利用低能β束理解超新星中微子物理
核理论
2009-11-11 v1
摘要
我们表明，将低能 β 束谱的线性组合拟合到超新星中微子能谱分布，能以非常精确的方式重建核靶对超新星通量的响应。这使得人们能对地面中微子探测器中的超新星中微子信号作出直接预言。
引用
@article{arxiv.nucl-th/0511069,
title = {Understanding Supernova Neutrino Physics using Low-Energy Beta-Beams},
author = {N. Jachowicz and G. C. McLaughlin},
journal= {arXiv preprint arXiv:nucl-th/0511069},
year = {2009}
}
备注
To appear in the proceedings of International School of Nuclear Physics: 27th Course: "Neutrinos in Cosmology, in Astro, Particle and Nuclear Physics". Erice, Sicily, Italy, 16-24