论文标题
带有切伦科夫望远镜阵列的tau中微子
Tau Neutrinos with Cherenkov Telescope Array
论文作者
论文摘要
下一代成像大气Cherenkov望远镜（例如CTA）将强烈提高高能量宇宙射线的检测能力。在我们的论文中，我们讨论了使用此类设备检测地球中微子的可能性。有趣的是，分析表明，在较大的较大的中微子通量的乐观案例中，平坦频谱无线电类星体产生的较大的中微子通量，每年的订单每年几乎无法检测到$ 10^8 $ GEV。但是，即使对于更保守的宇宙中微子通量，也将获得这种速度，但是在十年的运行中。该估计似乎也可以进行像CTA这样的设置，以执行高能量中微子天文学。
The next generation of Imaging Atmospheric Cherenkov telescope, like CTA, is going to strongly improve the detection capability of high-energy cosmic rays. In our paper we discuss the possibility to use such apparatus to detect Earth-skimming tau neutrinos. Interestingly the analysis shows that order few events per year can be detected for energies above $10^8$ GeV in the optimistic case of larger neutrino fluxes produced by Flat Spectrum Radio Quasars. However, even for more conservative cosmogenic neutrino fluxes such rate will be also obtained, but for a decade of running. This estimate seems to candidate a set up like CTA for performing high energy neutrino astronomy as well.
