T-2: Difference between revisions

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'''The model.''' In the spherical <math>p</math>-spin model the configurations <math> \vec{\sigma}=(\sigma_1, \cdots, \sigma_N) </math> that the system can take satisfy the spherical constraint <math> \sum_{i=1}^N \sigma_i^2=N </math>, and the energy associated to each configuration is  
=== The model: spherical <math>p</math>-spin ===
In the spherical <math>p</math>-spin model the configurations <math> \vec{\sigma}=(\sigma_1, \cdots, \sigma_N) </math> that the system can take satisfy the spherical constraint <math> \sum_{i=1}^N \sigma_i^2=N </math>, and the energy associated to each configuration is  


<center><math>
<center><math>
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'''Quenched vs annealed.'''  In TD1, we defined the quenched free energy density as the quantity controlling the scaling of the typical value of the partition function <math>Z </math>, which means:  
=== Quenched vs annealed ===
In TD1, we defined the quenched free energy density as the quantity controlling the scaling of the typical value of the partition function <math>Z </math>, which means:  
<center><math>
<center><math>
f= -\lim_{N \to \infty} \frac{1}{\beta N} \overline{ \log Z}.
f= -\lim_{N \to \infty} \frac{1}{\beta N} \overline{ \log Z}.

Revision as of 15:18, 9 December 2023

In this set of problems, we use the replica method to study the equilibrium properties of a prototypical toy model of glasses, the spherical p-spin model.


The model: spherical p-spin

In the spherical p-spin model the configurations σ→=(σ1,⋯,σN) that the system can take satisfy the spherical constraint ∑i=1Nσi2=N, and the energy associated to each configuration is

E(σ→)=∑1≤i1≤i2≤⋯ip≤NJi1i2⋯ipσi1σi2⋯σip,

where the coupling constants Ji1i2⋯ip are independent random variables with Gaussian distribution with zero mean and variance p!/(2Np−1), and p≥3 is an integer.


Quenched vs annealed

In TD1, we defined the quenched free energy density as the quantity controlling the scaling of the typical value of the partition function Z, which means:

f=−limN→∞1βNlog⁡Z‾.

The annealed free energy fann instead controls the scaling of the average value of Z. It is defined by

fann=−limN→∞1βNlog⁡Z‾.

These formulas differ by the order in which the logarithm and the average over disorder are taken. Computing the average of the logarithm is in general a hard problem, which one can address by using a smart representation of the logarithm, that goes under the name of replica trick:

log⁡x=limn→0xn−1n

which can be easily shown to be true by Taylor expanding xn=enlog⁡(x)=1+nlog⁡x+O(n2). Applying this to the average of the partition function, we see that

f=−limN→∞limn→01βNnZn‾−1n.

Therefore, to compute the quenched free-energy we need to compute the moments Zn‾ and then take the limit n→0. The annealed one only requires to do the calculation with n=1.


Problem 1: the annealed free energy

  1. Energy correlations. At variance with the REM, in the spherical p-spin the energies at different configurations are correlated. Show that E(σ→)E(τ→)‾=Nq(σ→,τ→)p/2+o(1), where q(σ→,τ→)=1N∑i=1Nσiτi is the overlap between the two configurations. Why an we say that for p→∞ this model converges with the REM discussed in the previous TD?
  1. Energy contribution. Show that computing Z‾ boils down to computing the average e−βJi1⋯ipσi1⋯σip‾. Compute this average. Hint: if X is a centered Gaussian variable with variance σ2, then eαX‾=eα2σ22.


  1. Entropy contribution. The volume of a sphere of radius N in dimension N is given by NN2πN2/(N2)!. Use the large-N asymptotic of this to conclude the calculation of the annealed free energy: the final result is only slightly different with respect to the free-energy of the REM in the high-temperature phase: can you identify the source of this difference?


Problem 2: the replica trick and the quenched free energy

  1. Step 1: average over the disorder. ccc


  1. Step 2: identify the order parameter. cccc


  1. Step 3: the saddle point. cccc