多相流动的光滑粒子流体动力学方法研究综述

陈飞国, 葛蔚 - 力学学报, 2021 - lxxb.cstam.org.cn
光滑粒子流体动力学(smoothed particle hydrodynamics, SPH) 具有粒子方法的无网格和全拉
格朗日特征, 适用于具有界面大变形, 不连续性和多物理场的多相流的高精度模拟. SPH …

Effects of impact and target parameters on the results of a kinetic impactor: predictions for the Double Asteroid Redirection Test (DART) mission

AM Stickle, ME DeCoster, C Burger… - The planetary …, 2022 - iopscience.iop.org
Abstract The Double Asteroid Redirection Test (DART) spacecraft will impact into the
asteroid Dimorphos on 2022 September 26 as a test of the kinetic impactor technique for …

A review of smoothed particle hydrodynamics family methods for multiphase flow

C Feiguo, G Wei - Chinese Journal of Theoretical and Applied …, 2021 - lxxb.cstam.org.cn
With meshfree and fully Lagrangian features of particle methods, smoothed particle
hydrodynamics (SPH) is suitable to achieve high-accurate simulations of multiphase flows …

Binary orbital evolution driven by a circumbinary disc

ABT Penzlin, W Kley, H Audiffren… - Astronomy & …, 2022 - aanda.org
The question whether the interaction of a circumbinary disc with the central binary system
leads to a shrinking or to an expansion of the binary orbit has attracted considerable interest …

New versus past silica crush curve experiments: application to Dimorphos benchmarking impact simulations

U Malamud, CM Schäfer, IL San Sebastián… - The Astrophysical …, 2024 - iopscience.iop.org
Crush curves are of fundamental importance to numerical modeling of small and porous
astrophysical bodies. The empirical literature often measures them for silica grains, and …

Building terrestrial planets: why results of perfect-merging simulations are not quantitatively reliable approximations to accurate modeling of terrestrial planet formation

N Haghighipour, TI Maindl - The Astrophysical Journal, 2022 - iopscience.iop.org
Although it is accepted that perfect-merging is not a realistic outcome of collisions, some
researchers state that perfect-merging simulations can still be considered as quantitatively …

Protoplanet collisions: New scaling laws from smooth particle hydrodynamics simulations

S Crespi, M Ali-Dib, I Dobbs-Dixon - Astronomy & Astrophysics, 2024 - aanda.org
One common approach for solving collisions between protoplanets in simulations of planet
formation is to employ analytical scaling laws. The most widely used one was developed by …

Protoplanet collisions: new scaling laws from SPH simulations

S Crespi, M Ali-Dib, I Dobbs-Dixon - arXiv preprint arXiv:2402.07803, 2024 - arxiv.org
One common approach for solving collisions between protoplanets in simulations of planet
formation is to employ analytical scaling laws. The most widely used one was developed by …

Protoplanet collisions: Statistical properties of ejecta

S Crespi, I Dobbs-Dixon… - Monthly Notices of …, 2021 - academic.oup.com
The last phase of the formation of rocky planets is dominated by collisions among Moon-to
Mars-sized planetary embryos. Simulations of this phase need to handle the difficulty of …

Residual neural networks for the prediction of planetary collision outcomes

PM Winter, C Burger, S Lehner, J Kofler… - Monthly Notices of …, 2023 - academic.oup.com
Fast and accurate treatment of collisions in the context of modern N-body planet formation
simulations remains a challenging task due to inherently complex collision processes. We …