim Beatty…

KamLAND Results Junpei Shirai for the KamLAND Collaboration Tohoku University NOW2006, Conca Specchiulla, Italy Sep.10-15, 2006 SUN… Earth Reactor KamLAND KamLAND (Kamioka…

Welcome to SNOLAB And to the Neutrino Geoscience Conference Art McDonald Queen’s University, Kingston Director, SNO Institute (+) The Enigmatic Neutrino I have done a terrible…