Slide 1Search for  13 at Daya Bay On behalf of the Daya Bay Collaboration Deb Mohapatra Virginia Tech Slide 2 Outline The neutrino mixing matrix and the mixing angle θ…

Slide 1 Snowmass 14-7-01G. Eigen, University of Bergen G. Eigen University of Bergen Snowmass July 14, 2001 Slide 2 Snowmass 14-7-01G. Eigen, University of Bergen OUTLINE…

Slide 1 Proposal to put 232 Th Source in  K for > 2MeV Gamma  Detection Bobby Lanza May 1, 2008 Neutron Meeting Slide 2 The case for 232 Th Why are  ’ s with…

Slide 1 Thoughts on Mu2e Electromagnetic Calorimeter Craig Dukes Mu2e Meeting June 3, 2008 Slide 2 Craig DukesMu2e - Fermilab 3/6/082 Performance Requirements Calorimeter…

Slide 1 Solar Neutrino Physics Aksel Hallin PIC 2010 University of Alberta 1 Solar Neutrino Physics Neutrino Physics (the sun is a very intense and quite well understood…

Exam Review: ABR- board exams ABR certification, state licensure (FL included), eligibility: NEED a campemp residency, EXAM- part 1: written (during grad school), part 2:…

R&D on Liquid-Scintillator Detectors R&D and Astroparticle Physics Lisbon, January 8th 2008 Michael Wurm Technische Universität München Organic Liquid Scintillators…

Proposal to put 232Th Source in mK for > 2MeV GammaDetection Bobby Lanza May 1, 2008 Neutron Meeting The case for 232Th Why are ’s with E > 2MeV important?…

The Sudbury Neutrino Observatory First Results and Implications Nick Jelley (University of Oxford) for the SNO Collaboration October 18th, 2001 CERN Dave Wark - TMU Meeting…

What Else Can SNO Do? Muons and Atmospheric Neutrinos Supernovae Anti-Neutrinos Baryon Number Non-Conservation The SNO Detector 9456 8” diameter PMTs 1000 tonnes D2O (99.92%…