Non-accelerator Experiments and Their Implications

该奖项是为重要的理论研究， 实验数据的解释和理解 宇宙射线广泛的空气簇射和中微子通量。 本集团 两名高级教师，以及一名博士后助理 专注于中微子相互作用率的计算， 各种探测器，进一步开发一个模型来计算 高能粒子的相互作用和 宇宙射线的主要成分。1014电子伏。 最后一点是 与基于假设加速度的预期进行比较 机制等

The award is for theoretical studies important for the interpretation and understanding of experimental data on cosmic-ray extensive air showers and neutrino fluxes. The group of two senior faculty, together with a post-doctoral associate focus on calculations of neutrino interaction rates in the various detectors, further development of a model to calculate particle interactions at high energies and determination of the primary composition of cosmic-rays at . 1014 eV. That last is to be compared with expectations based on hypothesized acceleration mechanisms.