Orateur
Mikhail Zotov
(Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University)
Description
KLYPVE-EUSO (K-EUSO) is a planned orbital detector of ultra-high energy cosmic rays (UHECRs), which is to be deployed on board the International Space Station. K-EUSO is expected to have an almost uniform exposure over the celestial sphere and register from 120 to 500 UHECRs at energies above ~57 EeV in a 2-year mission. We employ the CRPropa3 package to estimate prospects of testing the UHECR single source class model by Kachelriess, Kalashev, Ostapchenko and Semikoz (2017) with K-EUSO in terms of the large-scale anisotropy. According to the simulations, K-EUSO will be able to probe the model in case it records ~200 or more events and the from-source flux constitutes ~20% of the whole data set.
Auteurs principaux
Dr
Oleg Kalashev
(Institute of Nuclear Physics, RAS)
Prof.
Maxim Pshirkov
(Institute of Nuclear Physics, RAS)
Mikhail Zotov
(Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University)
