| Peer-Reviewed

Validation of Geant4 Physics Models Relevant for Space Radiation

Received: 20 January 2017     Accepted: 15 February 2017     Published: 6 March 2017
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Abstract

In order to use GEANT4 toolkit in the energies relevant to the space radiation it has been tested few of electromagnetic and hadronic models of it by comparing simulated values with NIST data and other experimental data available. For the validation of electromagnetic models energy-loss and electronic stopping powers are considered whereas for the validation of hadronic models, isotope production cross-sections and total fragmentation cross-sections are considered. The stopping power values simulated for protons in Al are agreeing very well with NIST database values. The energy-loss and residual energy values simulated for alpha particles in Si and Al respectively are in good agreement with experimental values at high energies and low-thicknesses of target materials. The stopping power values of alpha particles and Fe ions in Al are also agreeing well with tabulated values at the small thickness of target materials. The proton - proton production cross-section values for liquid hydrogen and polyethylene are within the limits of experimental errors. Although total fragmentation cross-sections for Fe ions in polyethylene and aluminum are not agreeing with the experimental values at low energies, they are agreeing at the peak of GCR spectrum which is around 1 GeV/nucleon. So the selected physics models used in the present simulation work can be used for the space radiation protection studies.

Published in American Journal of Environmental Protection (Volume 6, Issue 1)
DOI 10.11648/j.ajep.20170601.13
Page(s) 18-25
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2017. Published by Science Publishing Group

Keywords

Geant4, Space Radiation Protection, Electromagnetic Interactions, Hadronic Interactions

References
[1] Agostinelli, S., Allison, J., Amako, K., et al., 2003, ‘GEANT4- a simulation toolkit’, Nucl. Instr. and Meth. A, vol.506, pp. 250-303.
[2] Allison, J., Amako, K., Apostolakis, J., et al., 2006, ‘Geant4 developments and applications’, IEEE Trans. Nucl. Sci., vol.53, no.1, pp. 270-278.
[3] Apostolakis, J., Asai, M., Bogdanov, A. G., et al., 2009, ‘Geometry and physics of the Geant4 toolkit for high and medium energy applications’,Radiation Physics and Chemistry, vol. 78, pp. 859-873.
[4] Apostolakis, J., Asai, M., Bagulya, A., et al., 2015, ‘Progress in Geant4 Electromagnetic Physics Modelling and Validation’, Journal of Physics: Conference Series, 664072021. doi: 10.1088 / 1742-6596/ 664/7/072021
[5] Berger, M. J., Coursey, J. S., Jucker, M. A., et al., 2005, ‘ESTAR, PSTAR and ASTAR: Computer Programs for Calculating Stopping Power and Range Tables for Electrons, Protons and Helium Ions (version1.2.3)’‹http://www. nist. gov/Star› [29 Dec 2015]
[6] Cecchini, S., Chiarusi T., Giacomelli, G., et al., 2008, ‘Fragmentation cross sections of Fe26+,Si14+ and C6+ ions of 0.3-10A GeV on polyethylene, CR39 and aluminum targets’, Nuclear Physics A, vol.807, pp. 206-213.
[7] Durante, M., and Francis A. Cucinotta., 2011, ‘Physical basis of radiation protection in space travel’, Rev. Mod. Phys., vol.83, no.4, pp. 1245-1281.
[8] Filomena Loffredo, Mariagabriella Pugliese, Maria Quarto et al., 2015,‘Validation of Electromagnetic Physical Processes with Software SPENVIS’,Vol.4,no.6,pp.275-278. doi:10.11648 / j. ajep.20150406.12
[9] Geant4 Physics Reference Manual ‹www://geant4.web.cern.Ch /geant4/UserDocumentation/UserGuides/PhysicsReferenceManual /fo/PhysicsReferenceManual. pdf› [14 Oct 2015]
[10] Hubert, F., Rimbot, R., Gauvin, H., et al., 1990, ‘Range and Stopping-Power Tables for 2.5 – 500 MeV/nucleon Heavy Ions in Solids’, Atomic Data and Nuclear Data Tables, vol.46, pp. 1-213.
[11] Li-Chun Wang, Dong-Hai Zhang, Shiwei Yan et al., 2012, ‘Fragmentation cross sections of 56Fe at 471 A MeV on Al, C and CH2 Targets’, Acta Physica Polonica B, vol.43, no.8, pp. 1769-1782.
[12] Makato Asai, Andrea Dotti., Marc Verderi., et al., 2014, ‘Recent Developments in Geant4’, Ann. Nucl. Energy. ‹http://dx. doi.org /10.1016/j. anucene.2014.08.021›
[13] Mudundi R. Raju, 1965, ‘Heavy particle studies with silicon detectors’, University of California Research Laboratory Report, UCRL- 16354.
[14] Schwaller, P., Pepin, H., Favier, B., et al., 1979, ‘Proton total cross-sections on 1H, 2H 4He,9Be, C and O in the energy range 180 to 560 MeV’, Nucl. Phy. A, vol.316, pp. 317-344.
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  • APA Style

    V. Satya Prakash. (2017). Validation of Geant4 Physics Models Relevant for Space Radiation. American Journal of Environmental Protection, 6(1), 18-25. https://doi.org/10.11648/j.ajep.20170601.13

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    ACS Style

    V. Satya Prakash. Validation of Geant4 Physics Models Relevant for Space Radiation. Am. J. Environ. Prot. 2017, 6(1), 18-25. doi: 10.11648/j.ajep.20170601.13

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    AMA Style

    V. Satya Prakash. Validation of Geant4 Physics Models Relevant for Space Radiation. Am J Environ Prot. 2017;6(1):18-25. doi: 10.11648/j.ajep.20170601.13

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  • @article{10.11648/j.ajep.20170601.13,
      author = {V. Satya Prakash},
      title = {Validation of Geant4 Physics Models Relevant for Space Radiation},
      journal = {American Journal of Environmental Protection},
      volume = {6},
      number = {1},
      pages = {18-25},
      doi = {10.11648/j.ajep.20170601.13},
      url = {https://doi.org/10.11648/j.ajep.20170601.13},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajep.20170601.13},
      abstract = {In order to use GEANT4 toolkit in the energies relevant to the space radiation it has been tested few of electromagnetic and hadronic models of it by comparing simulated values with NIST data and other experimental data available. For the validation of electromagnetic models energy-loss and electronic stopping powers are considered whereas for the validation of hadronic models, isotope production cross-sections and total fragmentation cross-sections are considered. The stopping power values simulated for protons in Al are agreeing very well with NIST database values. The energy-loss and residual energy values simulated for alpha particles in Si and Al respectively are in good agreement with experimental values at high energies and low-thicknesses of target materials. The stopping power values of alpha particles and Fe ions in Al are also agreeing well with tabulated values at the small thickness of target materials. The proton - proton production cross-section values for liquid hydrogen and polyethylene are within the limits of experimental errors. Although total fragmentation cross-sections for Fe ions in polyethylene and aluminum are not agreeing with the experimental values at low energies, they are agreeing at the peak of GCR spectrum which is around 1 GeV/nucleon. So the selected physics models used in the present simulation work can be used for the space radiation protection studies.},
     year = {2017}
    }
    

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  • TY  - JOUR
    T1  - Validation of Geant4 Physics Models Relevant for Space Radiation
    AU  - V. Satya Prakash
    Y1  - 2017/03/06
    PY  - 2017
    N1  - https://doi.org/10.11648/j.ajep.20170601.13
    DO  - 10.11648/j.ajep.20170601.13
    T2  - American Journal of Environmental Protection
    JF  - American Journal of Environmental Protection
    JO  - American Journal of Environmental Protection
    SP  - 18
    EP  - 25
    PB  - Science Publishing Group
    SN  - 2328-5699
    UR  - https://doi.org/10.11648/j.ajep.20170601.13
    AB  - In order to use GEANT4 toolkit in the energies relevant to the space radiation it has been tested few of electromagnetic and hadronic models of it by comparing simulated values with NIST data and other experimental data available. For the validation of electromagnetic models energy-loss and electronic stopping powers are considered whereas for the validation of hadronic models, isotope production cross-sections and total fragmentation cross-sections are considered. The stopping power values simulated for protons in Al are agreeing very well with NIST database values. The energy-loss and residual energy values simulated for alpha particles in Si and Al respectively are in good agreement with experimental values at high energies and low-thicknesses of target materials. The stopping power values of alpha particles and Fe ions in Al are also agreeing well with tabulated values at the small thickness of target materials. The proton - proton production cross-section values for liquid hydrogen and polyethylene are within the limits of experimental errors. Although total fragmentation cross-sections for Fe ions in polyethylene and aluminum are not agreeing with the experimental values at low energies, they are agreeing at the peak of GCR spectrum which is around 1 GeV/nucleon. So the selected physics models used in the present simulation work can be used for the space radiation protection studies.
    VL  - 6
    IS  - 1
    ER  - 

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Author Information
  • Department of Physics, Government Degree College, Medak, India

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