Geometrical structure and thermal conductivity of dust aggregates formed via ballistic cluster-cluster aggregation
arXiv:1908.03125 · doi:10.1093/ptep/ptz102
Abstract
We herein report a theoretical study of the geometrical structure of porous dust aggregates formed via ballistic cluster-cluster aggregation (BCCA). We calculated the gyration radius and the graph-based geodesic radius as a function of the number of constituent particles . We found that and , where is the radius of constituent particles. Furthermore, we defined two constants that characterize the geometrical structure of fractal aggregates: and . The definition of and are and , respectively. Our study revealed that and for the clusters of the BCCA. In addition, we also studied the filling factor dependence of thermal conductivity of statically compressed fractal aggregates. From this study, we reveal that the thermal conductivity of statically compressed aggregates is given by , where is the material thermal conductivity, is the contact radius of constituent particles, and is the filling factor of dust aggregates.
14 pages, 8 figures. Accepted for publication in PTEP
References in corpus (10)
- The Physics of Protoplanetesimal Dust Agglomerates. IV. Towards a Dynamical Collision Model
- Microphysical Modeling of Mineral Clouds in GJ1214 b and GJ436 b: Predicting Upper Limits on the Cloud-Top Height
- Tensile Strength of Porous Dust Aggregates
- Compression Behaviour of Porous Dust Agglomerates
- Rocky Planetesimal Formation via Fluffy Aggregates of Nanograins
- Experimental study on compression property of regolith analogues
- Thermal conductivity of porous aggregates
- Thermal conductivity and coordination number of compressed dust aggregates
- Estimating the porosity structure of granular bodies using the Lane-Emden equation applied to laboratory measurements of the pressure-density relation of fluffy granular samples
- Gravitational instability of a dust layer composed of porous silicate dust aggregates in a protoplanetary disk
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- Investigating the Bouncing Barrier with Collision Simulations of Compressed Dust Aggregates
- On the elastoplastic behavior in collisional compression of spherical dust aggregates
- Interpebble contact radius in a comet nucleus
- Interparticle normal force in highly porous granular matter during compression
- Root mean squares of distance and geodesic between two constituent particles within fractal aggregates prepared by BCCA, DLA, and GSAW procedures
- Numerical Investigation on the Compressive Behavior of Hierarchical Granular Piles