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We present an experimental study of the statistical properties of millimeter-size spheres floating on the surface of a turbulent flow. The flow is generated in a layer of liquid metal by an electromagnetic forcing. By using two magnet…

流体动力学 · 物理学 2016-07-04 Pablo Gutiérrez , Sébastien Aumaître

We consider advection of small inertial particles by a random fluid flow with a strong steady shear component. It is known that inertial particles suspended in a random flow can exhibit clusterization even if the flow is incompressible. We…

混沌动力学 · 物理学 2013-05-30 Grigory A. Sizov

We propose a simple model for periodic clustering of particles under forced oscillation. Effective viscosity is assumed to increase owing to neighboring particles by analogy with the Einstein viscosity law. The linear stability analysis and…

斑图形成与孤子 · 物理学 2026-02-12 Hidetsugu Sakaguchi

Granular fronts are a common yet unexplained phenomenon emerging during the gravity driven free-surface flow of concentrated suspensions. They are usually believed to be the result of fluid convection in combination with particle size…

软凝聚态物质 · 物理学 2015-12-02 A. Leonardi , M. Cabrera , F. K. Wittel , R. Kaitna , M. Mendoza , W. Wu , H. J. Herrmann

We report and analyze the results of numerical studies of dense granular flows in two and three dimensions, using both linear damped springs and Hertzian force laws between particles. Chute flow generically produces a constant density…

软凝聚态物质 · 物理学 2009-10-31 Deniz Ertas , Gary S. Grest , Thomas C. Halsey , Dov Levine , Leonardo E. Silbert

To understand the process of pattern formation in a low-density granular flow, we propose a simple particle model. This model considers spherical particles moving over an inclined flat surface based on three forces: gravity as the driving…

软凝聚态物质 · 物理学 2019-04-24 Hirofumi Niiya , Akinori Awazu , Hiraku Nishimori

Small heavy particles cannot get attracted into a region of closed streamlines in a non-accelerating frame (Sapsis & Haller 2010). In a rotating system, however, particles can get trapped (Angilella 2010) near vortices. We perform numerical…

流体动力学 · 物理学 2025-02-12 Saumav Kapoor , Divya Jaganathan , Rama Govindarajan

Dense granular flows are often unstable and form inhomogeneous structures. Although significant advances have been recently made in understanding simple flows, instabilities of such flows are often not understood. We present experimental…

软凝聚态物质 · 物理学 2009-10-02 Tamas Borzsonyi , Robert E. Ecke , Jim N. McElwaine

We describe a new approach to gravitational instability in large-scale structure, where the equations of motion are written and solved as in field theory in terms of Feynman diagrams. The basic objects of interest are the propagator (which…

天体物理学 · 物理学 2015-06-24 Roman Scoccimarro

We study the motion of an inertial particle in a fractional Gaussian random field. The motion of the particle is described by Newton's second law, where the force is proportional to the difference between a background fluid velocity and the…

动力系统 · 数学 2012-03-20 Georg Schöchtel

Direct numerical simulation is used to investigate effects of turbulent flow in the confined geometry of a face-centered cubic porous unit cell on the transport, clustering, and deposition of fine particles at different Stokes numbers ($St…

流体动力学 · 物理学 2022-12-09 Sourabh V. Apte , Thibault Oujia , Keigo Matsuda , Benjamin Kadoch , Xiaoliang He , Kai Schneider

A new model that describes adsorption and clustering of particles on a surface is introduced. A {\it clustering} transition is found which separates between a phase of weakly correlated particle distributions and a phase of strongly…

统计力学 · 物理学 2009-10-31 Ofer Biham , Ofer Malcai , Daniel A. Lidar , David Avnir

To understand the earliest stages of planet formation, it is crucial to be able to predict the rate and the outcome of dust grains collisions, be it sticking and growth, bouncing, or fragmentation. The outcome of such collisions depends on…

地球与行星天体物理 · 物理学 2015-06-05 Alexander Hubbard

Solid particles in protoplanetary disks that are sufficiently super-solar in metallicity overcome turbulence generated by vertical shear to gravitationally condense into planetesimals. Super-solar metallicities result if solid particles…

天体物理学 · 物理学 2009-11-10 Andrew N. Youdin , Eugene I. Chiang

Superconductivity, superfluidity, condensation, cluster formation, etc. are phenomena that might occur in many-particle systems. These are due to residual interactions between the particles. To explain these phenomena consistently in a…

核理论 · 物理学 2007-05-23 Michael Beyer

Preferential concentration of inertial particles in turbulent flow is studied by high resolution direct numerical simulations of two-dimensional turbulence. The formation of network-like regions of high particle density, characterized by a…

混沌动力学 · 物理学 2009-11-10 G. Boffetta , F. De Lillo , A. Gamba

We consider a physical system comprising discrete massive particles on the real line whose trajectories interact via perfectly inelastic collision, also known as sticky particles. It turns out that polygons formed in a convex "cumulative…

动力系统 · 数学 2021-09-15 Chun-Kai Kevin Chien , Aidan Mager , Laurel Safranek , Jackson Zariski

We study size- and charge-asymmetric oppositely charged colloids driven by an external electric field. The large particles are connected by harmonic springs, forming a hexagonal-lattice network while the small particles are free of bonds…

软凝聚态物质 · 物理学 2023-04-24 Dingwen Qian , Monica Olvera de la Cruz

We present a new instability observed in rapid granular flows down rough inclined planes. For high inclinations and flow rates, the free surface of the flow experiences a regular deformation in the transverse direction. Measurements of the…

软凝聚态物质 · 物理学 2009-11-07 Yoel Forterre , Olivier Pouliquen

We use two high resolution CDM simulations to show that (i) when clusters of galaxies form the infall pattern of matter is not random but shows clear features which are correlated in time; (ii) in addition, the infall patterns are…

天体物理学 · 物理学 2007-05-23 J. M. Colberg , S. D. M. White , A. Jenkins , F. R. Pearce