Geometric Cross Sections of Dust Aggregates and a Compression Model for Aggregate Collisions
Geometric Cross Sections of Dust Aggregates and a Compression Model for Aggregate Collisions
复制标题
灰尘聚集体的几何横截面和聚集体碰撞的压缩模型
DOI:
10.1088/0004-637x/753/2/115
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发表时间:
2012
期刊:
影响因子:
--
通讯作者:
Tom Suyama
中科院分区:
文献类型:
--
作者:
田中有弥;野口裕;石井久夫;岡本卓也;Tom Suyama
Geometric cross sections of dust aggregates determine their coupling with disk gas, which governs their motions in protoplanetary disks. Collisional outcomes also depend on geometric cross sections of initial aggregates. In a previous paper, we performed three-dimensional N-body simulations of sequential collisions of aggregates composed of a number of sub-micron-sized icy particles and examined radii of gyration (and bulk densities) of the obtained aggregates. We showed that collisional compression of aggregates is not efficient and that aggregates remain fluffy. In the present study, we examine geometric cross sections of the aggregates. Their cross sections decrease due to compression as well as to their gyration radii. It is found that a relation between the cross section and the gyration radius proposed by Okuzumi et al. is valid for the compressed aggregates. We also refine the compression model proposed in our previous paper. The refined model enables us to calculate the evolution of both gyration radii and cross sections of growing aggregates and reproduces well our numerical results of sequential aggregate collisions. The refined model can describe non-equal-mass collisions as well as equal-mass cases. Although we do not take into account oblique collisions in the present study, oblique collisions would further hinder compression of aggregates.