@techreport{oai:jaxa.repo.nii.ac.jp:00041869,
 author = {森本, 久雄 and 亀井, 信一 and 伊丹, 俊夫 and Morimoto, Hisao and Kamei, Shinichi and Itami, Toshio},
 month = {Mar},
 note = {2成分剛体球混合物に対する分子動力学シミュレーションから、原子あるいはEinsteinの関係式の速度相関関数と平均2乗変位の両方に基づいて自己および相互拡散係数を計算した。後者の事例では、満足すべき後方散乱係数の挙動が得られた。求めた後方散乱係数は1成分剛体球の事例と類似している。相互拡散係数は、各自己拡散係数間の粒子数比の線形関係式と10%以内で一致した。拡散機構に及ぼす質量差の役割の幾つかを論じた。, From molecular dynamics simulations for binary hard sphere mixtures, the self- and mutual diffusion coefficients were calculated based on both velocity correlation functions and the mean square displacements of atoms or Einstein relation. Satisfactory behavior of the back scattering factor was obtained in the latter case. The obtained back scattering factor is similar to the case of one component hard spheres. The mutual diffusion coefficient was, within ten percent, in agreement with the linear relation of particle number ratio between respective self-diffusion coefficients. Some discussions were given for the role of mass difference on the mechanism of diffusion., 資料番号: AA0029039010, レポート番号: NASDA-TMR-000013E},
 title = {Molecular dynamics simulation of hard sphere mixtures},
 year = {2001}
}