日本地球惑星科学連合2019年大会

講演情報

[J] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS06] 惑星科学

2019年5月28日(火) 09:00 〜 10:30 A01 (東京ベイ幕張ホール)

コンビーナ:黒崎 健二(名古屋大学大学院 理学研究科 素粒子宇宙物理学専攻)、仲内 悠祐(宇宙航空研究開発機構)、座長:末次 竜(産業医科大学)、杉浦 圭祐(名古屋大学)

09:15 〜 09:30

[PPS06-26] 塵粒子集合体のグラフ構造から理解する熱伝導率の充填率依存性

*荒川 創太1竹本 正輝1中本 泰史1 (1.東京工業大学理学院)

キーワード:熱伝導率、ダストアグリゲイト、粉粒体

Previous studies (Arakawa et al. 2017; 2019) revealed that the thermal conductivity through the solid network of dust aggregates is proportional to the square of the filling factor. However, the reason why the thermal conductivity is given by the power-law function of the filling factor was still unclear. In order to understand the physical reason of this power-law dependence, we need to investigate the geometric structure of highly porous dust aggregates.
In this study, we study the graph structure of fractal aggregates called BCCA aggregates (e.g., Meakin 1991). The fractal dimension of BCCA aggregates is approximately 1.9 (e.g., Okuzumi et al. 2009) and the graph structure of BCCA aggregates is classified as a tree. Then the gyration radius rg and the filling factor φ is connected by the following equation, rgφ−1/(3−1.9), and the number of the heat conduction path per unit area, σ, is given by σφ2/(3−1.9) for BCCA aggregates. In addition, we calculated the graph-theoretical distances of monomer grains within a BCCA aggregate. We found that the root mean square of the graph-theoretical distance d is given by drg1.2. Therefore, the thermal conductivity of BCCA aggregates is proportional to σrg/dφ2.