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Langevin Dynamics of Non-reciprocally Coupled Spherical Spin Glasses

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Abstract

We analyze the limiting dynamics of two copies of a disordered mean-field spherical pp-spin system coupled non-reciprocally to one another and initialized independently of the disorder. We prove that, on every finite time interval, as the system size tends to infinity, the empirical correlation and integrated response functions converge almost surely and in LqL^q for q≥1q \geq 1, uniformly in time, to the unique non-random solution of a system of coupled integro-differential equations. For even pp-spin models, we establish stationarity and exponential decay of the correlation and response functions in the high-temperature regime. In the special case of the spherical Sherrington–Kirkpatrick model, we derive explicit representations of the limiting correlation and integrated response functions. These representations allow us to characterize the long-time dynamics throughout the full range of temperatures. In particular, we prove the occurrence of aging in the low-temperature regime and fluctuation-dissipation behavior in the high-temperature regime, and provide a separate characterization of the dynamics at the critical temperature.

Introduction

Non-reciprocal interactions arise naturally in biological systems. For instance, in predator-prey systems, the interaction between species benefits one population and harms the other [1], and in neural networks the influence of one neuron on another need not be symmetric [19]. Such interactions also play a role in collective motion and synchronization, where they can generate sustained oscillations, traveling waves, and other time-dependent phases including chaos [14, 21].

A particular natural class of non-reciprocal systems consists of multiple interacting species, with symmetric interactions among members of each species and antisymmetric interactions between members of different species. This structure has been previously known in the context of excitatory-inhibitory neural networks, for example in [20], where such interactions were shown to give rise to dynamics ranging from stable fixed points to limit cycles. Models with such non-reciprocal interactions have recently been studied in the statistical physics literature as well, for example, [5] where two non-reciprocally coupled Ising models were studied. In another direction, Lorenzana et al [15] analyzed the Langevin dynamics of two identical copies of the spherical Sherrington–Kirkpatrick spin glass model with a non-reciprocal coupling. Their analysis showed evidence that depending on the network structure spin glass systems could retain glassy-dynamics phenomena such as aging, now accompanied by oscillations. Contrary to their findings, previous studies had predicted that any amount of non-reciprocity tends to destroy glassiness. In this paper, we rigorously analyze the dynamics introduced in [15] and extend its analysis to the mixed pp-spin model.

For x=(x1,…,xN)∈RNx=(x_1,\ldots,x_N)\in\mathbb{R}^N, let HNH_N denote the Hamiltonian of a spin glass with mixed pp-spin interactions, i.e.,

HN(x)=∑p=1mHN,p(x)=∑p=1mapp!∑1≤i1,…,ip≤NJi1…ipxi1⋯xip.H_N(x)=\sum_{p=1}^{m}H_{N,p}(x)=\sum_{p=1}^{m}\frac{a_p}{p!}\sum_{1\leq i_1,\ldots,i_p\leq N}J_{i_1\ldots i_p}x_{i_1}\cdots x_{i_p}.

where m≥2m \ge2, am≠0a_m \ne0, and the disorder parameters Ji1…ip=J{i1…ip}J_{i_1\ldots i_p}=J_{\{i_1\ldots i_p\}} are independent (modulo the permutation of indices) centered normal random variables with variance N−p+1∏klk!N^{-p+1}\prod_k l_k!, with (l1,l2,…)(l_1,l_2,\ldots) denoting the multiplicities of each element in the multiset {i1,…,ip}\{i_1,\ldots,i_p\}. Alternatively, if we set ξ(r)=∑p=1map2rp/p!\xi(r)=\sum_{p=1}^{m}a_p^2r^p/p!, HNH_N is the centered Gaussian process defined on RN\mathbb{R}^N with covariance given by

EHN(x)HN(y)=Nξ(x⋅yN),\mathbb{E}H_N(x)H_N(y)=N\xi\left(\frac{x\cdot y}{N}\right),

where ⋅\cdot denotes the standard inner product in RN\mathbb{R}^N.

In this paper we study the Langevin dynamics of two identical copies of HNH_N coupled with a non-reciprocal parameter. Precisely, let f:R→R+f:\mathbb{R}\to\mathbb{R}_+ be a differentiable function such that f′f' is locally Lipschitz and there exist constants κ<∞\kappa<\infty and ρ,δ>0\rho,\delta>0 such that

sup⁡t≥0∣f′(t)∣(1+t)κ<∞,andinf⁡t≥0(f′(t)−ρtm/2+δ−1)>−∞.(1)\sup_{t\ge0}\frac{|f'(t)|}{(1+t)^\kappa}<\infty,\qquad\text{and}\qquad\inf_{t\ge0}\left(f'(t)-\rho t^{m/2+\delta-1}\right)>-\infty. \tag*{(1)}

Let x(t)=(x1(t),x2(t))∈R2Nx(t)=(x^1(t),x^2(t))\in\mathbb{R}^{2N}, where xa(t)=(x1a(t),…,xNa(t))∈RNx^a(t)=(x^a_1(t),\ldots,x^a_N(t))\in\mathbb{R}^N is the spin configuration of the species a∈{1,2}a\in\{1,2\} at time tt. At an inverse temperature β>0\beta>0 and coupling strength α>0\alpha>0, we consider the Langevin dynamics given by

dx(t)=[G∘(x(t))−f′(∥x(t)∥22N)x(t)]dt+dB(t),(2)dx(t)=\left[G^\circ(x(t))-f'\left(\frac{\|x(t)\|^2}{2N}\right)x(t)\right]dt+dB(t), \tag*{(2)}

where

G∘(x(t)):=G(x(t))+α(Θ⊗IN)x(t),G^\circ(x(t)):=G(x(t))+\alpha(\Theta\otimes I_N)x(t),

with ⊗\otimes denoting the Kronecker product of matrices, INI_N the identity matrix of size NN,

G(x(t)):=(G1(x(t))G2(x(t))):=β(∇HN(x1(t))∇HN(x2(t))),Θ=(01−10),(3)G(x(t)):=\begin{pmatrix}G^1(x(t))\\G^2(x(t))\end{pmatrix}:=\beta\begin{pmatrix}\nabla H_N(x^1(t))\\\nabla H_N(x^2(t))\end{pmatrix},\qquad \Theta=\begin{pmatrix}0&1\\-1&0\end{pmatrix}, \tag*{(3)}

and B(t)B(t) a standard Brownian motion in R2N\mathbb{R}^{2N}. The term containing ff in (2) is a Lagrange multiplier that implements a ‘soft’ spherical constraint on the spin configuration x(t)x(t). We assume that the initial condition x(0)x(0), drawn according to a distribution μ2N\mu_{2N} on R2N\mathbb{R}^{2N}, the disorder J:={Ji1,…,ip:1≤p≤m, 1≤i1,…,ip≤N}J:=\{J_{i_1,\ldots,i_p}:1\le p\le m,\ 1\le i_1,\ldots,i_p\le N\} in HNH_N and the Brownian motion B(t)B(t) are all independent of each other.

Note that when α=0\alpha=0, the drift in (2) is of gradient form, with the two copies sharing a common confining potential and following the same stochastic gradient descent dynamics. For α>0\alpha>0, the additional forces +αx2+\alpha x^2 and −αx1-\alpha x^1 favor alignment of the first species with the second and anti-alignment of the second with the first, creating now an asymmetric imbalance.

Define the following quantities for a,b∈{1,2}a,b\in\{1,2\}:

CNab(s,t)=1Nxa(s)⋅xb(t),χNab(s,t)=1Nxa(s)⋅Bb(t),C_N^{ab}(s,t)=\frac{1}{N}x^a(s)\cdot x^b(t),\qquad \chi_N^{ab}(s,t)=\frac{1}{N}x^a(s)\cdot B^b(t),
ANab(s,t)=1NGa(x(s))⋅xb(t),FNab(s,t)=1NGa(x(s))⋅Bb(t).A_N^{ab}(s,t)=\frac{1}{N}G^a(x(s))\cdot x^b(t),\qquad F_N^{ab}(s,t)=\frac{1}{N}G^a(x(s))\cdot B^b(t).

Denoting by MabM^{ab} the (a,b)(a,b)th entry of the matrix MM, we can assemble the above quantities in four 2×22\times2 matrices CN(s,t)C_N(s,t), χN(s,t)\chi_N(s,t), AN(s,t)A_N(s,t) and FN(s,t)F_N(s,t), where

CN(s,t)=(CN11(s,t)CN12(s,t)CN21(s,t)CN22(s,t))C_N(s,t)=\begin{pmatrix}C_N^{11}(s,t)&C_N^{12}(s,t)\\C_N^{21}(s,t)&C_N^{22}(s,t)\end{pmatrix}

and the others are defined similarly. Finally, we denote KN(t)=CN(t,t)K_N(t)=C_N(t,t).

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