EUSO-SPB2: A sub-orbital cosmic ray and neutrino multi-messenger pathfinder observatory

Austin Cummings, Johannes Eser, George Filippatos, Angela V. Olinto, Tonia M. Venters, Lawrence Wiencke
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引用次数: 1

Abstract

The next generation of ultra-high energy cosmic ray (UHECR) and very-high energy neutrino observatories will address the challenge of the extremely low fluxes of these particles at the highest energies. EUSO-SPB2 (Extreme Universe Space Observatory on a Super Pressure Balloon 2) is designed to prepare space missions to address this challenge. EUSO-SPB2 is equipped with 2 telescopes: the Fluorescence Telescope, which will point downwards and measure fluorescence emission from UHECR air showers with an energy above 2 EeV, and the Cherenkov Telescope (CT), which will point towards the Earth’s limb and measure direct Cherenkov emission from cosmic rays with energies above 1 PeV verifying the technique. Pointed below the limb, the CT will search for Cherenkov emission produced by neutrino-sourced tau-lepton decays above 10 PeV energies and study backgrounds for such events. The EUSO-SPB2 mission will provide pioneering observations and technical milestones on the path towards a space-based multi-messenger observatory.
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EUSO-SPB2:亚轨道宇宙射线和中微子多信使探路者天文台
下一代超高能宇宙射线(UHECR)和超高能中微子天文台将解决这些粒子在最高能量下极低通量的挑战。EUSO-SPB2(超压气球上的极端宇宙空间天文台2)的设计就是为了准备太空任务来应对这一挑战。EUSO-SPB2配备了两个望远镜:一个是荧光望远镜,它将向下指向并测量能量在2 EeV以上的UHECR空气簇的荧光发射,另一个是切伦科夫望远镜(CT),它将指向地球边缘并测量能量在1 PeV以上的宇宙射线的直接切伦科夫发射,以验证该技术。指向肢体下方,CT将搜索由中微子源的10 PeV能量以上的τ轻子衰变产生的切伦科夫辐射,并研究此类事件的背景。EUSO-SPB2任务将在通往天基多信使天文台的道路上提供开创性的观测和技术里程碑。
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