1. Electric  U*lity  Industry   Transforma*on   6th  SMART  GRIDS  &  CLEANPOWER   Cambridge,  UK       June  4,  2014   www.hvm-­‐uk.com   John  Di…

Slide 1 The on-going programme Slide 2 3-family oscillation matrix (Pontecorvo, Maki, Nakagawa, Sakata) S = sine c = cosine   CP violation phase.   …

Getting the first 7Be n detection: scintillator purification, detector response and data analysis in Borexino Marco Pallavicini Università di Genova & INFN On behalf…

Expected rates for various targets For a heavy target nucleus such as Xe, a very low recoil energy threshold is crucial. The expected rate, integrated above threshold of…

MARKETING DE SERVICIOS CURSO : MARKETING DE SERVICIOS DOCENTE : Lic. FRANKLIN CORDOVA BUIZA CARRERA : ADMINISTRACIÃN Y MARKETING INTEGRANTES : · CAIRO MERCADO, Jersihno…

Results from Borexino Davide Franco CNRS-APC NOW 2012 September 9-16, 2012 Davide Franco – APC CNRS – NOW2012 Detector layout and radiopurity Water Tank: g and n shield…

Status of bb decay Ruben Saakyan UCL Outline Motivation bb decay basics Results so far Current experiments Future projects and sensitivity Motivation Neutrino Mixing Observed…

PowerPoint Presentation A Guess at the Status of Neutrino Oscillation Physics in 2020 Dave Wark Oxford University/RAL 1st European Hyper Kamiokande Meeting QMUL, London Dec.…

Getting the first 7Be n detection: scintillator purification, detector response and data analysis in Borexino Marco Pallavicini Università di Genova & INFN On behalf…

Steve Boyd, University of Warwick “If we are to understand “why we are here” and the basic properties of the universe we live in, we must understand the neutrino.”…