LBan-IV

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Pinning and Depinning of a Disordered Material

In earlier lectures, we discussed how disordered systems can become trapped in deep energy states, forming a glass. Today, we will examine how such systems can also be pinned and resist external deformation. This behavior arises because disorder creates a complex energy landscape with numerous features, including minima (of varying depth), maxima, and saddle points.

When an external force is applied, it tilts this multidimensional energy landscape in a specific direction. However, local minima remain stable until a finite critical threshold is reached. Two important dynamical phase transitions are induced by pinning

  • The depinning transition: Interfaces pinned by impurities are ubiquitous and range from magnetic domain walls to crack fronts, from dislocations in crystals to vortices in superconductors. Above a critical force, interfaces depin, their motion becomes intermittent, and a Barkhausen noise is detected.
  • The yielding transition: Everyday amorphous materials such as mayonnaise, toothpaste, or foams exhibit behavior intermediate between solid and liquid. They deform under small stress (like a solid) and flow under large stress (like a liquid). In between, we observe intermittent plastic events.

Depinning tranition: the equation of motion

In the following we focus on the depinning trasition. At zero temperature and in the overdamped regime, where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \rho \partial_t^2 + \frac{1}{\mu} \partial_t \approx \frac{1}{\mu} \partial_t} , the equation of motion for the interface is:

Here we set , the external force and the disorder force is .

The No-Passing Rule

Interfaces obey the so-called no-passing rule. Consider two interfaces and such that for every . In the overdamped case, will never overtake .

To see why, assume for contradiction that at some time , reaches at a point , i.e., . At this point, it can be shown that the local velocity of , denoted by , is strictly less than the local velocity of , .

This contradiction implies that the no-passing rule holds: cannot overtake . An important consequence of the no-passing rule is that the value of the critical force is independent of the initial condition. Indeed, if at a given force the configuration is a dynamically stable state, it will act as an impenetrable boundary for all configurations preceding it.

When , the system possesses a single dynamically stable configuration. For , no metastable states exist, and the system transitions into a fully moving phase.

Cellular Automata

We now introduce a discrete version of the interface equation of motion. These cellular automata belong to the same universality class as the original model, and they are straightforward to implement numerically. For clarity, we first discuss the case of one spatial dimension, . We then extend its definition.

The 1D model

Step 1: Discretization along the x-direction

The interface is represented as a collection of blocks connected by springs with spring constant set to unity. The velocity of the -th block is given by:

Here, is the position of block at time , is the external driving force, and is the quenched random pinning force.

Step 2: Discretization along the h-direction

The key simplification is the narrow-well approximation for the disorder potential. In this approximation, impurities act as pinning centers, each trapping a block of the interface at discrete positions up to a local threshold force is overcomed. The distance between two consecutive pinning centers is a positive random variable , drawn from a distribution .

The total force acting on block is:

As is slowly increased, each block experiences a gradually increasing pulling force. An instability occurs when:


When this condition is met, block jumps to the next available well, and the forces are updated as:

After such an instability, one of the neighboring blocks may also become unstable, initiating a chain reaction.

Extensions of the 1D model

The system’s dimensionality is encoded in the elastic force acting on each block. In spatial dimension , the local force on block is written as a sum over its nearest neighbours:

where is the coordination number, i.e. the number of nearest neighbours of each block. The value of increases with the spatial dimension (e.g. for a square lattice in , in , and so on).

This form of the elastic force ensures that when a block becomes unstable and advances by an amount , its neighbours each receive an extra stress .

To describe the model in the limit of high dimension, it is convenient to replace the discrete Laplacian by a fully connected elasticity, corresponding to . In this case, the force becomes:

where is the center-of-mass height.

In the last part of the lecture we will solve the fully connected model explicitly. However, other elastic kernels are widely studied.


1. Long-range depinning kernels:

Here the sum extends over all sites, but the contribution decays with distance. The parameter controls the interaction range and typically lies between and . For these values, the critical exponents depend continuously on . For , one recovers the short-range results, while for one recovers the fully connected (mean-field) behavior. Many physical systems exhibit a long-range depinning transition; for instance, a 1D crack front corresponds to . Importantly, the transition remains a depinning transition, and in particular the no-passing rule continues to hold.

2. Kernels that violate the no-passing rule:

In some systems, such as the yielding transition of amorphous solids, the elastic interactions are described by Eshelby kernels. These interactions are long-ranged, anisotropic, and have a quadrupolar symmetry with zero spatial sum (the stress released in one region is redistributed so that the net force on the system remains unchanged). Such kernels break the no-passing rule and lead to qualitatively different critical behavior, which we will discuss in the conclusions of the next lecture.


Velocity-Force Caracteristics

It is convenient to introduce the distance to threshold:


An instability occurs when a block reaches . This is followed by its stabilization and by a uniform redistribution over all blocks: