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Failure of Ornstein–Zernike asymptotics for the pair correlation function at high temperature and small density

Yacine Aoun [email protected] Section de mathématiques, Université de Genève, Switzerland    Dmitry Ioffe Faculty of IE&M, Technion, Israel    Sébastien Ott [email protected] Section de mathématiques, Université de Genève, Switzerland    Yvan Velenik [email protected] Section de mathématiques, Université de Genève, Switzerland
Abstract

We report on recent results that show that the pair correlation function of systems with exponentially decaying interactions can fail to exhibit Ornstein–Zernike asymptotics at all sufficiently high temperatures and all sufficiently small densities. This turns out to be related to a lack of analyticity of the correlation length as a function of temperature and/or density and even occurs for one-dimensional systems.

In 1914, Ornstein and Zernike [1] introduced their celebrated equation for the density-density pair correlation function G(x,y)G(x,y):

G(x,y)=C(x,y)+ρC(x,z)G(z,y)dz,G(x,y)=C(x,y)+\rho\int C(x,z)G(z,y)\,\mathrm{d}z, (1)

where CC denotes the direct correlation function and ρ\rho the density. Using (1), Zernike [2] determined the asymptotic behavior of the pair correlation function of systems with short-range interactions (meaning here interactions decaying faster than some exponentially decreasing function of the distance):

G(0,x)Bdeνxx(d1)/2,G(0,x)\sim B_{d}\frac{e^{-\nu\left\|x\right\|}}{\left\|x\right\|^{(d-1)/2}}, (2)

as the Euclidean norm x\left\|x\right\| tends to infinity. His derivation relied on a certain mass gap assumption: |C(0,x)|emx|G(0,x)||C(0,x)|\leq e^{-m\left\|x\right\|}|G(0,x)|, which was believed to hold in wide generality for short-range models at low density [3].

It is usually expected that OZ behavior as displayed in (2) should hold for general simple fluids with short-range interactions at sufficiently high temperature and/or sufficiently small density. In this letter, we report on recent results that show that such is not necessarily the case. As will be explained below, this failure can be seen as resulting from a violation of the mass gap assumption.

For the sake of simplicity of exposition, we restrict our presentation to ferromagnetic Ising models on d\mathbb{Z}^{d}, but our results should hold in wide generality and have been established for other models in [4] (including the self-avoiding walk, Potts models, Bernoulli percolation, the massive Gaussian Free Field and the XY model). We start by discussing a simplified setting and then turn to a more general framework, in which some interesting new aspects emerge. A heuristic explanation of the underlying mechanism, relating the latter to a suitable condensation phenomenon, is also provided.

I Overview in a simplified setting

An anisotropic version of the OZ asymptotics (2) has been rigorously derived for finite-range ferromagnetic Ising models on d\mathbb{Z}^{d}, both above the critical temperature [5, 6] and when the magnetic field is non-zero [7]: in both cases, as x\left\|x\right\| tends to infinity,

σ0σxβ,hσ0β,hσxβ,h=Aβ,h(x^)xd12eνβ,h(x^)x(1+𝗈(1)),\langle\sigma_{0}\sigma_{x}\rangle_{\beta,h}-\langle\sigma_{0}\rangle_{\beta,h}\langle\sigma_{x}\rangle_{\beta,h}=\frac{A_{\beta,h}(\hat{x})}{\left\|x\right\|^{\frac{d-1}{2}}}e^{-\nu_{\beta,h}(\hat{x})\left\|x\right\|}(1+\mathsf{o}(1)), (3)

where both Aβ,hA_{\beta,h} and the inverse correlation length νβ,h\nu_{\beta,h} are positive, analytic functions of the direction x^=x/x\hat{x}=x/\left\|x\right\|. The same behavior still holds as long as the interaction decays super-exponentially [8]. Of course, this cannot be true for interactions decaying sub-exponentially, since the pair correlation function cannot decay slower than the interaction, as seems to have been first noted by Widom [9].

Let us thus restrict our attention to coupling constants Jx,y=JyxJ_{x,y}=J_{y-x} of the form

Jx=xαecx,J_{x}=\left\|x\right\|^{\alpha}e^{-c\left\|x\right\|}, (4)

for some α\alpha\in\mathbb{R} and c>0c>0. (More general forms will be considered below.) Let us also assume for simplicity that there is no magnetic field (and omit it from the notation). We emphasize, however, that the analysis below can also be done by fixing some arbitrary β\beta and looking at the behavior of hνβ,h(s)h\mapsto\nu_{\beta,h}(s).

Let ss be a unit vector in d\mathbb{R}^{d} and denote the inverse correlation length in direction ss by

νβ(s)=limn1nlnσ0σ[ns]β,\nu_{\beta}(s)=-\lim_{n\to\infty}\frac{1}{n}\ln\langle\sigma_{0}\sigma_{[ns]}\rangle_{\beta},

where [ns][ns] is a vertex of d\mathbb{Z}^{d} which is closest to nsdns\in\mathbb{R}^{d}. It is known [10] that νβ(s)>0\nu_{\beta}(s)>0 for all β<βc\beta<\beta_{\rm c}, where βc\beta_{\rm c} denotes the inverse critical temperature. In addition, it is easy to prove that νβ(s)\nu_{\beta}(s) is decreasing in β\beta and satisfies

limβ0νβ(s)=cs=c.\lim_{\beta\to 0}\nu_{\beta}(s)=c\left\|s\right\|=c. (5)

Moreover, limββcνβ(s)=0\lim_{\beta\uparrow\beta_{\rm c}}\nu_{\beta}(s)=0 [11]. The behavior in (5) is in sharp contrast with what happens when the interaction decays super-exponentially (in which case limβ0νβ(s)=\lim_{\beta\to 0}\nu_{\beta}(s)=\infty) and opens up the possibility that νβ(s)\nu_{\beta}(s) saturates at a finite temperature: νβ(s)=cs=c\nu_{\beta}(s)=c\left\|s\right\|=c for all β<βsat(s)\beta<\beta_{\rm sat}(s), for some βsat(s)(0,βc)\beta_{\rm sat}(s)\in(0,\beta_{\rm c}).

Observe that, if the latter were to occur, then there would be several remarkable consequences:

  • The inverse correlation length νβ(s)\nu_{\beta}(s) would not depend analytically on the temperature in the whole high-temperature regime (0,βc)(0,\beta_{\rm c}).

  • One of the basic assumptions of OZ theory, namely that the rate of decay of the pair correlation function is strictly slower than the rate of decay of the interaction (in the present case, νβ(s)<cs\nu_{\beta}(s)<c\left\|s\right\|) would be violated.

It turns out that such a saturation phenomenon can occur, in any dimension. Whether or not it does so depends on the value of the exponent α\alpha. Namely, saturation occurs (that is, βsat(s)>0\beta_{\rm sat}(s)>0) if and only if

α<(d+1)/2.\alpha<-(d+1)/2. (6)

In particular, even when d=1d=1, the inverse correlation length is a non-analytic function of β\beta whenever α<1\alpha<-1, which contrasts with the well-known analyticity of all thermodynamic quantities [12, 13].

As mentioned above, in the whole saturation regime β<βsat(s)\beta<\beta_{\rm sat}(s), one of the basic assumptions of the OZ theory fails to hold. In fact, one can show [8] that, while the OZ asymptotic behavior (3) still holds whenever β(βsat(s),βc)\beta\in(\beta_{\rm sat}(s),\beta_{\rm c}), it fails when β<βsat(s)\beta<\beta_{\rm sat}(s), where the pair correlation decays proportionally to the coupling constant.

II General setting

Let us now consider coupling constants of the form

Jx=ψ(x)e|x|,J_{x}=\psi(x)e^{-\lvert x\rvert}, (7)

where ||\lvert\cdot\rvert is an arbitrary norm on d\mathbb{R}^{d} and the prefactor ψ\psi is positive and sub-exponential, in the sense that lim|x|ln(ψ(x))/|x|=0\lim_{\lvert x\rvert\to\infty}\ln(\psi(x))/\lvert x\rvert=0. We also assume that it behaves in an approximately isotropic manner: there exists c1>0c_{1}>0 and a function ψ0:>0>0\psi_{0}:\mathbb{R}_{>0}\to\mathbb{R}_{>0} such that 1c1ψ0(x)ψ(x)c1ψ0(x)\frac{1}{c}_{1}\psi_{0}(\left\|x\right\|)\leq\psi(x)\leq c_{1}\psi_{0}(\left\|x\right\|) for all x0x\neq 0.

In order to ease the formulation of the extension of (6) to this more general framework, we need to make an additional genericity assumption on the direction ss. Let 𝒰\mathscr{U} be the unit-ball associated to the norm ||\lvert\cdot\rvert. Given a direction ss, consider the corresponding point s0=s/|s|𝒰s_{0}=s/\lvert s\rvert\in\partial\mathscr{U}. By convexity, every u𝒰u\in\partial\mathscr{U} close enough to s0s_{0} can be written as

u=s0+τvf(τv)t^,u=s_{0}+\tau v-f(\tau v)\hat{t}, (8)

where τ>0\tau>0 is some small real number, vv is unit vector in the tangent plane to 𝒰\partial\mathscr{U} at s0s_{0}, t^\hat{t} is a unit vector normal to the tangent plane and ff is some non-negative convex function defined on the tangent plane such that f(0)=0f(0)=0 (see Figure 1).

Refer to caption
Figure 1: Local parametrization of 𝒰\partial\mathscr{U}.

Our assumption on the direction ss is that the qualitative behavior of ff is the same in all directions vv: there exist c2>0c_{2}>0 and a non-decreasing convex function gg such that, for any unit vector vv in the tangent plane and τ\tau small enough, we have

1c2g(τ)f(τv)c2g(τ).\dfrac{1}{c_{2}}g(\tau)\leq f(\tau v)\leq c_{2}g(\tau). (9)

When this holds, we will say that 𝖴\partial\mathsf{U} is quasi-isotropic in direction ss. Examples when quasi-isotropy is satisfied in every direction ss include pp-norms with p[1,+]p\in[1,+\infty].

Our main result on whether βsat(s)>0\beta_{\rm sat}(s)>0 is the following:

Theorem 1

Fix a direction ss in which 𝖴\partial\mathsf{U} is quasi-isotropic. Then, saturation occurs in direction ss (that is, βsat(s)>0\beta_{\rm sat}(s)>0) if and only if

1ψ0()(g1(1/))d1<.\sum_{\ell\geq 1}\psi_{0}(\ell)(\ell g^{-1}(1/\ell))^{d-1}<\infty. (10)

(In (10), we make the convention g11g^{-1}\equiv 1 when g0g\equiv 0.)

When considering (4), we can take ψ0(x)=xα\psi_{0}(x)=\left\|x\right\|^{\alpha} and g(τ)=τ2g(\tau)=\tau^{2}; it is thus clear that (10) reduces to (6) in that case.

III An example

In this section, we illustrate on a specific example the direction-dependence of the saturation phenomenon.

Let us consider the model on 2\mathbb{Z}^{2} with interaction

Jx=xpαexp,J_{x}=\left\|x\right\|_{p}^{\alpha}e^{-\left\|x\right\|_{p}},

where p\left\|\cdot\right\|_{p} is the pp-norm and we assume that p(2,)p\in(2,\infty).

Let ss be a unit vector in 2\mathbb{R}^{2} and let us write s0=(x0,y0)=s/sps_{0}=(x_{0},y_{0})=s/\left\|s\right\|_{p}. When both x0x_{0} and y0y_{0} are nonzero, the local parametrization (8) of 𝒰\partial\mathscr{U} at s0s_{0} applies with

f(τv)=p12x0p2y0p2(x02p2+y02p2)3/2τ2+𝗈(τ2),f(\tau v)=\frac{p-1}{2}\frac{x_{0}^{p-2}y_{0}^{p-2}}{(x_{0}^{2p-2}+y_{0}^{2p-2})^{3/2}}\tau^{2}+\mathsf{o}(\tau^{2}),

so that one can choose g(τ)=τ2g(\tau)=\tau^{2}. Condition (10) then implies that there is saturation in direction ss if and only if α<3/2\alpha<-3/2, as in (6) (which should not be surprising, since 𝒰\partial\mathscr{U} has the same qualitative behavior in both cases).

In the remaining cases (s=±(1,0)s=\pm(1,0) or ±(0,1)\pm(0,1)), the local parametrization (8) of 𝒰\partial\mathscr{U} at s0s_{0} applies with

f(τv)=1pτp+𝗈(τp),f(\tau v)=\tfrac{1}{p}\tau^{p}+\mathsf{o}(\tau^{p}),

so that one can choose g(τ)=τpg(\tau)=\tau^{p}. Therefore, in this case, there is saturation in direction ss if and only if

α<1p2.\alpha<\frac{1}{p}-2.

This clearly shows that the occurrence of saturation depends on both the temperature and the direction. In particular, when 3/2>α1p2-3/2>\alpha\geq\frac{1}{p}-2, βsat(s)=0\beta_{\rm sat}(s)=0 when s{±(1,0),±(0,1)}s\in\{\pm(1,0),\pm(0,1)\} but is positive for all other directions.

IV An underlying condensation phenomenon

When β<βc\beta<\beta_{\rm c}, the 2-point function of the Ising model admits a graphical representation as a sum over paths:

σ0σxβ=γ: 0x𝗊β(γ),\langle\sigma_{0}\sigma_{x}\rangle_{\beta}=\sum_{\gamma:\,0\to x}\mathsf{q}_{\beta}(\gamma), (11)

where the sum is over edge-self-avoiding paths connecting 0 to xx and 𝗊β(γ)\mathsf{q}_{\beta}(\gamma) is a suitable non-negative weight [14]. Suppose that βsat(x^)>0\beta_{\rm sat}(\hat{x})>0. It turns out that the saturation phenomenon occurring at βsat(x^)\beta_{\rm sat}(\hat{x}) corresponds to a change of behavior of the typical paths contributing to the sum in (11). When β(βsat(x^),βc)\beta\in(\beta_{\rm sat}(\hat{x}),\beta_{\rm c}), typical paths γ\gamma have a length of order x\left\|x\right\| and behave diffusively, whereas when β(0,βsat(x^))\beta\in(0,\beta_{\rm sat}(\hat{x})), typical paths γ\gamma contain 𝖮(1)\mathsf{O}(1) steps: there is a giant step connecting a vertex close to 0 to a vertex close to xx, see Fig. 2. This change of behavior is reminiscent of condensation phenomena for sums of random variables; we refer to [15] for a review.

Refer to caption
Refer to caption
Figure 2: Sketches of a typical path γ\gamma in both regimes. Left: γ\gamma consists of one giant step for β<βsat(x^)\beta<\beta_{\rm sat}(\hat{x}). Right: γ\gamma consists of 𝖮(x)\mathsf{O}(\left\|x\right\|) small steps for β>βsat(x^)\beta>\beta_{\rm sat}(\hat{x}).

V Proof in dimension 1

In this section, we prove Theorem 1 when d=1d=1. The proof of the full Theorem 1 can be found in [4].

We consider the Ising model on \mathbb{Z} with interactions as in (7); for simplicity, we assume that ψ(y)=ψ(|y|)\psi(y)=\psi(|y|) for all yy and that ψ\psi is monotone in >0\mathbb{R}_{>0}. Introduce the generating functions (Laplace transforms)

𝕁(λ)=xJxeλx,𝔾(λ)=xσ0σxβeλx.\mathbb{J}(\lambda)=\sum_{x}J_{x}e^{\lambda x},\quad\mathbb{G}(\lambda)=\sum_{x}\langle\sigma_{0}\sigma_{x}\rangle_{\beta}e^{\lambda x}.

Note that 𝔾\mathbb{G} has radius of convergence νβ(1)\nu_{\beta}(1), while 𝕁\mathbb{J} has radius of convergence |1||1|. Moreover, since we are assuming that d=1d=1, condition (10) is equivalent to yψ(y)<\sum_{y\in\mathbb{Z}}\psi(y)<\infty and to 𝕁(|1|)<\mathbb{J}(|1|)<\infty.

Our analysis below will be based on the following inequalities satisfied by the weights in (11) (see [14]): there exists Cβ>0C_{\beta}>0 such that, if γ=(γ0,γ1,,γn)\gamma=(\gamma_{0},\gamma_{1},\dots,\gamma_{n}),

βni=1nJγiγi1𝗊β(γ)i=1nCβJγiγi1.\beta^{n}\prod_{i=1}^{n}J_{\gamma_{i}-\gamma_{i-1}}\geq\mathsf{q}_{\beta}(\gamma)\geq\prod_{i=1}^{n}C_{\beta}J_{\gamma_{i}-\gamma_{i-1}}. (12)

Note that the lower bound immediately implies that νβ(x^)|x^|\nu_{\beta}(\hat{x})\leq\lvert\hat{x}\rvert (simply consider the path γ\gamma composed of a single step from 0 to xx in (11)).

V.1 Proof that (10) implies βsat>0\beta_{\rm sat}>0

Using (11) and the upper bound (12), one straightforwardly obtains

𝔾(λ)β𝕁(λ)1β𝕁(λ),\mathbb{G}(\lambda)\leq\frac{\beta\mathbb{J}(\lambda)}{1-\beta\mathbb{J}(\lambda)},

whenever β𝕁(λ)<1\beta\mathbb{J}(\lambda)<1. So that if 𝕁(λ)<\mathbb{J}(\lambda)<\infty and β<𝕁(λ)1\beta<\mathbb{J}(\lambda)^{-1}, λ\lambda is in the convergence domain of 𝔾\mathbb{G}. As condition (10) implies that 𝕁(|1|)<\mathbb{J}(|1|)<\infty, it follows that νβ(1)|1|\nu_{\beta}(1)\geq|1| for β\beta small enough.

V.2 A comment on OZ equation at low density

Let us pause a moment to make a comment about the previous argument. Consider the OZ equation (1). Taking 𝔾\mathbb{G} and \mathbb{C} the Laplace transforms of xG(0,x)x\mapsto G(0,x) and xC(0,x)x\mapsto C(0,x), one obtains the relation 𝔾=1ρ\mathbb{G}=\frac{\mathbb{C}}{1-\rho\mathbb{C}}. For d=1d=1, C(0,x)0C(0,x)\geq 0 (ferromagnetic assumption), and supposing that the asymptotic decay of CC coincides with the one of JJ (which is for example the case in the Percus–Yevick approximation), the radii of convergence of 𝔾,\mathbb{G},\mathbb{C} are ν(1)\nu(1) and |1||1| respectively. Moreover, the same argument as previously implies that when (|1|)<\mathbb{C}(|1|)<\infty and ρ\rho is small enough, 𝔾(|1|)<\mathbb{G}(|1|)<\infty and therefore that |1|ν(1)|1|\leq\nu(1) (failure of mass gap). In higher dimensions, the same argument (with more involved considerations about the link between the convergence domains of 𝔾,\mathbb{G},\mathbb{C} and ν,||\nu,|\ |) is at the heart of the general condition (10).

V.3 Proof that yψ(y)=+\sum_{y}\psi(y)=+\infty implies βsat=0\beta_{\rm sat}=0

Since ψ\psi is non-summable, there exists RR such that

y=1Rψ(y)eCβ.\sum_{y=1}^{R}\psi(y)\geq\frac{e}{C_{\beta}}.

Let xx\in\mathbb{N} and N=x/RN=\left\|x\right\|/R. We have

σ0σxβ\displaystyle\langle\sigma_{0}\sigma_{x}\rangle_{\beta} y1=1RyN=1R(i=1NCβJyi)Jx(y1++yN)\displaystyle\geq\sum_{y_{1}=1}^{R}\cdots\sum_{y_{N}=1}^{R}\Bigl{(}\prod_{i=1}^{N}C_{\beta}J_{y_{i}}\Bigr{)}J_{x-(y_{1}+\dots+y_{N})}
e|x|y1=1RyN=1R(i=1nCβψ(yi))ψ(xiyi)\displaystyle\geq e^{-\lvert x\rvert}\sum_{y_{1}=1}^{R}\cdots\sum_{y_{N}=1}^{R}\Bigl{(}\prod_{i=1}^{n}C_{\beta}\psi(y_{i})\Bigr{)}\psi\bigl{(}x-\sum_{i}y_{i}\bigr{)}
=e|x|𝗈(x)(Cβy=1Rψ(yi))N\displaystyle=e^{-\lvert x\rvert-\mathsf{o}(\left\|x\right\|)}\Bigl{(}C_{\beta}\sum_{y=1}^{R}\psi(y_{i})\Bigr{)}^{\!N}
e|x|𝗈(x)eN=e|x|+xR𝗈(x),\displaystyle\geq e^{-\lvert x\rvert-\mathsf{o}(\left\|x\right\|)}e^{N}=e^{-\lvert x\rvert+\frac{\left\|x\right\|}{R}-\mathsf{o}(\left\|x\right\|)},

where we used |x|=|y1++yN|\lvert x\rvert=\lvert y_{1}+\dots+y_{N}\rvert in the second line; the fact that ψ\psi is sub-exponential in the third line; the choice of RR in the fourth line. This immediately implies that νβ(x^)|x^|1R\nu_{\beta}(\hat{x})\leq\lvert\hat{x}\rvert-\frac{1}{R}. Since β(0,βc)\beta\in(0,\beta_{\rm c}) was arbitrary, we conclude that βsat=0\beta_{\rm sat}=0.

VI Failure of Ornstein-Zernike asymptotics

In this section, we illustrate, in a simple example, the mechanism leading to a violation of OZ asymptotics when saturation occurs. Let us thus consider the Ising model on \mathbb{Z} with coupling constants of the form

Jy=|y|αe|y|.J_{y}=\lvert y\rvert^{\alpha}e^{-\lvert y\rvert}.

(Again, we refer to [4] for a treatment of the general case in any dimension.)

In the previous section, it was shown that saturation occurs when

y{0}|y|α<.\sum_{y\in\mathbb{Z}\setminus\{0\}}\lvert y\rvert^{\alpha}<\infty. (13)

We are going to show that there exists cβ>0c_{\beta}>0 such that

1cβ|x|αe|x|σ0σxβcβ|x|αe|x|.\dfrac{1}{c_{\beta}}\lvert x\rvert^{\alpha}e^{-\lvert x\rvert}\leq\langle\sigma_{0}\sigma_{x}\rangle_{\beta}\leq c_{\beta}\lvert x\rvert^{\alpha}e^{-\lvert x\rvert}. (14)

The lower bound follows directly from (11) by considering the path composed of a single step from 0 to xx. For the upper bound, note first that (12) implies

σ0σxβ\displaystyle\langle\sigma_{0}\sigma_{x}\rangle_{\beta} n=1y1,,yn{0}y1++yn=xβni=1n|yi|αe|yi|\displaystyle\leq\sum_{n=1}^{\infty}\sum_{\begin{subarray}{c}y_{1},\dots,y_{n}\in\mathbb{Z}\setminus\{0\}\\ y_{1}+\dots+y_{n}=x\end{subarray}}\beta^{n}\prod_{i=1}^{n}\lvert y_{i}\rvert^{\alpha}e^{-\lvert y_{i}\rvert}
e|x|n=1ny1,,yn{0}y1++yn=x|y1|maxi|yi|βni=1n|yi|α,\displaystyle\leq e^{-\lvert x\rvert}\sum_{n=1}^{\infty}n\sum_{\begin{subarray}{c}y_{1},\dots,y_{n}\in\mathbb{Z}\setminus\{0\}\\ y_{1}+\dots+y_{n}=x\\ \lvert y_{1}\rvert\geq\max_{i}\lvert y_{i}\rvert\end{subarray}}\beta^{n}\prod_{i=1}^{n}\lvert y_{i}\rvert^{\alpha}, (15)

where in the last line, we assumed that y1y_{1} is the vector with maximal ||\lvert\cdot\rvert-norm and used that |y1|++|yn||y1++yn|=|x|\lvert y_{1}\rvert+\dots+\lvert y_{n}\rvert\geq\lvert y_{1}+\dots+y_{n}\rvert=\lvert x\rvert. Observe now that, for any two real numbers a,ba,b with aba\geq b, we have

aαbα(a+b2)αbα=2α(a+b)αbα,a^{\alpha}b^{\alpha}\leq\biggl{(}\frac{a+b}{2}\biggr{)}^{\!\!\alpha}b^{\alpha}=2^{-\alpha}(a+b)^{\alpha}b^{\alpha},

since α\alpha is negative (by (13)). Using this observation n1n-1 times, it follows that

|y1|αi=2n|yi|α\displaystyle\lvert y_{1}\rvert^{\alpha}\prod_{i=2}^{n}\lvert y_{i}\rvert^{\alpha} (i=1n|yi|)αi=2n2α|yi|α\displaystyle\leq\Bigl{(}\sum_{i=1}^{n}\lvert y_{i}\rvert\Bigr{)}^{\!\alpha}\prod_{i=2}^{n}2^{-\alpha}\lvert y_{i}\rvert^{\alpha}
|x|αi=2n2α|yi|α,\displaystyle\leq\lvert x\rvert^{\alpha}\prod_{i=2}^{n}2^{-\alpha}\lvert y_{i}\rvert^{\alpha}, (16)

where we used |y1|maxi|yi|\lvert y_{1}\rvert\geq\max_{i}\lvert y_{i}\rvert for the first inequality and |y1|++|yn||x|\lvert y_{1}\rvert+\dots+\lvert y_{n}\rvert\geq\lvert x\rvert and α<0\alpha<0 for the second one.

Using (16) in (15) yields

σ0σxβ\displaystyle\langle\sigma_{0}\sigma_{x}\rangle_{\beta} |x|αe|x|n=1ny1,,yn{0}y1++yn=x|y1|maxi|yi|(2αβ)ni=2n|yi|α\displaystyle\leq\lvert x\rvert^{\alpha}e^{-\lvert x\rvert}\sum_{n=1}^{\infty}n\!\!\!\!\sum_{\begin{subarray}{c}y_{1},\dots,y_{n}\in\mathbb{Z}\setminus\{0\}\\ y_{1}+\dots+y_{n}=x\\ \lvert y_{1}\rvert\geq\max_{i}\lvert y_{i}\rvert\end{subarray}}\!\!\!\!(2^{-\alpha}\beta)^{n}\prod_{i=2}^{n}\lvert y_{i}\rvert^{\alpha}
|x|αe|x|2αβn=1n(2αβy{0}|y|α)n1.\displaystyle\leq\lvert x\rvert^{\alpha}e^{-\lvert x\rvert}2^{-\alpha}\beta\sum_{n=1}^{\infty}n\Bigl{(}2^{-\alpha}\beta\sum_{y\in\mathbb{Z}\setminus\{0\}}\lvert y\rvert^{\alpha}\Bigr{)}^{\!n-1}.

Thanks to Condition (13), we conclude that the sum over nn is convergent when β\beta is small enough, which yields the upper bound in (14).

VII Conclusion

We have considered an Ising model with exponentially decaying interactions and have explained how the latter can, in suitable circumstances, undergo a saturation “transition”, in which the rate of exponential decay of the pair correlation function coincides with the rate of exponential decay of the interaction over a non-empty interval of temperatures (0,βsat)(0,\beta_{\rm sat}) (where βsat(0,βc)\beta_{\rm sat}\in(0,\beta_{\rm c}) is in general direction-dependent). Since the inverse correlation length becomes independent of the temperature below βsat\beta_{\rm sat}, it is not an analytic function of β\beta on (0,βc)(0,\beta_{\rm c}). When this occurs, the pair correlation function fails to exhibit Ornstein–Zernike asymptotics for all β<βsat\beta<\beta_{\rm sat}.

A number of issues remain open. We have limited our analysis, for technical reasons, to ferromagnetic systems. It is unclear to us whether the general phenomenology changes when this assumption is dropped. In addition, the behavior of the system at βsat\beta_{\rm sat} is not understood, although it can be shown that in one-dimensional ferromagnetic systems, saturation does not occur at βsat\beta_{\rm sat} [8].

Acknowledgements.
YA thanks Hugo Duminil-Copin for financial support. YV was partially supported by the Swiss National Science Foundation through the NCCR SwissMAP.

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