利用大型液体闪烁体探测器寻找来自$^{40}$K的反中微子通量
仪器与探测器
2015-06-19 v2 高能物理 - 实验
摘要
我们考虑了探测地球内部K产生的反中微子通量的可能性。观测此类通量有助于更好地理解地球的热通量。我们给出了K反中微子通量的下限和上限。
引用
@article{arxiv.1405.3140,
title = {Looking for antineutrino flux from $^{40}$K with large liquid scintillator detector},
author = {V. V. Sinev and L. B. Bezrukov and E. A. Litvinovich and I. N. Machulin and M. D. Skorokhvatov and S. V. Sukhotin},
journal= {arXiv preprint arXiv:1405.3140},
year = {2015}
}
备注
Latex 8 pages, 4 figures. Talk given at International Workshop on Prospects of Particle Physics: {\guillemotleft}Neutrino Physics and Astrophysics{\guillemotright}, Valday, January 27 - February 2, 2014