2012
DOI: 10.21236/ada554870
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Neutron-Activated Gamma-Emission: Technology Review

Abstract: Public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, searching existing data sources, gathering and maintaining the data needed, and completing and reviewing the collection information. Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing the burden, to Department of Defense, Washington Headquarters Services, Directorate for Informat… Show more

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Cited by 7 publications
(2 citation statements)
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“…The reaction channel opens at a threshold energy recorded over 10 keV and mainly around 100 keV for heavy nuclei and a few MeV for light nuclei [58]. The maximum inelastic cross section is around 5 barns while for most nuclei it is around 1 barn [59]. Regarding the goal of the current investigation, the advantages of inelastic scattering in comparison to elastic are related to the substantial energy loss during collisions, as well as to the energy range where the reaction occurs, that is, in high energies.…”
Section: Effect Of Materials With Important Inelastic Scatteringmentioning
confidence: 99%
“…The reaction channel opens at a threshold energy recorded over 10 keV and mainly around 100 keV for heavy nuclei and a few MeV for light nuclei [58]. The maximum inelastic cross section is around 5 barns while for most nuclei it is around 1 barn [59]. Regarding the goal of the current investigation, the advantages of inelastic scattering in comparison to elastic are related to the substantial energy loss during collisions, as well as to the energy range where the reaction occurs, that is, in high energies.…”
Section: Effect Of Materials With Important Inelastic Scatteringmentioning
confidence: 99%
“…One can consider that all constituent materials of an S-type asteroid that can be activated during an explosion have a very short decay time in general and all decay emitting β or α particles. For example, silica has isotopes with a decay time that ranges from 60 ns for Si High energy neutrons can only be spontaneously generated by the decay of heavy atoms that cannot come from the core of the asteroid post explosion (Litz et al , 2012). Neutron activation on the antipodal side is also not possible, neither neutron scattering.…”
Section: Post-explosion Radiation Exposurementioning
confidence: 99%