Neutron yields from interactions of GCR-like beams in stopping targets.
In order to accurately determine the radiation risk to astronauts from GCR, the nature of the secondary radiation field created by the fragmentation of GCR in shielding and tissue must be understood.  Due to the their high penetrabilities, neutrons are an important component of the secondary radiation field, especially for astronauts protected by thick shielding on lunar or Martian bases.  Neutron yields from 435A MeV and 272A MeV Nb stopping in Nb and Al targets are presented, along with some preliminary analysis of neutron yields from 155A MeV C stopping in Al.  Energy spectra and angular distributions are shown for neutron energies above 20 MeV.  The data provides some information about the dependence of the neutron yield on projectile energy and target mass.  Comparisons of the data with BUU calculations are also shown.
Heilbronn
L
L
Lawrence Berkeley Laboratory, Berkeley, CA 94720, USA.
D000535:Aluminum; D018480:Astronauts; D002244:Carbon; D003359:Cosmic Radiation; D016208:Databases, Factual; D019471:Elementary Particle Interactions; D006371:Helium; D006801:Humans; D008962:Models, Theoretical; D009502:Neutrons; D009556:Niobium; D010315:Particle Accelerators; D011835:Radiation Protection; D012306:Risk
D009556:Niobium; D006371:Helium; D002244:Carbon; D000535:Aluminum