Fragmentation with discontinuous Galerkin schemes: non-linear fragmentation

被引:10
作者
Lombart, Maxime [1 ]
Hutchison, Mark [2 ]
Lee, Yueh-Ning [1 ]
机构
[1] Natl Taiwan Normal Univ, Dept Earth Sci, 88,Sec 4,Ting Chou Rd, Taipei 11677, Taiwan
[2] Ludwig Maximilians Univ Munchen, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany
基金
欧盟地平线“2020”; 欧洲研究理事会;
关键词
methods: numerical; dust; extinction; FINITE-VOLUME SCHEME; SIZE DISTRIBUTION; DUST COAGULATION; NUMERICAL-SIMULATION; CONVERGENCE ANALYSIS; KINETICS; AGGREGATION; PARTICLES; GRAINS; DISKS;
D O I
10.1093/mnras/stac2232
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Small grains play an essential role in astrophysical processes such as chemistry, radiative transfer, and gas/dust dynamics. The population of small grains is mainly maintained by the fragmentation process due to colliding grains. An accurate treatment of dust fragmentation is required in numerical modelling. However, current algorithms for solving fragmentation equation suffer from an overdiffusion in the conditions of 3D simulations. To tackle this challenge, we developed a discontinuous Galerkin scheme to solve efficiently the non-linear fragmentation equation with a limited number of dust bins.
引用
收藏
页码:2012 / 2027
页数:16
相关论文
共 73 条
[1]   Observations of Protoplanetary Disk Structures [J].
Andrews, Sean M. .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 58, 2020, 58 :483-528
[2]  
[Anonymous], 2000, Smoke, Dust, and Haze-Fundamentals of Aerosol Dynamics
[3]  
[Anonymous], 1957, Trans. Amer. Math. Soc.
[4]  
[Anonymous], 1928, Kolloidchemische Beihefte, DOI DOI 10.1007/BF02558510
[5]   INTRODUCTION TO MATHEMATICAL DESCRIPTION OF GRINDING AS A RATE PROCESS [J].
AUSTIN, LG .
POWDER TECHNOLOGY, 1971, 5 (01) :1-&
[6]  
Banasiak J., 2019, ANAL METHODS COAGULA
[7]   Dust Evolution and the Formation of Planetesimals [J].
Birnstiel, T. ;
Fang, M. ;
Johansen, A. .
SPACE SCIENCE REVIEWS, 2016, 205 (1-4) :41-75
[8]   Gas- and dust evolution in protoplanetary disks [J].
Birnstiel, T. ;
Dullemond, C. P. ;
Brauer, F. .
ASTRONOMY & ASTROPHYSICS, 2010, 513
[9]   Dust Evolution in Protoplanetary Discs and the Formation of Planetesimals What Have We Learned from Laboratory Experiments? [J].
Blum, Juergen .
SPACE SCIENCE REVIEWS, 2018, 214 (02)
[10]   The fossilized size distribution of the main asteroid belt [J].
Bottke, WF ;
Durda, DD ;
Nesvorny, D ;
Jedicke, R ;
Morbidelli, A ;
Vokrouhlicky, D ;
Levison, H .
ICARUS, 2005, 175 (01) :111-140