@article{oai:repo.qst.go.jp:00047204,
 author = {Ota, S. and Sihver, L. and 小林, 進悟 and Hasebe, N. and 小林 進悟},
 issue = {10},
 journal = {Advances in Space Research},
 month = {Dec},
 note = {Depth dependency of neutrons produced by cosmic rays (CRs) in the lunar subsurface was estimated using the three-dimensional
Monte Carlo particle and heavy ion transport simulation code, PHITS, incorporating the latest high energy nuclear data, JENDL/
HE-2007. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with the measurement
by Apollo 17 Lunar Neutron Probe Experiment (LNPE). Our calculations reproduced the LNPE data except for the 350–400 mg/cm2
region under the improved condition using the CR spectra model based on the latest observations, well-tested nuclear interaction models
with systematic cross section data, and JENDL/HE-2007.},
 pages = {2114--2121},
 title = {Depth dependency of neutron density produced by cosmic rays in the lunar subsurface},
 volume = {54},
 year = {2014}
}