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=Exercise 1: Back to REM=
The Random Energy Model (REM) exhibits two distinct phases:
* '''High-Temperature Phase:''' 
: At high temperatures, the system is in a paramagnetic phase where the entropy is extensive, and the occupation probability of a configuration is approximately <math>\sim 1/M</math>. 
* '''Low-Temperature Phase:''' 
: Below a critical freezing temperature <math>T_f</math>, the system transitions into a glassy phase. In this phase, the entropy becomes subextensive (i.e., the extensive contribution vanishes), and only a few configurations are visited with finite, <math>M</math>-independent probabilities.
''' Calculating the Freezing Temperature <math>T_f</math>'''
Thanks to the computation of <math>\overline{n(x)}</math>, we can identify the fingerprints of the glassy phase and calculate <math>T_f</math>. 
Let's compare the weight of the ground state against the weight of all other states:
<center> 
<math>
\frac{\sum_\alpha z_\alpha}{z_{\alpha_{\min}}} = 1 + \sum_{\alpha \ne \alpha_{\min}} \frac{z_\alpha}{z_{\alpha_{\min}}} = 1 + \sum_{\alpha \ne \alpha_{\min}} e^{-\beta(E_\alpha - E_\min)} \sim 1 + \int_0^\infty dx\, \frac{d\overline{n(x)}}{dx} \, e^{-\beta x}= 1+ \int_0^\infty dx\, \frac{e^{x/b_M}}{b_M} \, e^{-\beta x}
</math>
</center>
=== Behavior in Different Phases:===
* '''High-Temperature Phase (<math> T > T_f= b_M = 1/\sqrt{2 \log2}</math>):''' 
: In this regime, the weight of the excited states diverges. This indicates that the ground state is not deep enough to render the system glassy.
* '''Low-Temperature Phase (<math> T < T_f= b_M = 1/\sqrt{2 \log2}</math>):''' 
: In this regime, the integral is finite: 
<center> 
<math>
\int_0^\infty dx \, e^{ (1/b_M-\beta) x}/b_M = \frac{1}{\beta b_M-1}  = \frac{T}{T_f - T}
</math> 
</center> 
This result implies that below the freezing temperature <math>T_f</math>, the weight of all excited states is of the same order as the weight of the ground state. Consequently, the ground state is occupied with a finite probability, reminiscent of Bose-Einstein condensation.
= Exercise 2: Edwards-Wilkinson Interface with Stationary Initial Condition  =
= Exercise 2: Edwards-Wilkinson Interface with Stationary Initial Condition  =



Revision as of 16:29, 31 August 2025

Exercise 1: Back to REM

The Random Energy Model (REM) exhibits two distinct phases:

  • High-Temperature Phase:
At high temperatures, the system is in a paramagnetic phase where the entropy is extensive, and the occupation probability of a configuration is approximately 1/M.
  • Low-Temperature Phase:
Below a critical freezing temperature Tf, the system transitions into a glassy phase. In this phase, the entropy becomes subextensive (i.e., the extensive contribution vanishes), and only a few configurations are visited with finite, M-independent probabilities.

Calculating the Freezing Temperature Tf

Thanks to the computation of n(x), we can identify the fingerprints of the glassy phase and calculate Tf. Let's compare the weight of the ground state against the weight of all other states:

αzαzαmin=1+ααminzαzαmin=1+ααmineβ(EαEmin)1+0dxdn(x)dxeβx=1+0dxex/bMbMeβx

Behavior in Different Phases:

  • High-Temperature Phase (T>Tf=bM=1/2log2):
In this regime, the weight of the excited states diverges. This indicates that the ground state is not deep enough to render the system glassy.
  • Low-Temperature Phase (T<Tf=bM=1/2log2):
In this regime, the integral is finite:

0dxe(1/bMβ)x/bM=1βbM1=TTfT

This result implies that below the freezing temperature Tf, the weight of all excited states is of the same order as the weight of the ground state. Consequently, the ground state is occupied with a finite probability, reminiscent of Bose-Einstein condensation.

Exercise 2: Edwards-Wilkinson Interface with Stationary Initial Condition

Consider an Edwards-Wilkinson interface in 1+1 dimensions, at temperature T, and of length L with periodic boundary conditions:

h(x,t)t=ν2h(x,t)+η(x,t)

where η(x,t) is a Gaussian white noise with zero mean and variance:

η(x,t)η(x,t)=2Tδ(xx)δ(tt)

The solution can be written in Fourier space as:

h^q(t)=h^q(0)eνq2t+0tdseνq2(ts)ηq(s)

with Fourier decomposition:

h^q(t)=1L0Leiqxh(x,t),h(x,t)=qeiqxh^q(t),ηq1(t)ηq2(t)=2TLδq1,q2δ(tt)

where q=2πn/L,n=,1,0,1,.

In class, we computed the width of the interface starting from a flat interface at t=0, i.e., h(x,0)=0. The mean square displacement of a point h(x,t) is similar but includes also the contribution of the zero mode. The result is:

Δhflat2=2TLt+{T2tπν,tL2,TνL12,tL2.

The first term describes the diffusion of the center of mass, while the second comes from the non-zero Fourier modes.

Now consider the case where the initial interface h(x,0) is drawn from the equilibrium distribution at temperature T:

Pstat.[h]exp[ν2T0Ldx(xh)2]

For simplicity, set the initial center of mass to zero: h^q=0(0)=0. We consider the mean square displacement of the point h(x=0,t). The average is performed over both the thermal noise and the initial condition :

Δh2=[h(0,t)h(0,0)]2=h2(0,t)+h2(0,0)2h(0,t)h(0,0)

Questions:

  1. Compute the ensemble average of the Gaussian initial condition:
h^q1(0)h^q2(0)
  • Hint:* Write the integral in terms of Fourier modes and use 0Ldxeiqx=Lδq,0.
  1. Show that:
h2(0,0)=TνLq01q2,h(0,t)h(0,0)=TνLq0eνq2tq2
  1. Show that:
h2(0,t)=A+Δhflat2

where the term A depends only on the initial condition. Show that:

A(t)=TνLq0e2νq2tq2
  1. Hence write:
C(t)Δh2Δhflat2=2TνLn=1(1eν(2πn/L)2t)2(2πn/L)2

Estimate C(t) for tL2.

  1. Estimate C(t) for tL2 and large L.
  • Hint:* Write the series as an integral using the continuum variable z=2πn/L. It is helpful to know:
0ds(1es2)2s2=π(22)

Provide the two asymptotic behaviors of Δh2.