Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays
Abstract The determination of the injection composition of cosmic ray nuclei within astrophysical sources requires sufficiently accurate descriptions of the source physics and the propagation – apart from controlling astrophysical uncertainties. We therefore study the implications of nuclear data an...
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Nature Portfolio
2017
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oai:doaj.org-article:017dc46f5b6146d6b5942976e60808da2021-12-02T11:40:42ZNuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays10.1038/s41598-017-05120-72045-2322https://doaj.org/article/017dc46f5b6146d6b5942976e60808da2017-07-01T00:00:00Zhttps://doi.org/10.1038/s41598-017-05120-7https://doaj.org/toc/2045-2322Abstract The determination of the injection composition of cosmic ray nuclei within astrophysical sources requires sufficiently accurate descriptions of the source physics and the propagation – apart from controlling astrophysical uncertainties. We therefore study the implications of nuclear data and models for cosmic ray astrophysics, which involves the photo-disintegration of nuclei up to iron in astrophysical environments. We demonstrate that the impact of nuclear model uncertainties is potentially larger in environments with non-thermal radiation fields than in the cosmic microwave background. We also study the impact of nuclear models on the nuclear cascade in a gamma-ray burst radiation field, simulated at a level of complexity comparable to the most precise cosmic ray propagation code. We conclude with an isotope chart describing which information is in principle necessary to describe nuclear interactions in cosmic ray sources and propagation.Denise BoncioliAnatoli FedynitchWalter WinterNature PortfolioarticleMedicineRScienceQENScientific Reports, Vol 7, Iss 1, Pp 1-10 (2017) |
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Medicine R Science Q Denise Boncioli Anatoli Fedynitch Walter Winter Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
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Abstract The determination of the injection composition of cosmic ray nuclei within astrophysical sources requires sufficiently accurate descriptions of the source physics and the propagation – apart from controlling astrophysical uncertainties. We therefore study the implications of nuclear data and models for cosmic ray astrophysics, which involves the photo-disintegration of nuclei up to iron in astrophysical environments. We demonstrate that the impact of nuclear model uncertainties is potentially larger in environments with non-thermal radiation fields than in the cosmic microwave background. We also study the impact of nuclear models on the nuclear cascade in a gamma-ray burst radiation field, simulated at a level of complexity comparable to the most precise cosmic ray propagation code. We conclude with an isotope chart describing which information is in principle necessary to describe nuclear interactions in cosmic ray sources and propagation. |
format |
article |
author |
Denise Boncioli Anatoli Fedynitch Walter Winter |
author_facet |
Denise Boncioli Anatoli Fedynitch Walter Winter |
author_sort |
Denise Boncioli |
title |
Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
title_short |
Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
title_full |
Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
title_fullStr |
Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
title_full_unstemmed |
Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
title_sort |
nuclear physics meets the sources of the ultra-high energy cosmic rays |
publisher |
Nature Portfolio |
publishDate |
2017 |
url |
https://doaj.org/article/017dc46f5b6146d6b5942976e60808da |
work_keys_str_mv |
AT deniseboncioli nuclearphysicsmeetsthesourcesoftheultrahighenergycosmicrays AT anatolifedynitch nuclearphysicsmeetsthesourcesoftheultrahighenergycosmicrays AT walterwinter nuclearphysicsmeetsthesourcesoftheultrahighenergycosmicrays |
_version_ |
1718395559955398656 |