Vertical dynamics of a horizontally-oscillating active object in a 2D granular medium

TL;DR

This study combines DEM simulations and analytical modeling to explore how a horizontally oscillating object behaves in a 2D granular medium, revealing conditions for rising, sinking, or stable equilibrium based on oscillation parameters.

Contribution

The paper introduces a cavity model that analytically predicts the vertical dynamics of an oscillating object in granular media, including critical thresholds for rising and sinking.

Findings

Identified a critical frequency $f_c$ for upward movement.

Derived a minimal amplitude $A_{min}$ for rising.

Established a critical acceleration $g_c$ for sinking.

Abstract

We use a DEM simulation and analytical considerations to study the dynamics of a self-energised object, modelled as a disc, oscillating horizontally within a two-dimesional bed of denser and smaller particles. We find that, for given material parameters, the immersed object (IO) may rise, sink or not change depth, depending on the oscillation amplitude and frequency, as well as on the initial depth. With time, the IO settles at a specific depth that depends on the oscillation parameters. We construct a phase diagram of this behaviour in the oscillation frequency and velocity amplitude variable space. We explain the observed rich behaviour by two competing effects: climbing on particles, which fill voids opening under the disc, and sinking due to bed fluidisation. We present a cavity model that allows us to derive analytically general results, which agree very well with the observations and explain quantitatively the phase diagram. Our specific analytical results are the following. (i) Derivation of a critical frequency, $f_c$, above which the IO cannot float up against gravity. We show that this frequency depends only on the gravitational acceleration and the IO size. (ii) Derivation of a minimal amplitude, $A_{min}$, below which the IO cannot rise even if the frequency is below $f_c$. We show that this amplitude also depends only on the gravitational acceleration and the IO size. (iii) Derivation of a critical value, $g_c$, of the IO's acceleration amplitude, below which the IO cannot sink. We show that the value of $g_c$ depends on the characteristics of both the IO and the granular bed,as well as on the initial IO's depth.