Title :
Modeling of secondary neutron production from space radiation interactions
Author :
Braley, G. Scott ; Townsend, Lawrence W. ; Cucinotta, Francis A. ; Heilbronn, Lawrence H.
Author_Institution :
Armed Forces Radiobiol. Res. Inst., Bethesda, MD, USA
fDate :
12/1/2002 12:00:00 AM
Abstract :
A knockout-ablation-coalescence model capable of making quantitative predictions of neutron spectra produced in high-energy nucleon-nucleus and nucleus-nucleus collisions is presented. A Glauber model is used to describe neutrons produced in the knockout or abrasion stage of the reaction. In the ablation stage, a statistical evaporation model is used to calculate the neutron spectrum produced by the excited prefragment nucleus left over from the abrasion stage. The effects of coalescence in reducing free neutron emission by composite particle formation are included. Typical results for predicted neutron energy and double-differential spectra are presented and compared with recently reported measurements for a variety of projectile and target nuclei of interest in space radiation protection. Except for differences resulting from the neglect of isobar production and decay in the model, predictions are in fairly good agreement with the measured data.
Keywords :
evaporation model; heavy ion-nucleus reactions; knock-out reactions; neutron production; nuclear optical model; nucleon-nucleus reactions; shielding; space vehicles; statistical models (nuclear); (N,X); Glauber model; abrasion stage; composite particle formation; double-differential spectra; free neutron emission; heavy ion collisions; high-energy nucleon-nucleus collisions; isobar production; knockout-ablation-coalescence model; neutron energy spectra; neutron spectra; nucleus-nucleus collisions; secondary neutron production modeling; space radiation interactions; statistical evaporation model; Extraterrestrial measurements; Mars; Moon; Neutrons; Nuclear measurements; Predictive models; Production; Projectiles; Space vehicles; Terrestrial atmosphere;
Journal_Title :
Nuclear Science, IEEE Transactions on
DOI :
10.1109/TNS.2002.805343