Neutron Production in the Lunar Subsurface from Galactic Cosmic Ray Nuclei

Physics – Medical Physics

Scientific paper

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Scientific paper

The neutron production from galactic cosmic ray (GCR) protons and alpha particles in the lunar subsurface was estimated using the three-dimensional Monte Carlo simulation code PHITS, together with GCR input spectra based on the BESS measurements. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with experimental data by Apollo 17 Lunar Neutron Probe Experiment. By use of accurate spectra and nuclear interaction models, our calculations successfully reproduced the data within the experimental error at the shallower region than 300 g/cm2. However, our calculation was up to 30% higher in the deeper region.

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