Light ion components of the galactic cosmic rays:  nuclear interactions and transport theory.
Light nuclei are present in the primary galactic cosmic rays (GCR) and are produced in thick targets due to projectile or target fragmentation from both nucleon and heavy ion induced reactions. In the primary GCR, 4He is the most abundant nucleus after 1H. However, there are also a substantial fluxes of 2H and 3He. In this paper we describe theoretical models based on quantum multiple scattering theory for the description of light ion nuclear interactions. The energy dependence of the light ion fragmentation cross section is considered with comparisons of inclusive yields and secondary momentum distributions to experiments described. We also analyze the importance of a fast component of lights ions from proton and neutron induced target fragmentation. These theoretical models have been incorporated into the cosmic ray transport code HZETRN and will be used to analyze the role of shielding materials in modulating the production and the energy spectrum of light ions.
Cucinotta
F A
FA
NASA Langley Research Center, Hampton, VA 23681-0001, USA.
Townsend
L W
LW
Wilson
J W
JW
Shinn
J L
JL
Badhwar
G D
GD
Dubey
R R
RR
D003359:Cosmic Radiation; D019471:Elementary Particle Interactions; D006371:Helium; D006859:Hydrogen; D007477:Ions; D007554:Isotopes; D008962:Models, Theoretical; D009502:Neutrons; D009686:Nuclear Physics; D011522:Protons; D011789:Quantum Theory; D011835:Radiation Protection; D012542:Scattering, Radiation; D014316:Tritium
D007477:Ions; D007554:Isotopes; D011522:Protons; D014316:Tritium; D006371:Helium; D006859:Hydrogen