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* (ii) '''Random Field''': If <math>V(x,h)</math> behaves like a Brownian motion along <math>h</math>, then <math>\Delta(h)</math> is short-range correlated.
* (ii) '''Random Field''': If <math>V(x,h)</math> behaves like a Brownian motion along <math>h</math>, then <math>\Delta(h)</math> is short-range correlated.


=== Velocity-Force Characteristics ===   
=== The No-Passing Rule ===   


We set to zero the temperature and consider the dynamics in the overdamped regime, where  <math>
Interfaces obey the so-called no-passing rule. Consider two interfaces <math>h_\alpha(x,t)</math> and <math>h_\beta(x,t)</math> such that <math>h_\alpha(x,t=0) < h_\beta(x,t=0)</math> for every <math>x</math>. In the overdamped case, <math>\alpha</math> will never overtake <math>\beta</math>
\rho \partial_t^2 +\eta \partial_t \approx \eta \partial_t </math>. In presence of an external force <math> f </math> the equation of motion of the interface is
<center><math>
\partial_t h(x,t)= \nabla^2  h +f +F(x,h(x,t)), \quad \text{with} \; F(x,h(x,t))= - \frac{\delta V(x,h(x,t))}{\delta h(x,t)}
</math></center>


The disorder force <math>F(x,h(x,t))</math> is a stochastic function:
To see why, assume for contradiction that at some time <math>t^*</math>, <math>\alpha</math> reaches <math>\beta</math> at a point <math>x^*</math>, i.e., <math>h_\alpha(x^*,t^*) = h_\beta(x^*,t^*)</math>. At this point, it can be shown that the local velocity of <math>\alpha</math>, denoted by <math>v_\alpha(x^*,t^*)</math>, is strictly less than the local velocity of <math>\beta</math>, <math>v_\beta(x^*,t^*)</math>.
<center><math>
\overline{F(x,h) F(x',h')} =\delta^d(x-x') \Delta(h-h')
</math></center>
There are usually two kind of disorder: (i) Random Bond (RB) if <math>V(x,h)</math> is short range correlated. Hence, the area below <math>\Delta(h)</math> is zero, (ii) Random field if <math>V(x,h)</math> is a Brownian motion along <math>h</math>.Hence, <math>\Delta(h)</math> is short range corraleted.


* The velocity - force characteristics
This contradiction implies that the no-passing rule holds: <math>\alpha</math> cannot overtake <math>\beta</math>.
 
* Existence of a unique critical force <math> f_c </math>: no-passing rule.
 
* Large force behaviour shows that in the moving phase the long distance properties of the interface are described by Edwards-Wilkinson.


== Scaling behaviour of the depinning transition ==  
== Scaling behaviour of the depinning transition ==  

Revision as of 17:33, 13 February 2025

Goal: This is the first lecture on the dynamics of disordered systems. We will explore how disorder in various systems induces pinning up to a critical threshold. Near this threshold, the dynamics become intermittent and are dominated by large reorganizations known as avalanches.

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  

ρt2+1μt1μt, the equation of motion for the interface is:

th(x,t)=2h+f+F(x,h(x,t)),withF(x,h(x,t))=δV(x,h(x,t))δh(x,t)

Here we setμ=1, f the external force and the disorder force is F(x,h(x,t)). Again we can consider a gaussian force of zero mean and correlations:

F(x,h)F(x,h)=δd(xx)Δ(hh)

There are usually two kinds of disorder:

  • (i) Random Bond (RB): If V(x,h) is short-range correlated, the area below Δ(h) is zero.
  • (ii) Random Field: If V(x,h) behaves like a Brownian motion along h, then Δ(h) is short-range correlated.

The No-Passing Rule

Interfaces obey the so-called no-passing rule. Consider two interfaces hα(x,t) and hβ(x,t) such that hα(x,t=0)<hβ(x,t=0) for every x. In the overdamped case, α will never overtake β.

To see why, assume for contradiction that at some time t*, α reaches β at a point x*, i.e., hα(x*,t*)=hβ(x*,t*). At this point, it can be shown that the local velocity of α, denoted by vα(x*,t*), is strictly less than the local velocity of β, vβ(x*,t*).

This contradiction implies that the no-passing rule holds: α cannot overtake β.

Scaling behaviour of the depinning transition

  • The order parameter of the transition is the velocity of the center of mass of the interface. It is vanishing as
vCM|ffc|β.
  • Two point correlation function:
v(y+x,t)v(y,t)ex/ξ(f)|x|κ,ξ(f)|ffc|ν
  • The interface is rough at fc
u(bx)bζu(x),u^bqbζduq


u^qu^q=δd(q+q)S(q),S(q)1|q|d+2ζ


  • The motion is intermittent with avalanches even below fc. Their size and duration is scale free up to a cut-off:
P(S)=Sτf(S/Smax),Smaxξ(f)d+ζ|ffc|(d+ζ)ν
P(T)=Tαf(T/Tmax),Tmaxξ(f)z|ffc|(z)ν


|===scaling arguemnts=== |{| class="wikitable" |+ Depinning exponents |- ! Exponent  !! Observable !! Mean field !! d=1 |- | z || (t)tz || 2 || 1.43±0.01 |- | ζ || h(bx)bζh(x) ||0|| 1.25±0.01 |- | ν || ξ(f)|ffc|ν ||1/2 || ν=12ζ |- | β || vCM|ffc|β || 1 || β=ν(zζ) |- | τ || P(S)Sτ|| 3/2 || τ=22d+ζ |}

Cellular Automata

We introduce a discrete version of the continuous equation of motion of the interface. These cellular automata share the same universality class of the original model, are very convenient for numerical studies and can be solved in the mean field limit. For simplicity we discuss the d=1 case.

The first step is the disretization along the x direction. The line is now a collection of L blocks connected by springs. The spring constant is set equal to one. Hence the velocity of each block is

vi(t)=thi(t)=12(hi+1(t)+hi1(t)2hi(t))+f+Fi(hi(t)),


To study avalanches below threshold, one as to trigger them at constant force, which is not very convenient. It is useful to replace the external force with a parabolic potential m22(whi(t))2, here m2 is the spring constant, try to bring each block at the equilibrium position w. The velocity of each block becomes

vi(t)=thi(t)=hi+1(t)+hi1(t)2hi(t)+m2(whi(t))+Fi(hi(t)),

Note that in a stable configuration, where all the velocity are zero, the force acting on the line per unit length is m2(whCM(t)). Increasing w the force slowly increases if hCM doest not move. When an avalanche occurs the force decreses.

Finally, the most important step is to introduce the narrow-well approximation for the disorder. We imagine that along hi impurities act as pinning center that trap the block around their position until a local threshold σith is reached. In this limit the local velocities are zero when the block is trapped and quickly move to the next impurity once the threshold is overcome. The obteained cellular automata can be described by the following algorithm:


  • Drive: Increasing w each point of the interface is pulled with a slowly increasing force or stress:
σi=12(hi+1+hi12hi)+m2(whi)

.

  • Instability: An instability occurs when σi reaches its σith. Hence the point moves to the next well
{σi=σiΔstress dropσi±1=σi±1+12Δ1+m2stress redistribution

Note that Δ is a positive random variable drwan from g(Δ).

  • Avalanche: The two neighbours can be unstable... An avalanche can start...