T-II-3: Difference between revisions
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where <math> Q_{ab}^{SP}</math> are the saddle point values of the overlap matrix. | where <math> Q_{ab}^{SP}</math> are the saddle point values of the overlap matrix introduced in Problem 2.2. The solution of the saddle point equations for the overlap matrix <math> Q</math> thus encodes a lot of information on the system; in particular, they contain the information on whether spin glass order emerges (meaning that <math>q^{(1)}>0 </math>). More generally, we can write: | ||
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\overline{P}(q)=\lim_{n \to 0} \frac{2}{n(n-1)}\sum_{a>b}\delta \left(q- Q_{ab}^{SP}\right) | q^{(1)}= \int dq \, \overline{P}(q) q \quad \quad | ||
\overline{P}(q)=\lim_{n \to 0} \frac{2}{n(n-1)}\sum_{a>b}\delta \left(q- Q_{ab}^{SP}\right), | |||
</math> | </math> | ||
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where <math> \overline{P}(q)</math> is a probability distribution | |||
probability that two copies of the system that are equilibrating in the same disordered environment at an inverse temperature beta end up having overlap q. Then | probability that two copies of the system that are equilibrating in the same disordered environment at an inverse temperature beta end up having overlap q. Then | ||
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Revision as of 15:40, 20 December 2023
Goal of these problems:
In this set of problems, we compute the free energy of the spherical -spin model in the Replica Symmetric (RS) framework, and in the 1-step Replica Symmetry Broken (1-RSB) framework.
Key concepts:
The order parameters: overlaps, and their meaning
In the lectures, we have introduced the spin-glass order parameter
This quantity can be computed within the replica formalism, and one finds
where are the saddle point values of the overlap matrix introduced in Problem 2.2. The solution of the saddle point equations for the overlap matrix thus encodes a lot of information on the system; in particular, they contain the information on whether spin glass order emerges (meaning that ). More generally, we can write:
where is a probability distribution probability that two copies of the system that are equilibrating in the same disordered environment at an inverse temperature beta end up having overlap q. Then
Indicator of ergodicity breaking: the Boltzmann measure is partitioned into pure states, and this is the distribution of overlaps between pure states. In Ising, only two pure states.
Problem 3.1: the RS (Replica Symmetric) calculation
Let us consider the simplest possible ansatz for the structure of the matrix Q, that is the Replica Symmetric (RS) ansatz:
Under this assumption, there is a unique saddle point variable, that is .
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Check that the inverse of the overlap matrix is
Compute the saddle point equation for in the limit , and show that this equation admits always the solution : why is this called the paramagnetic solution?
- Compute the free energy corresponding to the solution , and show that it reproduces the annealed free energy. Do you have an interpretation for this?
- Overlpa interpretation
Problem 3.2: the 1-RSB (Replica Symmetry Broken) calculation
In the previous problem, we have chosen a certain parametrization of the overlap matrix , which corresponds to assuming that typically all the copies of the systems fall into configurations that are at overlap with each others, no matter what is the pair of replicas considered. This assumption is however not the good one at low temperature. We now assume a different parametrisation, that corresponds to breaking the symmetry between replicas: in particular, we assume that typically the replicas fall into configurations that are organized in groups of size ; pairs of replicas in the same group are more strongly correlated and have overlap , while pairs of replicas belonging to different groups have a smaller overlap . This corresponds to the following block structure for the overlap matrix:
Here we have three parameters: (in the formula above, ).
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Using that
show that the free energy now becomes:
Under which limit this reduces to the replica symmetric expression?
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Compute the saddle point equations with respect to the parameter and are. Check that is again a valid solution of these equations, and that for the remaining equations reduce to:
How does one recover the paramagnetic solution?
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We now look for a solution different from the paramagnetic one. To begin with, we set to satisfy the first equation, and look for a solution of
Plot this function for and different values of , and show that there is a critical temperature where a solution appears: what is the value of this temperature (determined numerically)?