Open Access
| Issue |
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 | |
| DOI | https://doi.org/10.1051/epjconf/202328303010 | |
| Published online | 28 April 2023 | |
- 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]
- 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]
- K. Greisen, “End to the cosmic ray spectrum?,” Phys. Rev. Lett. 16 (1966), 748-750 doi:10.1103/PhysRevLett.16.748 [Google Scholar]
- G. T. Zatsepin and V. A. Kuzmin, “Upper limit of the spectrum of cosmic rays,” JETP Lett. 4 (1966), 78-80 [Google Scholar]
- 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]
- 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]
- 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]
- 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]
- 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]
- 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]
- 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]
- 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]
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.