Non-accelerator Experiments and Their Implications

该奖项旨在表彰对解释和理解关于宇宙射线广泛空气簇射和中微子通量的实验数据具有重要意义的理论研究。这个由两名资深教员和一名博士后组成的小组专注于计算各种探测器中的中微子相互作用率，进一步开发计算高能粒子相互作用的模型，并确定宇宙射线的主要成分。1014 eV。最后一个是与基于假设的加速机制的预期进行比较。

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.