中文
相关论文

相关论文: An experimental test of the viscous anisotropy hyp…

200 篇论文

Physical experiments can characterize the elastic response of granular materials in terms of macroscopic state-variables, namely volume (packing) fraction and stress, while the microstructure is not accessible and thus neglected. Here, by…

软凝聚态物质 · 物理学 2015-06-16 Nishant Kumar , Stefan Luding , Vanessa Magnanimo

We report on the differences between colloidal systems left to evolve in the earth's gravitational field and the same systems for which a slow continuous rotation averaged out the effects of particle sedimentation on a distance scale small…

Viscoplastic deformation of shale is frequently observed in many subsurface applications. Many studies have suggested that this viscoplastic behavior is anisotropic---specifically, transversely isotropic---and closely linked to the layered…

地球物理 · 物理学 2022-11-24 Jinhyun Choo , Shabnam J. Semnani , Joshua A. White

Radiation creep and swelling are irreversible deformation phenomena occurring in materials irradiated even at low temperatures. On the microscopic scale, energetic particles initiate collision cascades, generating and eliminating defects…

材料科学 · 物理学 2024-09-23 Luca Reali , Max Boleininger , Daniel R. Mason , Sergei L. Dudarev

We study the crushing strength of brittle materials whose internal structure (e.g., mineral particles or graining) presents a layered arrangement reminiscent of sedimentary and metamorphic rocks. Taking a discrete-element approach, we probe…

软凝聚态物质 · 物理学 2021-03-09 David Cantor , Carlos Ovalle , Emilien Azéma

We present results of a simulation study of inelastic hard-disks vibrated in a vertical container. An Event-Driven Molecular Dynamics method is developed for studying the onset of convection. Varying the relevant parameters (inelasticity,…

统计力学 · 物理学 2016-08-31 Daniela Paolotti , Alain Barrat , Umberto Marini Bettolo Marconi , Andrea Puglisi

We ran several series of two-dimensional numerical mantle convection simulations representing in idealized form the thermochemical evolution of a Mars-like planet. In order to study the importance of compositional buoyancy of melting…

地球与行星天体物理 · 物理学 2017-08-15 Thomas Ruedas , Doris Breuer

We present the latest development of the disk gravitational instability and fragmentation model, originally introduced by us to explain episodic accretion bursts in the early stages of star formation. Using our numerical hydrodynamics model…

太阳与恒星天体物理 · 物理学 2015-06-03 Eduard I. Vorobyov , Shantanu Basu

In parallel with advances in microscale imaging techniques, the fields of biology and materials science have focused on precisely extracting particle properties based on their diffusion behavior. Although the majority of real-world…

介观与纳米尺度物理 · 物理学 2024-05-22 Kaito Takanami , Daisuke Taniguchi , Sawako Enoki , Masafumi Kuroda , Yasushi Okada , Yoshiyuki Kabashima

Much of a planet's composition could be determined right at the onset of formation. Laboratory experiments can constrain these early steps. This includes static tensile strength measurements or collisions carried out under Earth's gravity…

地球与行星天体物理 · 物理学 2018-08-31 Gerhard Wurm

Inertial waves in fluid regions of planets and stars play an important role in their dynamics and evolution, through energy, heat and angular momentum transport and mixing of chemicals. While inertial wave propagation in flows prescribed by…

地球物理 · 物理学 2026-05-20 Lennart Kira , Jerome Noir , Daniel Lecoanet

The Earth appears non-chondritic in its abundances of refractory lithophile elements, posing a significant problem for our understanding of its formation and evolution. It has been suggested that this non-chondritic composition may be…

地球与行星天体物理 · 物理学 2015-11-04 Philip J. Carter , Zoë M. Leinhardt , Tim Elliott , Michael J. Walter , Sarah T. Stewart

In this paper a model for partial melts is constructed using two-scale homogenization theory. While this technique is well known to the mathematics and materials communities, it is relatively novel to problems in the solid Earth. This…

地球物理 · 物理学 2015-05-13 Gideon Simpson , Marc Spiegelman , Michael I. Weinstein

ALMA observations of dust ring/gap structures in a minority but growing sample of protoplanetary disks can be explained by the presence of planets at large disk radii - yet the origins of these planets remains debated. We perform planet…

地球与行星天体物理 · 物理学 2022-02-08 Jessica Speedie , Ralph E. Pudritz , Alex J. Cridland , Farzana Meru , Richard A. Booth

The flow behaviors of polymer melt composed of short chains with ten beads between parallel plates are simulated by using a hybrid method of molecular dynamics and computational fluid dynamics. Three problems are solved: creep motion under…

软凝聚态物质 · 物理学 2014-01-20 Shugo Yasuda , Ryoichi Yamamoto

We investigate the down-hill creep of a layer of granular material on a slope caused by an oscillatory variation of the size of the particles. The material is modeled as an athermal two dimensional polydisperse system of soft disks under…

软凝聚态物质 · 物理学 2022-08-31 E. A. Jagla

We report new patterns, consisting of coexistence of sub-harmonic/harmonic and asynchronous states [for example, a granular gas co-existing with (i) bouncing bed, (ii) undulatory subharmonic waves and (iii) Leidenfrost-like state], in…

软凝聚态物质 · 物理学 2018-01-31 I. H. Ansari , N. Rivas , M. Alam

We investigate with numerical simulations the molecular origin of viscosity in melts of flexible and semiflexible oligomer rings in comparison to corresponding systems with linear chains. The strong increase of viscosity with ring stiffness…

软凝聚态物质 · 物理学 2023-07-28 Ranajay Datta , Fabian Berressem , Friederike Schmid , Arash Nikoubashman , Peter Virnau

Multiphase shear flows often show banded structures that affect the global behavior of complex fluids e.g. in microdevices. Here we investigate numerically the banding of emulsions, i.e. the formation of regions of high and low volume…

流体动力学 · 物理学 2020-04-30 Francesco De Vita , Marco Edoardo Rosti , Sergio Caserta , Luca Brandt

We perform numerical simulations of solid particle motion in a shearing box model of a protoplanetary disc. The accretion flow is turbulent due to the action of the magnetorotational instability. Aerodynamic drag on the particles is…

天体物理学 · 物理学 2009-11-13 Augusto Carballido , James M. Stone , Neal J. Turner