白皮书：Arianna-200高能中微子望远镜

论文标题

白皮书：Arianna-200高能中微子望远镜

White Paper: ARIANNA-200 high energy neutrino telescope

论文作者

Anker, A., Baldi, P., Barwick, S. W., Bergman, D., Bernhoff, H., Besson, D. Z., Bingefors, N., Botner, O., Chen, P., Chen, Y., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Huang, J. J., Klein, S. R., Kleinfelder, S. A., Kuo, C. -Y., Lahmann, R., Latif, U., Liu, T., Lyu, Y., McAleer, S., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Shiao, J. Y., Tatar, J., van Vliet, A., Wang, S. -H., Wang, Y. -H., Welling, C.

论文摘要

拟建的Arianna-200中微子检测器位于南极洲的Ross Ice Beshelf的海平面，由200个自主和独立的探测器站组成，在一个均匀的三角形网格中被1公里隔开，并作为未来Icecube-gen2项目的途径任务。 Arianna-200的主要科学任务是搜索能量大于10^17 eV的中微子的来源，以补充IceCube的范围。对中微子来源的Arianna观察将为宇宙射线的神秘来源提供深刻的见解。 Arianna观察到南极冰中高能量中微子相互作用的无线电发射。在目前调查的基于无线电的概念中，Arianna-200在任何瞬间的任何瞬间都将唯一地调查南部天空的绝大多数，而北方天空的重要区域则是由于其位于南极洲的Ross Ice架子的位置。宽阔的天空覆盖范围是摩尔湾遗址的特殊性，使Arianna-200非常适合为美国国家科学基金会（美国国家科学基金会），宇宙中的Windows-Multi Messenger天体物理学做出贡献，提供了从未知方向观察爆炸性来源的能力。 Arianna结构旨在测量每个中微子候选者在3度以内的角度方向，这在追求天体物理学来源的多间隔观察中也起着重要作用。

The proposed ARIANNA-200 neutrino detector, located at sea-level on the Ross Ice Shelf, Antarctica, consists of 200 autonomous and independent detector stations separated by 1 kilometer in a uniform triangular mesh, and serves as a pathfinder mission for the future IceCube-Gen2 project. The primary science mission of ARIANNA-200 is to search for sources of neutrinos with energies greater than 10^17 eV, complementing the reach of IceCube. An ARIANNA observation of a neutrino source would provide strong insight into the enigmatic sources of cosmic rays. ARIANNA observes the radio emission from high energy neutrino interactions in the Antarctic ice. Among radio based concepts under current investigation, ARIANNA-200 would uniquely survey the vast majority of the southern sky at any instant in time, and an important region of the northern sky, by virtue of its location on the surface of the Ross Ice Shelf in Antarctica. The broad sky coverage is specific to the Moore's Bay site, and makes ARIANNA-200 ideally suited to contribute to the multi-messenger thrust by the US National Science Foundation, Windows on the Universe - Multi-Messenger Astrophysics, providing capabilities to observe explosive sources from unknown directions. The ARIANNA architecture is designed to measure the angular direction to within 3 degrees for every neutrino candidate, which too plays an important role in the pursuit of multi-messenger observations of astrophysical sources.

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