Performance and science reach of the Probe of Extreme Multimessenger Astrophysics for ultrahigh-energy particles

被引:28
作者
Anchordoqui, Luis A. [1 ,2 ,3 ]
Bergman, Douglas R. [4 ,5 ]
Bertaina, Mario E. [6 ]
Fenu, Francesco [6 ]
Krizmanic, John F. [7 ,8 ]
Liberatore, Alessandro [6 ]
Olinto, Angela V. [9 ]
Reno, Mary Hall [10 ]
Sarazin, Fred [11 ]
Shinozaki, Kenji [6 ]
Soriano, Jorge F. [1 ,2 ]
Ulrich, Ralf [12 ]
Unger, Michael [12 ]
Venters, Tonia M. [13 ]
Wiencke, Lawrence [11 ]
机构
[1] CUNY, Lehman Coll, Dept Phys & Astron, New York, NY 10468 USA
[2] CUNY, Grad Ctr, Dept Phys, New York, NY 10016 USA
[3] Amer Museum Nat Histde, Dept Astrophys, New York, NY 10024 USA
[4] Univ Utah, High Energy Astrophys Inst, Salt Lake City, UT 84112 USA
[5] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA
[6] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy
[7] NASA, CRESST, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[8] Univ Maryland Baltimore Cty, Baltimore, MD 21250 USA
[9] Univ Chicago, Dept Astron & Astrophys, KICP, EFI, 5640 S Ellis Ave, Chicago, IL 60637 USA
[10] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[11] Colorado Sch Mines, Dept Phys, Golden, CO 80401 USA
[12] Karlsruher Inst Technol, Inst Kernphys, D-76021 Karlsruhe, Germany
[13] NASA, Astrophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
基金
美国国家科学基金会;
关键词
HEAVY DARK-MATTER; GAMMA-RAY BURSTS; COSMIC-RAYS; AIR; ANISOTROPY; SPECTRUM; ARRAY; RADIATION; DETECTOR; CANDIDATES;
D O I
10.1103/PhysRevD.101.023012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Probe of Extreme Multimessenger Astrophysics (POEMMA) is a potential NASA Astrophysics Probe-class mission designed to observe ultrahigh-energy cosmic rays (UHECRs) and cosmic neutrinos from space. POEMMA will monitor colossal volumes of the Earth's atmosphere to detect extensive air showers (EASs) produced by extremely energetic cosmic messengers: UHECRs above 20 EeV over the full sky and cosmic neutrinos above 20 PeV. We focus most of this study on the impact of POEMMA for UHECR science by simulating the detector response and mission performance for EAS from UHECRs. We show that POEMMA will provide a significant increase in the statistics of observed UHECRs at the highest energies over the entire sky. POEMMA will be the first UHECR fluorescence detector deployed in space that will provide high-quality stereoscopic observations of the longitudinal development of air showers. Therefore it will be able to provide event-by-event estimates of the calorimetric energy and nuclear mass of UHECRs. The particle physics in the interactions limits the interpretation of the shower maximum on an event-by-event basis. In contrast, the calorimetric energy measurement is significantly less sensitive to the different possible final states in the early interactions. POEMMA will increase by a factor of 30 fluorescence observations, with accurate measurements of the shower maximum. We study the prospects to discover the origin and nature of UHECRs using expectations for measurements of the energy spectrum, the distribution of arrival direction, and the atmospheric column depth at which the EAS longitudinal development reaches maximum. We also explore supplementary science capabilities of POEMMA through its sensitivity to particle interactions at extreme energies and its ability to detect ultrahigh-energy neutrinos and photons produced by top-down models including cosmic strings and superheavy dark matter particle decay in the halo of the Milky Way.
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页数:39
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