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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 .
  • Low-Temperature Phase:
Below a critical freezing temperature , 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, -independent probabilities.

Calculating the Freezing Temperature

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

Behavior in Different Phases:

  • High-Temperature Phase ():
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 ():
In this regime, the integral is finite:

This result implies that below the freezing temperature , 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 , and of length with periodic boundary conditions:

where is a Gaussian white noise with zero mean and variance:

The solution can be written in Fourier space as:

with Fourier decomposition:

where .

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

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 is drawn from the equilibrium distribution at temperature :

For simplicity, set the initial center of mass to zero: . We consider the mean square displacement of the point . The average is performed over both the thermal noise and the initial condition :

Questions:

  1. Compute the ensemble average of the Gaussian initial condition:
  • Hint:* Write the integral in terms of Fourier modes and use .
  1. Show that:
  1. Show that:

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

  1. Hence write:

Estimate for .

  1. Estimate for and large .
  • Hint:* Write the series as an integral using the continuum variable . It is helpful to know:

Provide the two asymptotic behaviors of .