The Payload for Ultrahigh Energy Observations (PUEO): a white paper

The Payload for Ultrahigh Energy Observations (PUEO): a white paper
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DOI:
10.1088/1748-0221/16/08/p08035
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发表时间:
2020-10
影响因子:
1.3
通讯作者:
Q. Abarr;P. Allison;J. Ammerman Yebra;J. Alvarez-Muñiz;J. Beatty;D. Besson;P. Chen;Y. Chen;C. Xie;J. Clem;A. Connolly;L. Cremonesi;C. Deaconu;J. Flaherty;D. Frikken;P. Gorham;C. Hast;C. Hornhuber;J. Huang;K. Hughes;A. Hynous;Y. Ku;C. Kuo;T. Liu;Z. Martin;C. Miki;J. Nam;R. Nichol;K. Nishimura;A. Novikov;A. Nozdrina;E. Oberla;S. Prohira;R. Prechelt;B. Rauch;J. M. Roberts;A. Romero-Wolf;J. W. Russell;D. Seckel;J. Shiao;D. Smith;D. Southall;G. Varner;A. Vieregg;S. Wang;Y. Wang;S. Wissel;R. Young;E. Zas;A. Zeolla
Q. Abarr;P. Allison;J. Ammerman Yebra;J. Alvarez-Muñiz;J. Beatty;D. Besson;P. Chen;Y. Chen;C. Xie;J. Clem;A. Connolly;L. Cremonesi;C. Deaconu;J. Flaherty;D. Frikken;P. Gorham;C. Hast;C. Hornhuber;J. Huang;K. Hughes;A. Hynous;Y. Ku;C. Kuo;T. Liu;Z. Martin;C. Miki;J. Nam;R. Nichol;K. Nishimura;A. Novikov;A. Nozdrina;E. Oberla;S. Prohira;R. Prechelt;B. Rauch;J. M. Roberts;A. Romero-Wolf;J. W. Russell;D. Seckel;J. Shiao;D. Smith;D. Southall;G. Varner;A. Vieregg;S. Wang;Y. Wang;S. Wissel;R. Young;E. Zas;A. Zeolla
中科院分区:
工程技术4区
文献类型:
--
作者:
Q. Abarr;P. Allison;J. Ammerman Yebra;J. Alvarez-Muñiz;J. Beatty;D. Besson;P. Chen;Y. Chen;C. Xie;J. Clem;A. Connolly;L. Cremonesi;C. Deaconu;J. Flaherty;D. Frikken;P. Gorham;C. Hast;C. Hornhuber;J. Huang;K. Hughes;A. Hynous;Y. Ku;C. Kuo;T. Liu;Z. Martin;C. Miki;J. Nam;R. Nichol;K. Nishimura;A. Novikov;A. Nozdrina;E. Oberla;S. Prohira;R. Prechelt;B. Rauch;J. M. Roberts;A. Romero-Wolf;J. W. Russell;D. Seckel;J. Shiao;D. Smith;D. Southall;G. Varner;A. Vieregg;S. Wang;Y. Wang;S. Wissel;R. Young;E. Zas;A. Zeolla

文献摘要

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超高能观测有效载荷(PUEO)长期气球实验旨在对能量超过1 EeV的超高能中微子具有世界领先的灵敏度。探测这个能量区域对于理解所有距离尺度上的极端能量宇宙至关重要。PUEO利用了成功的南极脉冲瞬态天线(ANITA)计划的经验,并取代了该计划,其改进的设计在能量低于30 EeV时将灵敏度大幅提高了一个数量级以上。PUEO将对超高能中微子通量进行首次重要探测或设定最佳限制。
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to have world-leading sensitivity to ultrahigh-energy neutrinos at energies above 1 EeV. Probing this energy region is essential for understanding the extreme-energy universe at all distance scales. PUEO leverages experience from and supersedes the successful Antarctic Impulsive Transient Antenna (ANITA) program, with an improved design that drastically improves sensitivity by more than an order of magnitude at energies below 30 EeV. PUEO will either make the first significant detection of or set the best limits on ultrahigh-energy neutrino fluxes.