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000410424 0247_ $$2datacite_doi$$a10.3204/PUBDB-2018-00782/C8
000410424 037__ $$aPUBDB-2018-03606
000410424 041__ $$aEnglish
000410424 1001_ $$0P:(DE-H253)PIP1006295$$aSigl, Guenter$$b0$$eCorresponding author
000410424 245__ $$aPropagation of Very High Energy Radiation in the Universe
000410424 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2018
000410424 29510 $$aSigl, Günter "Propagation of Very High Energy Radiation in the Universe" in Particles, Strings and the Early Universe : The Structure of Matter and Space-Time / Haller, Johannes, Grefe, Michael (eds.), Verlag Deutsches Elektronen-Synchrotron : 2018
000410424 300__ $$a379-386
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000410424 520__ $$aThe sources of cosmic rays, in particular ultra-high energy cosmic rays with macroscopic energies above $\sim10^{18}\,$eV, have still not been identified. This is partly caused by the fact that the sky observed in these cosmic rays is surprisingly isotropic and that deflection in galactic and extragalactic magnetic fields may still be substantial. The main goal of project C8 of the SFB 676 was to further develop a general software tool, known as CRPropa, which allows to propagate ultra-high energy cosmic rays from the sources to the observer and make predictions for spectrum, mass composition and sky distribution with a given astrophysical scenario for distribution and injection spectra and composition of the sources and the structure of cosmic magnetic fields.
000410424 536__ $$0G:(DE-HGF)POF3-611$$a611 - Fundamental Particles and Forces (POF3-611)$$cPOF3-611$$fPOF III$$x0
000410424 536__ $$0G:(GEPRIS)13245592$$aDFG project 13245592 - SFB 676: Teilchen, Strings und frühes Universum: Struktur von Materie und Raum-Zeit (13245592)$$c13245592$$x1
000410424 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000410424 7870_ $$0PUBDB-2018-00782$$aHaller, Johannes et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$tParticles, Strings and the Early Universe : The Structure of Matter and Space-Time
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