{ "id": "1810.02284", "version": "v1", "published": "2018-10-04T15:56:50.000Z", "updated": "2018-10-04T15:56:50.000Z", "title": "Prospects of testing a minimal model for extragalactic cosmic rays and neutrinos with the K-EUSO orbital telescope", "authors": [ "O. Kalashev", "M. Pshirkov", "M. Zotov" ], "comment": "13 pages", "categories": [ "astro-ph.HE", "astro-ph.IM" ], "abstract": "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 a uniform exposure over the celestial sphere and register from 120 to 500 UHECRs at energies above 57 EeV in a 2-year mission. We employed the CRPropa 3 package to estimate prospects of testing a minimal model for extragalactic cosmic rays and neutrinos by Kachelriess, Kalashev, Ostapchenko and Semikoz (2017) with K-EUSO in terms of the large-scale anisotropy assuming the Jansson-Farrar (2012) model of the galactic magnetic field. Nearby active galactic nuclei Centaurus A, M82, NGC 253, M87 and Fornax A were considered as possible sources of UHECRs. We demonstrate that an observation of 200 events will allow testing predictions of the model with a high confidence level providing the fraction of from-source events is 12-19%, depending on a particular source, with a smaller contribution for larger samples. Thus the K-EUSO experiment will provide good opportunities for verifying the KKOS model basing on an analysis of the large-scale anisotropy if UHECR flux from any of the sources satisfies the above demands.", "revisions": [ { "version": "v1", "updated": "2018-10-04T15:56:50.000Z" } ], "analyses": { "keywords": [ "extragalactic cosmic rays", "k-euso orbital telescope", "minimal model", "ultra-high energy cosmic rays", "nearby active galactic nuclei centaurus" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }