Supernova Detection via a Network of Neutral Current Spherical TPC's

Details Supernova Detection via a Network of Neutral Current Spherical TPC's Supernova Detection via a Network of Neutral Current Spherical TPC's

2006-01-12

arxiv.org/abs/hep-ph/0601093v1

AIP Conf.Proc.847:140-146,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, 2 figures. Talk presented at the International Symposium on Origin of Matter and Evolution of Galaxies (OMEG05)- New

Scientific paper

10.1063/1.2234395

The coherent contribution of all neutrons in neutrino nucleus scattering due to the neutral current offers a realistic prospect of detecting supernova neutrinos. For a typical supernova at 10 kpc, about 1000 events are expected using a spherical gaseous detector of radius 4 m and employing Xe gas at a pressure of 10 Atm. We propose a world wide network of several such simple, stable and low cost supernova detectors with a running time of a few centuries.

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