PDF | This document represents the response of the Intensity Frontier Neutrino Working Group to the Snowmass charge. We summarize the current status of neutrino physics and identify many exciting Sterile-neutrino DM produced is colder than DM produced via oscillations, and thus has different small-scale structure properties . Thermal content of DM sterile neutrinos Producing the right amount of DM fixes the coupling of Experimental discovery of neutrino 1953 Clyde Cowan and Fred Reines set to observe neutrino interactions. Their first idea was to use the pulse of huge neutrino flux coming out from a nuclear explosion The use of a nuclear reactor proved to be much more practical—they chose Savanna River Reactor in South Carolina. Neutrino Properties INTRODUCTION TO THE NEUTRINO PROPERTIES LISTINGS Revised August 2013 by P. Vogel (Caltech) and A. Piepke (University of Alabama). The following Listings concern measurements of various properties of neutrinos. Nearly all of the measurements, all of which so far are limits, actually concern superpositions of The Detector A neutrino interacts with matter in the telescope, creating a muon or a hadronic or electromagnetic shower The muon (or shower) emits Cherenkov radiation as it travels through the ice Photomultipliers pick up the Cherenkov radiation and can infer the direction of travel The Oscillating Neutrino After Reines and Cowan detected he neutrino in the late 1950s, particle hysics went through a spectacular ? owering that culminated in the formu-ation of the Standard Model. This model incorporates all that is known bout the subatomic world. It identi? es he most elementary constituents of matter, the elusive Neutrino is founded upon the dual-notion of drag-and-drop simplicity and the ability to configure the precise DSP design required by the customer. Accordingly, Neutrino's drag-and-drop Xilica Designer software can be used to accommodate each project need, and incorporates a GUI that is designed t