A Xenon Solar Neutrino Detector
Nuclear Experiment
2011-05-23 v1 High Energy Physics - Phenomenology
Nuclear Theory
Abstract
The neutrino capture by Xe with a threshold at 352 keV as reaction to detect solar neutrinos is examined. The most important feature of this process is its high sensitivity to beryllium neutrinos, which contribute approximately 40% to the total capture rate (45 SNU) assuming the fluxes predicted by the Standard Solar Model.
Cite
@article{arxiv.nucl-ex/9707006,
title = {A Xenon Solar Neutrino Detector},
author = {A. Sh. Georgadze and H. V. Klapdor-Kleingrothaus and H. Päs and Yu. G. Zdesenko},
journal= {arXiv preprint arXiv:nucl-ex/9707006},
year = {2011}
}
Comments
9 pages, Latex, Talk given by Yu.G. Zdesenko at the 4th Int. Conf. on Solar Neutrinos, Heidelberg