POEMMA: Probe Of Extreme Multi-Messenger Astrophysics
POEMMA: Probe Of Extreme Multi-Messenger Astrophysics
复制标题
POEMMA:极限多信使天体物理学探测器
DOI:
10.22323/1.301.0542
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发表时间:
2017
期刊:
影响因子:
--
通讯作者:
R. Young
中科院分区:
文献类型:
--
作者:
A. Olinto;J. H. Adams;R. Aloisio;L. Anchordoqui;D. Bergman;M. Bertaina;P. Bertone;M. Bustamante;M. Christl;S. Csorna;J. Eser;F. Fenu;C. Guépin;E. Hays;S. Hunter;E. Judd;I. Jun;K. Kotera;J. Krizmanic;E. Kuznetsov;Š. Mackovjak;L. M. Martinez;M. Mastafa;J. Matthews;J. Mcenery;J. Mitchell;A. Neronov;A. Otte;É. Parizot;T. Paul;J. Perkins;G. Prévôt;P. Reardon;M. Reno;F. Sarazin;K. Shinozaki;F. Stecker;R. Streitmatter;T. Venters;L. Wiencke;R. Young
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission is being designed to establish charged-particle astronomy with ultra-high energy cosmic rays (UHECRs) and to observe cosmogenic tau neutrinos (CTNs). The study of UHECRs and CTNs from space will yield orders-of-magnitude increase in statistics of observed UHECRs at the highest energies, and the observation of the cosmogenic flux of neutrinos for a range of UHECR models. These observations should solve the long-standing puzzle of the origin of the highest energy particles ever observed, providing a new window onto the most energetic environments and events in the Universe, while studying particle interactions well beyond accelerator energies. The discovery of CTNs will help solve the puzzle of the origin of UHECRs and begin a new field of Astroparticle Physics with the study of neutrino properties at ultra-high energies.
DOI:
--
发表时间:
2005
期刊:
影响因子:
--
作者:
J.-L. Atteia;N. Kawai;R. Vanderspek;他36名;J.-L.Atteia;T.Sakamoto;J.S.Villasenor;R.Sato;辺見 香理;恩田 香織;辺見香理;山岡和貴;大野雅功;恩田香織;園田絵里;大野 雅功;大野雅功;田代信;寺田幸功;山岡和貴;山岡和貴;K. Yamaoka;K. Yamaoka;M. Ohno;D. Yonetoku;杉田聡司;洪秀徴;M.S. Tashiro;M. Ohno;Y.E. Nakagawa;山内誠;杉原将;田代信;J. S. Villasenor;前野将太;杉原将
通讯作者:
杉原将