Table 3 Interaction model options in the PHITS (* denotes the default model).
From: Neutron production in the lunar subsurface from alpha particles in galactic cosmic rays
Particle | Model options (E denotes the kinetic energy of particle) |
|---|---|
Proton | Bertini Free (1 MeV < E < 3.5 GeV) + *JAM (E > 3.5 GeV) |
| Â | *Bertini Cugnon Old (1 MeV < E < 3.5 GeV) + *JAM (E > 3.5 GeV) |
| Â | Bertini Cugnon New (1 MeV < E < 3.5 GeV) + *JAM (E > 3.5 GeV) |
| Â | Isober (1 MeV < E < 1 GeV) + *Bertini Cugnon Old (1 GeV < E < 3.5 GeV) + * JAM (E > 3.5 GeV) |
| Â | JAM (E > 1 MeV) |
| Â | JQMD (E > 1 MeV) |
| Â | JAMQMD (E > 1MeV) |
Alpha | JQMD (E > 10 MeV/n) |
| Â | JAMQMD (E > 10 MeV/n) |