Open Access
EPJ Web Conf.
Volume 283, 2023
Ultra High Energy Cosmic Rays (UHECR 2022)
Article Number 03010
Number of page(s) 4
Section Anisotropies, Magnetic Fields and UHECR Propagation
Published online 28 April 2023
  1. A. Aab et al. [Pierre Auger], “The Pierre Auger Cosmic Ray Observatory,” Nucl. Instrum. Meth. A 798 (2015), 172-213 doi:10.1016/j.nima.2015.06.058 [arXiv:1502.01323 [astro-ph.IM]]. [Google Scholar]
  2. A. Aab et al. [Pierre Auger], “Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above 8 1018 eV,” Science 357 (2017) no.6537, 1266-1270 doi:10.1126/science.aan4338 [arXiv:1709.07321 [astro-ph.HE]]. [Google Scholar]
  3. K. Greisen, “End to the cosmic ray spectrum?,” Phys. Rev. Lett. 16 (1966), 748-750 doi:10.1103/PhysRevLett.16.748 [Google Scholar]
  4. G. T. Zatsepin and V. A. Kuzmin, “Upper limit of the spectrum of cosmic rays,” JETP Lett. 4 (1966), 78-80 [Google Scholar]
  5. R. Alves Batista, A. Dundovic, M. Erdmann, K. H. Kampert, D. Kuempel, G. Müller, G. Sigl, A. van Vliet, D. Walz and T. Winchen, “CRPropa 3 - a Public Astrophysical Simulation Framework for Propagating Extraterrestrial Ultra-High Energy Particles,” JCAP 05 (2016), 038 doi:10.1088/1475-7516/2016/05/038 [arXiv:1603.07142 [astro-ph.IM]]. [CrossRef] [Google Scholar]
  6. G. L. Bryan et al. [ENZO], “Enzo: An Adaptive Mesh Refinement Code for Astrophysics,” Astrophys. J. Suppl. 211 (2014), 19 doi:10.1088/0067-0049/211/2/19 [arXiv:1307.2265 [astro-ph.IM]]. [CrossRef] [Google Scholar]
  7. S. Hackstein, F. Vazza, M. Brüggen, J. G. Sorce and S. Gottlöber, “Simulations of ultra-high Energy Cosmic Rays in the local Universe and the origin of Cosmic Magnetic Fields,” Mon. Not. Roy. Astron. Soc. 475 (2018) no.2, 2519-2529 doi:10.1093/mnras/stx3354 [arXiv:1710.01353 [astro-ph.CO]]. [Google Scholar]
  8. K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke and M. Bartelman, “HEALPix - A Framework for high resolution discretization, and fast analysis of data distributed on the sphere,” Astrophys. J. 622 (2005), 759-771 doi:10.1086/427976 [arXiv:astro-ph/0409513 [astro-ph]]. [CrossRef] [Google Scholar]
  9. H. P. Bretz, M. Erdmann, P. Schiffer, D. Walz and T. Winchen, “PARSEC: A Parametrized Simulation Engine for Ultra-High Energy Cosmic Ray Protons,” Astropart. Phys. 54 (2014), 110-117 doi:10.1016/j.astropartphys.2013.12.002 [arXiv:1302.3761 [astro-ph.HE]]. [CrossRef] [Google Scholar]
  10. R. Jansson and G. R. Farrar, “The Galactic Magnetic Field,” Astrophys. J. Lett. 761 (2012), L11 doi:10.1088/2041-8205/761/1/L11 [arXiv:1210.7820 [astro-ph.GA]]. [CrossRef] [Google Scholar]
  11. J. Jasche, A. van Vliet and J. P. Rachen, “Targeting Earth: CRPropa learns to aim,” PoS ICRC2019 (2020), 447 doi:10.22323/1.358.0447 [arXiv:1911.05048 [astro-ph.HE]]. [Google Scholar]
  12. R. Alves Batista, J. Becker Tjus, J. Dörner, A. Dundovic, B. Eichmann, A. Frie, C. Heiter, M. R. Hoerbe, K. H. Kampert and L. Merten, et al. “CRPropa 3.2 — an advanced framework for high-energy particle propagation in extragalactic and galactic spaces,” JCAP 09 (2022), 035 doi:10.1088/1475-7516/2022/09/035 [arXiv:2208.00107 [astro-ph.HE]]. [CrossRef] [Google Scholar]

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