Production and propagation of ultra-high energy photons using CRPropa 3

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00547156" target="_blank" >RIV/68378271:_____/18:00547156 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1016/j.astropartphys.2018.05.003" target="_blank" >https://doi.org/10.1016/j.astropartphys.2018.05.003</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.astropartphys.2018.05.003" target="_blank" >10.1016/j.astropartphys.2018.05.003</a>

Result language
angličtina
Original language name
Production and propagation of ultra-high energy photons using CRPropa 3
Original language description
In order to interpret cosmic ray observations, detailed modeling of propagation effects invoking all important messengers is necessary. We introduce a new photon production and propagation code as an inherent part of the CRPropa 3 software framework. By implementing additional photon production channels, which are important for energies below similar to 10(18) eV, this code can be used for multi-messenger studies connecting the TeV and sub EeV energy regime and for interpreting models of ultra-high energy cosmic ray sources. We discuss the importance of the individual production channels and propagation effects and present example applications.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10303 - Particles and field physics

Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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