Abstract
Bethe lattice spins glasses are supposed to be marginally stable, i.e. their equilibrium probability distribution changes discontinuously when we add an external perturbation. So far the problem of a spin glass on a Bethe lattice has been studied only using an approximation where marginal stability is not present, which is wrong in the spin glass phase. Because of some technical difficulties, attempts at deriving a marginally stable solution have been confined to some perturbative regimes, high connectivity lattices or temperature close to the critical temperature. Using the cavity method, we propose a general non-perturbative approach to the Bethe lattice spin glass problem using approximations that should be hopefully consistent with marginal stability.
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Notes
I apologize for using here the replica jargon; this could be avoided in many cases because the replica language statements have been translated into the probabilistic language in most of the cases. Unfortunately, the stability analysis based on infinitesimal perturbations is not yet been translated into a probabilistic language and I cannot avoid using the replica language.
I use the notation h(i) and not \(h_i\) in order to stress that here i is not a node of the original graph. Cavity equations can also be written on a given graph, usually under the name of belief propagation equations. I will not discuss here this approach.
We are speaking of many equilibrium states for a finite system, while many equilibrium states should be present only in the infinite volume limit [28]. However the considerations we present have only a heuristic value.
As before K is a random Poisson variable with average z.
I am grateful to Dmitry Panchenko for clarifying this point to me.
In [43] the authors introduced a population of populations in order to formulate the problem in such a way that numerical computations are possible.
In the first line of Eq. (46) \(\rho _1(\theta _0,\theta _1)\) is a function, in the second line of the same equation \(\rho \) is a variable.
From the numerical viewpoint [62] it may also be convenient to do the computation at finite, but large r, provided that the computational weight does not increase too fast with r.
If the reader does not like white noises, he can reformulate everything in terms of Brownian motions \(B(x)=\int _0^x \eta (x)\): we could also use Ito stochastic calculus.
The function x(q) is the inverse of the function x(q). The functional F[x(q)] is concave: the concavity of this functional (proved in [66]) is surprising and counter-intuitive, at least to me.
The function \(\text{ Int }(y)\) denotes the integer part of the real number y.
The variable K is as usual a random Poisson number with average z.
In the SK model A(x, z) does not depends on z and \(C(z)=z\).
If we compute the annealed free energy \(F(x)\equiv \lim _{N\rightarrow \infty }-{\log \left( \overline{Z^N_J(\beta )^x}\right) /(\beta N x)}\) in presence of a magnetic field, we can derive similar formulae where the quantity \(h(x|x_0,h_0)_\eta \) has a more important physical role.
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Acknowledgements
It is a pleasure to thank Dmitry Panchenko for many discussions and clarifications. I would like also to thank Valerio Astuti, Silvio Franz, Carlo Lucibello, Federico Ricci-Tersenghi, and Pierfrancesco Urbani for a critical reading of the manuscript. This work has been supported by the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation program (Grant Agreement No. [694925]).
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I would like to dedicate this paper to the memory of my good friend Leo Kadanoff. I presented for the first time my spin glass theory at a Les Houches winter workshop in 1980 in an after dinner seminar. Leo was among the public, quite near to me in the front row, and I was comforted by his facial expressions of interest and approbation during the seminar; Leo congratulated with me after the seminar. His reactions were an important confirmation that I was on the right track: I was very grateful to him.
Appendix: The Cavity Equations in the Case of Broken Replica Symmetry
Appendix: The Cavity Equations in the Case of Broken Replica Symmetry
The cavity equations are often a direct way to find the maximum of the free energy.
At this end it is convenient to introduce the cavity equations for the probability over the descriptors i.e. \(\mathcal{P}_{}[\mathcal{D}]\). These equations can be derived heuristically by considering a N nodes system to which we add an extra node. A natural requirement is that the properties of the spin the extra node is the same of the others N spins. Alternatively, we could remove one spin from a \(N+1\) system forming a cavity, hence the name “cavity” method.
It has been proved [36] that a stochastically stable probability \(\mathcal{P}_{}[\mathcal{D}]\) that maximizes the free energy, should also satisfy of some equations that generalize the naive cavity equations (3). They are defined as follows. For each state \(\alpha \) we construct a new set of fields and weights using the fields \(vh_\alpha \) that are uncorrelated in i and correlated in \(\alpha \).
Z being a normalisation factor that enforces \(\sum w'_\alpha =1\). The quantities \(h'_\alpha \) and \(w'_\alpha \) are the fields and weights corresponding to new spin. These equations can be formally written as
According to the heuristic argument we finally impose that the probability distribution of the \(\{w'_\alpha ,h'_\alpha \}\) (i.e. \(\mathcal{P}'\) is again \(\mathcal{P}[\mathcal{D}]\). This constraint is called the cavity equations for \(\mathcal{P}_{}[\mathcal{D}]\) [40, 42, 43]: the cavity equations (\(\mathcal{P}'= \mathcal{C}[\mathcal{P}]\)) are valid in general for stochastically stable distributions, not only in the reproducible case.
The cavity equations can be considered the moral equivalent of
These equations are a necessary condition but not a sufficient condition. The cavity equations have many solutions; we need to find out the one that maximizes the free energy \(\mathcal{F}[\mathcal{P}_{}[\mathcal{D}]]\).
In the heuristic approach one often requires a further condition of stability. It can formally written as follows. Let us consider a solution (\(\mathcal{P}^*[\mathcal{D}]])\) of the cavity equation (74). For small \(\delta \mathcal{P}[\mathcal{D}]\) we can write a Taylor expansion
where the linear term in \(\delta \mathcal{P}[\mathcal{D}]\) is absent as effect of the cavity equation (74).
This equation defines a generalized Hessian (i.e. \(\mathbf{\large H}\)) that plays a crucial role in the heuristic approach.
Let us call \({\large H}_0\) the largest eigenvalues of \(\mathbf{H}\) (the so called replicon eigenvalue). It natural to assume that if \(\mathcal{P}^*[\mathcal{D}]\) maximize the free energy only if
or equivalently the matrix \(\mathbf{H}\) is non-positive, This condition generalizes the De Almeida–Thouless (DAT) stability condition. It is interesting to note that the DAT stability condition is usually equivalent to the condition:
where \(\langle \sigma _0 \sigma _l\rangle _c\) is the connected correlation function of two spins at distance l on the infinite Bethe Lattice [74].
It is also conjectured that this stability condition in saturated when the replica symmetry is spontaneously broken in a continuous way:
Indeed in all known cases, the saturation of DAT stability condition is the necessary condition for marginal stability.
It is conjectured that for spin glasses on the Bethe lattice when replica symmetry is spontaneously broken at r steps we have
This conjecture implies that the stability condition forces us to consider continuous RSB. This is the reason we are interested in finding approximations to spin glasses such that Eq. (78) is satisfied, maybe in some restricted space.
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Parisi, G. The Marginally Stable Bethe Lattice Spin Glass Revisited. J Stat Phys 167, 515–542 (2017). https://doi.org/10.1007/s10955-017-1724-z
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DOI: https://doi.org/10.1007/s10955-017-1724-z