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Planet formation in the discs around young stars involves the coagulation of sub-micron sized dust grains into much larger grains that may be mixed by turbulence and migrate through the disc. In this paper, we describe how we have combined…

地球与行星天体物理 · 物理学 2026-02-04 Matthew R. Bate , Mark A. Hutchison , Daniel Elsender

This study employed grain dynamic models to examine the density distribution of debris discs, and discussed the effects of the collisional time-intervals of asteroidal bodies, the maximum grain sizes, and the chemical compositions of the…

太阳与恒星天体物理 · 物理学 2010-11-02 Ing-Guey Jiang , Li-Chin Yeh

We consider a fiber bundle model with a equal load sharing and uniformly distributed breakdown thresholds. A unified probability-theoretic approach was used to describe bundle under continuous and discrete load increase. It was shown that…

无序系统与神经网络 · 物理学 2012-02-14 I. V. Bezsudnov , A. A. Snarskii

Many dense granular systems are non-monodisperse, consisting of particles of different sizes, and will segregate based on size during flow. This phenomenon is an important aspect of many industrial and geophysical processes, necessitating…

软凝聚态物质 · 物理学 2024-05-28 Harkirat Singh , David L. Henann

Granular intrusion is commonly observed in natural and human-made settings. Unlike typical solids and fluids, granular media can simultaneously display fluid-like and solid-like characteristics in a variety of intrusion scenarios. This…

软凝聚态物质 · 物理学 2021-07-16 Shashank Agarwal , Andras Karsai , Daniel I Goldman , Ken Kamrin

Conventional grain growth is rate-limited by the mobility of grain boundary. To describe similar phenomena limited by the mobility of other grain junctions, we have developed a general theory allowing for size-dependent mobility and its…

材料科学 · 物理学 2017-08-16 Yanhao Dong , I-Wei Chen

Dust plays a key role in the evolution of the ISM and its correct modelling in numerical simulations is therefore fundamental. We present a new and self-consistent model that treats grain thermal coupling with the gas, radiation balance,…

星系天体物理 · 物理学 2017-01-25 T. Grassi , S. Bovino , T. Haugboelle , D. R. G. Schleicher

We present a reduced-dimension, ballistic deposition, Monte Carlo particle packing algorithm and discuss its application to the analysis of the microstructure of hard-sphere systems with broad particle size distributions. We extend our…

材料科学 · 物理学 2007-05-23 M. D. Webb , I. L. Davis

Ripples or corrugations are common phenomena observed in unpaved roads in less developed countries or regions. They cause several damages in vehicles leading to increased maintenance and product costs. In this paper, we present a…

软凝聚态物质 · 物理学 2019-01-31 Tiago Moy da Silva , Americo T. Bernardes

A two-dimensional, transient, multi-scale modeling approach is presented for predicting the magnitude and rate of percolation segregation for binary mixtures of granular material in a rotating drum and conical hopper. The model utilizes…

软凝聚态物质 · 物理学 2018-10-08 Yu Liu , Marcial Gonzalez , Carl Wassgren

We model the effect of grain size distribution in a galaxy on the evolution of CO and H$_2$ abundances. The formation and dissociation of CO and H$_2$ in typical dense clouds are modelled in a manner consistent with the grain size…

星系天体物理 · 物理学 2023-05-10 Hiroyuki Hirashita

We study the role of the unknown microphysical properties of carbonaceous dust particles in determining the amount and size distribution of carbonaceous dust condensed in type II supernova explosions. We parametrize the microphysical…

太阳与恒星天体物理 · 物理学 2015-05-28 David W. Fallest , Takaya Nozawa , Ken'ichi Nomoto , Hideyuki Umeda , Keiichi Maeda , Takashi Kozasa , Davide Lazzati

We study the local and global roughness scaling in growth models with grains at the film surfaces. The local roughness, measured as a function of window size r, shows a crossover at a characteristic length r_c, from a rapid increase with…

统计力学 · 物理学 2007-05-23 T. J. Oliveira , F. D. A. Aarao Reis

The paper develops the stiffness relationship between the movements and forces among a system of discrete interacting grains. The approach is similar to that used in structural analysis, but the stiffness matrix of granular material is…

软凝聚态物质 · 物理学 2019-05-01 Matthew R. Kuhn , Florent Prunier , Ali Daouadji

We present a method for simulating the dynamics of a mixture of gas and multiple species of large Stokes number dust grains, typical of evolved protoplanetary discs and debris discs. The method improves upon earlier methods, in which only a…

地球与行星天体物理 · 物理学 2020-10-27 Daniel Mentiplay , Daniel J. Price , Christophe Pinte , Guillaume Laibe

We test grip strength and shock absorption properties of various granular material in granular jamming robotic components. The granular material comprises a range of natural, manufactured, and 3D printed material encompassing a wide range…

机器人学 · 计算机科学 2022-12-14 David Howard , Jack O'Connor , Jordan Letchford , Therese Joseph , Sophia Lin , Sarah Baldwin , Gary Delaney

Analysis of thermal dust emission spectra for dust mineralogy and physical grain properties depends on laboratory-measured or calculated comparison spectra. Often, the agreement between these two kinds of spectra is not satisfactory because…

天体物理仪器与方法 · 物理学 2015-05-13 H. Mutschke , M. Min , A. Tamanai

Model pruning is a popular approach to enable the deployment of large deep learning models on edge devices with restricted computational or storage capacities. Although sparse models achieve performance comparable to that of their dense…

Diffusion probabilistic models (DPMs) have emerged as a promising technique in generative modeling. The success of DPMs relies on two ingredients: time reversal of diffusion processes and score matching. In view of possibly unguaranteed…

机器学习 · 计算机科学 2024-10-15 Wenpin Tang , Hanyang Zhao

We calculate the absorption efficiency of the composite grains, made up of host silicate spheroids and inclusions of ices/graphites/or voids, in the spectral region $7.0-14.0\mu$m The absorption efficiencies of the composite spheroidal…

星系天体物理 · 物理学 2009-04-03 Deepak B. Vaidya , Ranjan Gupta