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Proton Dominance of Sub-LET Threshold GCR SEE Rate
We apply a Monte Carlo based integral rectangular parallel-piped (IRRP) approach to evaluate the impact of heavy ion reaction products on the Galactic Cosmic Ray (GCR) Single Event Effect (SEE) rate, concluding that owing to their similar high-energy (>100 MeV/n) SEE cross section and much larger...
Autores principales: | , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2017
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1109/TNS.2016.2628363 http://cds.cern.ch/record/2280541 |
_version_ | 1780955598689402880 |
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author | Garcia Alia, Ruben Brugger, Markus Ferlet-Cavrois, Veronique Brandenburg, Sytze Calcutt, Jordan Cerutti, Francesco Daly, Eamonn Ferrari, Alfredo Muschitiello, Michele Santin, Giovanni Uznanski, Slawosz Van Goethem, Marc-Jan Zadeh, Ali |
author_facet | Garcia Alia, Ruben Brugger, Markus Ferlet-Cavrois, Veronique Brandenburg, Sytze Calcutt, Jordan Cerutti, Francesco Daly, Eamonn Ferrari, Alfredo Muschitiello, Michele Santin, Giovanni Uznanski, Slawosz Van Goethem, Marc-Jan Zadeh, Ali |
author_sort | Garcia Alia, Ruben |
collection | CERN |
description | We apply a Monte Carlo based integral rectangular parallel-piped (IRRP) approach to evaluate the impact of heavy ion reaction products on the Galactic Cosmic Ray (GCR) Single Event Effect (SEE) rate, concluding that owing to their similar high-energy (>100 MeV/n) SEE cross section and much larger abundance, protons are expected to be the dominating contributor. In addition, a broad set of components, ions and energies is used to explore the sub-LET threshold experimental region for standard ground-level heavy ion test energies, identifying an overall decreasing trend in the 10-80 MeV/n range due to the decreased contribution of complete and break-up fusion, and pointing out the limitations associated to the application of Monte Carlo SEE models in this energy interval. |
id | oai-inspirehep.net-1614010 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2017 |
record_format | invenio |
spelling | oai-inspirehep.net-16140102019-09-30T06:29:59Zdoi:10.1109/TNS.2016.2628363http://cds.cern.ch/record/2280541engGarcia Alia, RubenBrugger, MarkusFerlet-Cavrois, VeroniqueBrandenburg, SytzeCalcutt, JordanCerutti, FrancescoDaly, EamonnFerrari, AlfredoMuschitiello, MicheleSantin, GiovanniUznanski, SlawoszVan Goethem, Marc-JanZadeh, AliProton Dominance of Sub-LET Threshold GCR SEE RateNuclear Physics - TheoryAstrophysics and AstronomyWe apply a Monte Carlo based integral rectangular parallel-piped (IRRP) approach to evaluate the impact of heavy ion reaction products on the Galactic Cosmic Ray (GCR) Single Event Effect (SEE) rate, concluding that owing to their similar high-energy (>100 MeV/n) SEE cross section and much larger abundance, protons are expected to be the dominating contributor. In addition, a broad set of components, ions and energies is used to explore the sub-LET threshold experimental region for standard ground-level heavy ion test energies, identifying an overall decreasing trend in the 10-80 MeV/n range due to the decreased contribution of complete and break-up fusion, and pointing out the limitations associated to the application of Monte Carlo SEE models in this energy interval.oai:inspirehep.net:16140102017 |
spellingShingle | Nuclear Physics - Theory Astrophysics and Astronomy Garcia Alia, Ruben Brugger, Markus Ferlet-Cavrois, Veronique Brandenburg, Sytze Calcutt, Jordan Cerutti, Francesco Daly, Eamonn Ferrari, Alfredo Muschitiello, Michele Santin, Giovanni Uznanski, Slawosz Van Goethem, Marc-Jan Zadeh, Ali Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title_full | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title_fullStr | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title_full_unstemmed | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title_short | Proton Dominance of Sub-LET Threshold GCR SEE Rate |
title_sort | proton dominance of sub-let threshold gcr see rate |
topic | Nuclear Physics - Theory Astrophysics and Astronomy |
url | https://dx.doi.org/10.1109/TNS.2016.2628363 http://cds.cern.ch/record/2280541 |
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