On the largest eigenvalue of a Hermitian random matrix model with spiked external source I. Rank one case

Jinho Baik, Dong Wang

Introduction and results

Fix an n×nn\times n Hermitian matrix An\mathbf{A}_{n} and consider the following density function on the set Hn\mathcal{H}_{n} of n×nn\times n Hermitian matrices:

where ZnZ_{n} is the normalization constant. Here the ‘external potential’ V(x)V(x) is a real-valued function which decays fast enough as ∣x∣→∞|x|\to\infty so that ZnZ_{n} is convergent. The matrix An\mathbf{A}_{n} is called the external source: see e.g. , , , , , , . Note that the distribution of eigenvalues of MM is unchanged if An\mathbf{A}_{n} is replaced by UAnU−1U\mathbf{A}_{n}U^{-1} for any unitary matrix UU. Since we are only concerned on eigenvalues of MM, we assume without loss of generality that An\mathbf{A}_{n} is a diagonal matrix.

A special case is when for all nn, the external source has a fixed number m\mathbf{m}, called the rank of An\mathbf{A}_{n}, of fixed non-zero eigenvalues. In this case, the sequence of probability spaces (Hn,pn)(\mathcal{H}_{n},p_{n}) is called a Hermitian matrix model with spiked external source, spiked source model for short. In this paper we only consider the case when m=1\mathbf{m}=1. The higher rank case when m>1\mathbf{m}>1 will be analyzed in the upcoming companion paper. Throughout this paper, we assume that n≥1n\geq 1 and

where aa is a real number, independent of nn.

There are two important special cases. When V(x)=x2/2V(x)=x^{2}/2, the spiked source model is called the GUE spiked model. The density pn(M)p_{n}(M) is that of M=H+AnM=H+\mathbf{A}_{n} where HH is an n×nn\times n GUE (Gaussian unitary ensemble) matrix. When V(x)=((1+c)x−clog⁡x)χ(0,∞)(x)V(x)=((1+c)x-c\log x)\chi_{(0,\infty)}(x), c=(m−n)/n≥0c=(m-n)/n\geq 0, the spiked source model is the complex Wishart spiked model. In this case, setting Σ:=(1−(1+c)−1An)−1\Sigma:=(1-(1+c)^{-1}\mathbf{A}_{n})^{-1}, the density pn(M)p_{n}(M) is that of M=Σ1/2XX†Σ1/2M=\Sigma^{1/2}XX^{\dagger}\Sigma^{1/2} where XX is an n×mn\times m complex rectangular matrix with i.i.d. standard complex Gaussian entries.For the complex Wishart spiked model, VV is not real analytic at x=0x=0. Throughout this paper, we only consider VV which is real analytic in the whole line. However, the method can be generalized to the Wishart-type potentials in a straightforward way. For these two cases, the limit of the largest eigenvalue ξmax⁡(n)\xi_{\max}(n) of MM was studied in great detail in and . An important feature is the following phase transition phenomenon. Let e\mathbf{e} denote the right-end point of the limiting empirical distribution of the eigenvalues of the Hermitian matrix model with no external source (see (10) below).The limiting empirical distribution in the spiked source model is the same as the Hermitian model with no external source. It was shown in both the GUE and the complex Wishart spiked models that as n→∞n\to\infty, with probability 11,

Here the function G(T)=12π∫−∞Te−12ξ2dξG(T)=\frac{1}{\sqrt{2\pi}}\int_{-\infty}^{T}e^{-\frac{1}{2}\xi^{2}}d\xi is the cumulative distribution function of the standard normal distribution, and F0F_{0} and F1\sqrt{F_{1}} are the GUE and GOE Tracy-Widom distribution functions, respectively. They are defined in (16) and (20) below, respectively. A limit theorem was also proven for the double scaling case when a=12V′(e)+αn1/3a=\frac{1}{2}V^{\prime}(\mathbf{e})+\frac{\alpha}{n^{1/3}}.

The purpose of this paper is to extend the results (3)–(5) to the spiked source model with general potential VV. It turns out that if V(x)V(x) is convex in the interval x∈(e,∞)x\in(\mathbf{e},\infty), then all of (3)–(5) still hold. Especially, the ‘critical value’ of aa is again given by 12V′(e)\frac{1}{2}V^{\prime}(\mathbf{e}). However, if VV is not convex in (e,∞)(\mathbf{e},\infty), new features may occur. Two key new features are the followings.

The critical value of aa may be smaller than 12V′(e)\frac{1}{2}V^{\prime}(\mathbf{e}). See Lemma 1.2 and Theorem 1.2. For such a case, when aa equals this critical value, ξmax⁡(n)\xi_{\max}(n) does not converge with probability 1. Instead it converges to two or more values, each with non-zero probability. In this case, the fluctuation of ξmax⁡(n)\xi_{\max}(n) is generically F0F_{0} at the smallest limiting value and GG at the larger limiting values. See Theorem 1.3.

There may be a discrete set of ‘secondary critical values’ of aa, which are greater than the critical value. If aa is at a secondary critical value, then ξmax⁡(n)\xi_{\max}(n) converge to two or more values, each with non-zero probability. In this case, the fluctuation of ξmax⁡(n)\xi_{\max}(n) is generically GG at each of the limiting values. See Theorem 1.4.

The exact assumptions on the potential VV is given in Subsection 1.2. The universality result for convex potentials is in Subsection 1.3. In Subsection 1.4 we define the critical and the secondary critical values for non-convex potentials. The limit laws for the non-convex potentials are given in Subsection 1.5.

While we were preparing for this paper and the companion paper for the higher rank case, we learned that M. Bertola, R. Buckingham, S. Y. Lee and V. Pierce were also working on the spiked source models (see for the first part of their work). While we focus, especially in the second paper, on the limit laws when a1,⋯ ,ama_{1},\cdots,a_{\mathbf{m}} are distinct, Bertola, Buckingham, Lee and Pierce focus on the case when a1=⋯=ama_{1}=\cdots=a_{\mathbf{m}} and m→∞\mathbf{m}\to\infty slower than nn. Also we use the asymptotics of usual orthogonal polynomials but Bertola, Buckingham, Lee and Pierce use asymptotics of multiple orthogonal polynomials via Riemann-Hilbert problem of size larger than 22.

Before closing this subsection, we mention that the spiked real symmetric matrix model is much more difficult. Even for the GOE and the real Wishart case, the limiting distribution at the critical value is not yet known. For the quaternionic case, the limiting distribution is obtained when the rank m=1\mathbf{m}=1 (see for the Wishart model; Gaussian model is also similar).

We also mention that there are several results for the spiked Wigner ensembles and spiked sample covariance matrices. See, for example, , , , , , and .

2 Assumptions on external potential V𝑉V.

Throughout this paper, we assume the following three conditions on VV:

The second condition is to ensure the convergence of the density function: compare this with the condition on VV in . The third condition on being ‘regular’ is a technical condition as defined in . We need a few definitions to state it.

First, recall the equilibrium measure and the so-called g\mathbf{g}-function. General references are and . For a given potential VV, the empirical distribution of the eigenvalues of the matrix model with no external source converges to the associated equilibrium measure μ\mu. The equilibrium measure is characterized by a certain variational problem. If VV is real analytic, μ\mu is supported on a finite union of intervals,

for some N≥0N\geq 0. We denote the right-most edge of the support by

On JJ, dμd\mu has the form dμ=Ψ(x)dxd\mu=\Psi(x)dx,

The so-called g\mathbf{g}-function is defined by

The potential VV is said to be regular (see ) if

The first condition implies that the function Ψ(x)>0\Psi(x)>0 for all x∈Jx\in J, and also that Ψ(x)\Psi(x) vanishes like a square-root at each end of the interval of the support. This in turn implies, in particular, that for the model with An=0\mathbf{A}_{n}=0, the largest eigenvalue has the limiting distribution given by F0F_{0} (see e.g. for the non-varying weight; varying weight case is similar using the analysis of .) Note that the second condition restricted to the domain x>ex>\mathbf{e} implies that

3 Statement of results: convex potentials

Let F0(T)F_{0}(T) be the GUE Tracy-Widom distribution defined by

where χ[T,∞)\chi_{[T,\infty)} denotes the projection operator on [T,∞)[T,\infty), and KAiry⁡K_{\operatorname{Airy}} is the Airy operator defined by the kernel

Here Ai⁡\operatorname{Ai} is the Airy function.

where the contour is from ∞e5πi/6\infty e^{5\pi i/6} to ∞eπi/6\infty e^{\pi i/6} and the pole z=−iαz=-i\alpha lies above the contour in the complex plane: see Figure 1.

where ⟨f,g⟩E\langle f,g\rangle_{E} denotes the real inner product over EE, ∫Ef(x)g(x)dx\int_{E}f(x)g(x)dx. (See [3, Definition 1.3].) When α=0\alpha=0,

equals the square of the GOE Tracy-Widom distribution (see [3, Formula (24)]).

Fix a potential VV satisfying the assumptions (6)–(8). In the companion paper on the higher rank case, we need to consider the spiked source model of rank 11 whose density function is same as in (1) but with the change that the matrix MM is now of size n−j+1n-j+1 and An\mathbf{A}_{n} is replaced by An−j+1\mathbf{A}_{n-j+1} for fixed jj:

Let e\mathbf{e} be as in (10). Set (recall (11))

for x∗>ex_{*}>\mathbf{e}, if V′′(x∗)−g′′(x∗)>0V^{\prime\prime}(x_{*})-\mathbf{g}^{\prime\prime}(x_{*})>0. Note that if V(x)V(x) is convex in x≥ex\geq\mathbf{e}, then V′′(x)−g′′(x)>0V^{\prime\prime}(x)-\mathbf{g}^{\prime\prime}(x)>0 for all x>ex>\mathbf{e}. For later reference we note that V′′(x∗)−g′′(x∗)=−G′′(x∗)V^{\prime\prime}(x_{*})-\mathbf{g}^{\prime\prime}(x_{*})=-\mathbf{G}^{\prime\prime}(x_{*}) in terms of the notation (32) that is defined below.

The following is the first main result of this paper. Let V(x)V(x) be a potential that is convex in x∈(e,∞)x\in(\mathbf{e},\infty). For a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}), let x0(a)x_{0}(a) be the unique maximizer of the function g(x)−V(x)+ax\mathbf{g}(x)-V(x)+ax in x∈(e,∞)x\in(\mathbf{e},\infty). Such a maximizer exists since g(x)−V(x)\mathbf{g}(x)-V(x) in x∈(e,∞)x\in(\mathbf{e},\infty) is strictly concave and g′(e)−V′(e)+a=−12V′(e)+a>0\mathbf{g}^{\prime}(\mathbf{e})-V^{\prime}(\mathbf{e})+a=-\frac{1}{2}V^{\prime}(\mathbf{e})+a>0 (see (30)) and g′(x)−V′(x)+a<0\mathbf{g}^{\prime}(x)-V^{\prime}(x)+a<0 for all large enough xx. This x0(a)x_{0}(a) is same as in Lemma 1.3.

Let V(x)V(x) be a potential that is convex in x∈(e,∞)x\in(\mathbf{e},\infty). Set

Hence the transition phenomenon is universal for convex potentials. The next two subsections are about non-convex potentials

4 Critical value and secondary critical values

In this Subsection, we define critical values and the secondary critical values of aa.

By definition (14), g(x)\mathbf{g}(x) is real analytic in (e,∞)(\mathbf{e},\infty), is continuously differentiable in [e,∞)[\mathbf{e},\infty) and satisfies

For a∈(0,12V′(e))a\in(0,\frac{1}{2}V^{\prime}(\mathbf{e})), define c=c(a)c=c(a) as the unique point in (e,∞)(\mathbf{e},\infty) satisfying

For a≥12V′(e)a\geq\frac{1}{2}V^{\prime}(\mathbf{e}), define c(a):=ec(a):=\mathbf{e}.

Note that c(a)c(a) decreases strictly in a∈(0,V′(e)/2)a\in(0,V^{\prime}(\mathbf{e})/2) and continuous in a∈(0,∞)a\in(0,\infty).

Let a>0a>0. We have the following properties.

H(x)\mathbf{H}(x) is a convex function in x∈[e,∞)x\in[\mathbf{e},\infty) with the unique minimum attained at x=c(a)x=c(a).

H(x)>G(x)\mathbf{H}(x)>\mathbf{G}(x) for all x∈(e,∞)x\in(\mathbf{e},\infty).

lim⁡x↓eH′(x)=lim⁡x↓eG′(x)=a−12V′(e)\displaystyle\lim_{x\downarrow\mathbf{e}}\mathbf{H}^{\prime}(x)=\lim_{x\downarrow\mathbf{e}}\mathbf{G}^{\prime}(x)=a-\frac{1}{2}V^{\prime}(\mathbf{e}).

As x→+∞x\to+\infty, H(x)→+∞\mathbf{H}(x)\to+\infty, H(x)/x→a\mathbf{H}(x)/x\to a, G(x)→−∞\mathbf{G}(x)\to-\infty and G(x)/x→−∞\mathbf{G}(x)/x\to-\infty.

See Figures 2, 3 and 4 for a few examples of the graphs of G\mathbf{G} and H\mathbf{H}.

The critical value for the spiked source model with potential VV is defined as

(12V′(e),∞)⊂AV(\frac{1}{2}V^{\prime}(\mathbf{e}),\infty)\subset\mathcal{A}_{V}. Hence ac≤12V′(e)\mathbf{a}_{c}\leq\frac{1}{2}V^{\prime}(\mathbf{e}).

The set AV\mathcal{A}_{V} is an open, semi-infinite interval. Hence AV=(ac,∞)\mathcal{A}_{V}=(\mathbf{a}_{c},\infty).

For 0<a<ac0<a<\mathbf{a}_{c}, we have G(x;a)<H(c(a);a)\mathbf{G}(x;a)<\mathbf{H}(c(a);a) for all x∈(c(a),∞)x\in(c(a),\infty).

If the potential V(x)V(x) is convex for x≥ex\geq\mathbf{e}, then ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}), and G(x;ac)<H(e;ac)\mathbf{G}(x;\mathbf{a}_{c})<\mathbf{H}(\mathbf{e};\mathbf{a}_{c}) for all x>ex>\mathbf{e}. (Note that c(ac)=ec(\mathbf{a}_{c})=\mathbf{e} and G(e;ac)=H(e,ac)\mathbf{G}(\mathbf{e};\mathbf{a}_{c})=\mathbf{H}(\mathbf{e},\mathbf{a}_{c}).)

If the potential VV is such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}), then G(x;ac)≤H(c(ac);ac)\mathbf{G}(x;\mathbf{a}_{c})\leq\mathbf{H}(c(\mathbf{a}_{c});\mathbf{a}_{c}) for all x∈(c(a),∞)x\in(c(a),\infty), and the equality is attained at least at one point.

Let a∈(12V′(e),∞)a\in(\frac{1}{2}V^{\prime}(\mathbf{e}),\infty). Since lim⁡x↓eG′(x)=a−12V′(e)>0\lim_{x\downarrow\mathbf{e}}\mathbf{G}^{\prime}(x)=a-\frac{1}{2}V^{\prime}(\mathbf{e})>0, there is xˉ>e\bar{x}>\mathbf{e} such that G(xˉ)>G(e)=H(e)\mathbf{G}(\bar{x})>\mathbf{G}(\mathbf{e})=\mathbf{H}(\mathbf{e}). Thus a∈AVa\in\mathcal{A}_{V}.

The continuity of G\mathbf{G} and H\mathbf{H} in aa implies that AV\mathcal{A}_{V} is an open set. Now we show that A\mathcal{A} is a semi-infinite interval. Suppose that a∈AVa\in\mathcal{A}_{V} and a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}). Let xˉ∈(c(a),∞)\bar{x}\in(c(a),\infty) be the point such that G(xˉ;a)>H(c(a);a)\mathbf{G}(\bar{x};a)>\mathbf{H}(c(a);a). Let a′∈(a,12V′(e)]a^{\prime}\in(a,\frac{1}{2}V^{\prime}(\mathbf{e})]. From Definition 1.1 of c(a)c(a), we see that c(a′)<c(a)c(a^{\prime})<c(a), and hence xˉ∈(c(a′),∞)\bar{x}\in(c(a^{\prime}),\infty). Moreover,

is strictly positive since each term in bracket is strictly positive. Thus a′∈AVa^{\prime}\in\mathcal{A}_{V}, and this, together with (a), implies that AV\mathcal{A}_{V} is a semi-infinite interval.

Let 0<a<ac0<a<\mathbf{a}_{c}. Suppose that there is xˉ∈(c(a),∞)\bar{x}\in(c(a),\infty) such that G(xˉ;a)=H(c(a);a)\mathbf{G}(\bar{x};a)=\mathbf{H}(c(a);a). For any a′∈(a,ac)a^{\prime}\in(a,\mathbf{a}_{c}), we have c(a)>c(a′)c(a)>c(a^{\prime}) since a<a′<12V′(e)a<a^{\prime}<\frac{1}{2}V^{\prime}(\mathbf{e}). Thus we find from (35) that G(xˉ;a′)−H(c(a′);a′)>0\mathbf{G}(\bar{x};a^{\prime})-\mathbf{H}(c(a^{\prime});a^{\prime})>0. This implies that a′∈AVa^{\prime}\in\mathcal{A}_{V} which is a contradiction.

Let 0<a<12V′(e)0<a<\frac{1}{2}V^{\prime}(\mathbf{e}). We will show that a∉Aa\notin\mathcal{A}. Since VV is convex, G(x)\mathbf{G}(x) is concave in x∈(e,∞)x\in(\mathbf{e},\infty). As G′(e;a)<0\mathbf{G}^{\prime}(\mathbf{e};a)<0, this implies that G(x)\mathbf{G}(x) is decreasing in x∈(e,∞)x\in(\mathbf{e},\infty). Thus for x∈(c(a),∞)x\in(c(a),\infty), G(x)<G(c(a))<H(c(a))\mathbf{G}(x)<\mathbf{G}(c(a))<\mathbf{H}(c(a)). Hence a∉AVa\notin\mathcal{A}_{V}. When a=12V′(e)a=\frac{1}{2}V^{\prime}(\mathbf{e}), a similar argument implies that G(x)<H(x)\mathbf{G}(x)<\mathbf{H}(x) for all x>ex>\mathbf{e}.

This follows from the continuity of G\mathbf{G} and H\mathbf{H} in aa and the fact that ac=inf⁡AV\mathbf{a}_{c}=\inf\mathcal{A}_{V}.

See typical graphs of G\mathbf{G} and H\mathbf{H} for ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) in Figure 2, and typical graphs of G\mathbf{G} and H\mathbf{H} for 0<ac<12V′(e)0<\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}) in Figure 3.

When VV is non-convex, there may exist xˉ>e\bar{x}>\mathbf{e} such that G(xˉ;ac)=H(e,ac)\mathbf{G}(\bar{x};\mathbf{a}_{c})=\mathbf{H}(\mathbf{e},\mathbf{a}_{c}) even if ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}).

By Definition 1.2 of ac\mathbf{a}_{c}, when a>aca>\mathbf{a}_{c}, G(x;a)>H(c(a);a)\mathbf{G}(x;a)>\mathbf{H}(c(a);a) for some x>c(a)x>c(a). The point xx at which G(x;a)\mathbf{G}(x;a) attains its maximum plays an important role. Indeed, we will show in the below that if the maximum is attained at a unique point, then ξmax⁡(n)\xi_{\max}(n) converges to this point (see Theorem 1.2). However, it may happen that for some aa’s, the function G(x;a)\mathbf{G}(x;a) attain its maximum at more than one point. Let

This set is discrete since G(x;a)\mathbf{G}(x;a) is analytic in both xx and aa. Note that when VV is convex, ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V} from Lemma 1.2(e). For a non-convex VV, as indicated in Remark 1.1, ac\mathbf{a}_{c} may or may not be in JV\mathcal{J}_{V} no matter if ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}). See typical graphs of G\mathbf{G} and H\mathbf{H} for a∈JVa\in\mathcal{J}_{V} in Figure 4.

For a∈[ac,∞)a\in[\mathbf{a}_{c},\infty) such that a∉JVa\not\in\mathcal{J}_{V}, let x0(a)x_{0}(a) be the unique point in [c(a),∞)[c(a),\infty) at which G(x;a)\mathbf{G}(x;a) attains its maximum. Then x0(a)x_{0}(a) is a continuous, strictly increasing function in a∈[ac,∞)∖JVa\in[\mathbf{a}_{c},\infty)\setminus\mathcal{J}_{V}.

If a0∈JVa_{0}\in\mathcal{J}_{V} and a0>aca_{0}>\mathbf{a}_{c}, then

Note that if a∈JVa\in\mathcal{J}_{V} satisfies a>aca>\mathbf{a}_{c} or a=ac<12V′(e)a=\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}), then there exist points x1(a)<x2(a)<⋯<xr(a)x_{1}(a)<x_{2}(a)<\dots<x_{r}(a) in (c(a),∞)(c(a),\infty), for some r≥2r\geq 2, such that

On the other hand, if VV is a potential such that ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∈JV\mathbf{a}_{c}\in\mathcal{J}_{V}, then there exist, for some r≥1r\geq 1, x1(ac)<x2(ac)<⋯<xr(ac)x_{1}(\mathbf{a}_{c})<x_{2}(\mathbf{a}_{c})<\dots<x_{r}(\mathbf{a}_{c}) in (e,∞)(\mathbf{e},\infty) such that

The continuity of x0(a)x_{0}(a) for a∉JVa\not\in\mathcal{J}_{V} is a direct consequence of the continuity of G(x;a)\mathbf{G}(x;a) in both xx and aa. Let ac≤a1<a2\mathbf{a}_{c}\leq a_{1}<a_{2} and a1,a2∉JVa_{1},a_{2}\not\in\mathcal{J}_{V}. If we assume x0(a1)≥x0(a2)x_{0}(a_{1})\geq x_{0}(a_{2}), then since G(x0(a1);a1)>G(x0(a2);a1)\mathbf{G}(x_{0}(a_{1});a_{1})>\mathbf{G}(x_{0}(a_{2});a_{1}), we have

This is contradictory to the assumption that x0(a2)x_{0}(a_{2}) is the maximizer of G(x;a2)\mathbf{G}(x;a_{2}). Thus x0(a1)<x0(a2)x_{0}(a_{1})<x_{0}(a_{2}).

If a0∈JVa_{0}\in\mathcal{J}_{V} and a0>aca_{0}>\mathbf{a}_{c}, then G(x;a0)\mathbf{G}(x;a_{0}) attains its maximum in [c(a0),∞)[c(a_{0}),\infty) at x1(a0),…,xr(a0)x_{1}(a_{0}),\dots,x_{r}(a_{0}) for some r≥2r\geq 2 as in (39). It is easy to check from the continuity of G(x;a)\mathbf{G}(x;a) in aa that lim⁡a↑a0x0(a)=x1(a0)\lim_{a\uparrow a_{0}}x_{0}(a)=x_{1}(a_{0}) and lim⁡a↓a0x0(a)=xr(a0)\lim_{a\downarrow a_{0}}x_{0}(a)=x_{r}(a_{0}). ∎

The secondary critical values for the spiked model are defined as the points a∈JVa\in\mathcal{J}_{V} such that a>aca>\mathbf{a}_{c}.

For a potential VV such that V(x)V(x) is convex for x≥ex\geq\mathbf{e}, JV=∅\mathcal{J}_{V}=\emptyset since G′(x;a)\mathbf{G}^{\prime}(x;a) is a decreasing function in x≥ex\geq\mathbf{e}. Hence there is no secondary critical value.

5 Statement of results: non-convex potentials

Let V(x)V(x) be a potential satisfying the conditions (6)–(8). Let InTI_{n}^{T} and JnT(x∗)J_{n}^{T}(x_{*}) be the intervals defined in (23) and (24), respectively.

For a>aca>\mathbf{a}_{c} such that a∉JVa\notin\mathcal{J}_{V}, if G′′(x0(a))≠0\mathbf{G}^{\prime\prime}(x_{0}(a))\neq 0, then

When aa is at or near the critical value ac\mathbf{a}_{c}, we have the following result. The case when a=aca=\mathbf{a}_{c} is attained by setting α=0\alpha=0.

Suppose that VV is a potential such that ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V}. Then for

Let VV be a potential such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}). If ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V} and G′′(x0(ac);ac)≠0\mathbf{G}^{\prime\prime}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0, then for

where the constant pj,n(α)∈(0,1)p_{j,n}(\alpha)\in(0,1) is defined by (145). As a function of α\alpha, pj,n(α)p_{j,n}(\alpha) is decreasing and satisfies pj,n(α)→0p_{j,n}(\alpha)\to 0 as α→∞\alpha\to\infty and pj,n(α)→1p_{j,n}(\alpha)\to 1 as α→−∞\alpha\to-\infty for each fixed nn. Also for each fixed α\alpha, pj,n(α)p_{j,n}(\alpha) lies in a compact subset of (0,1)(0,1) for all large nn.

When the potential V(x)V(x) is convex for x≥ex\geq\mathbf{e}, then ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}), JV=∅\mathcal{J}_{V}=\emptyset (see Remark 1.2) and G′′(x)<0\mathbf{G}^{\prime\prime}(x)<0 for all x>ex>\mathbf{e}. Hence Theorem 1.2 and Theorem 1.3(a) imply Theorem 1.1.

For aa at or near the secondary critical values JV∖{ac}\mathcal{J}_{V}\setminus\{\mathbf{a}_{c}\}, we have the following result.

Let VV be a potential such that JV≠∅\mathcal{J}_{V}\neq\emptyset. Let a0∈JV∖{ac}a_{0}\in\mathcal{J}_{V}\setminus\{\mathbf{a}_{c}\} be a secondary critical point. If G(x;a0)\mathbf{G}(x;a_{0}) attains its maximum Gmax⁡(a0)\mathbf{G}_{\max}(a_{0}) at two points x1(a0)<x2(a0)x_{1}(a_{0})<x_{2}(a_{0}) in (c(a),∞)(c(a),\infty) and if G′′(x1(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{1}(a_{0});a_{0})\neq 0 and G′′(x2(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{2}(a_{0});a_{0})\neq 0, then for

where pj,n(1)(α)p^{(1)}_{j,n}(\alpha) and pj,n(2)(α)∈(0,1)p^{(2)}_{j,n}(\alpha)\in(0,1) are defined in (164) and (158), and pj,n(1)(α)+pj,n(2)(α)=1p^{(1)}_{j,n}(\alpha)+p^{(2)}_{j,n}(\alpha)=1. As a function of α\alpha, pj,n(1)(α)p^{(1)}_{j,n}(\alpha) is decreasing and satisfies pj,n(1)(α)→0p^{(1)}_{j,n}(\alpha)\to 0 as α→∞\alpha\to\infty and pj,n(1)(α)→1p^{(1)}_{j,n}(\alpha)\to 1 as α→−∞\alpha\to-\infty for each fixed nn. Also for each fixed α\alpha, pj,n(1)(α)p^{(1)}_{j,n}(\alpha) is in a compact subset of (0,1)(0,1) independent of nn.

The above three theorems describe the ‘generic’ cases. The next part describes the three ‘exceptional cases’.

As the first exceptional case, suppose that in Theorem 1.4, the maximum of G\mathbf{G} is attained at more than two points. Let x1(a)<x2(a)<⋯<xr(a)x_{1}(a)<x_{2}(a)<\cdots<x_{r}(a) be these maximizers. If G′′(xj(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{j}(a_{0});a_{0})\neq 0 for all k=1,⋯ ,rk=1,\cdots,r, then we have, for each k=1,⋯ ,rk=1,\cdots,r,

for some pj,n(i)(α)∈(0,1)p_{j,n}^{(i)}(\alpha)\in(0,1) such that pj,n(1)(α)+⋯+pj,n(r)(α)=1p^{(1)}_{j,n}(\alpha)+\cdots+p^{(r)}_{j,n}(\alpha)=1. Explicitly, pj,n(i)(α):=Ai(α)A1(α)+⋯+Ar(α)p^{(i)}_{j,n}(\alpha):=\frac{A_{i}(\alpha)}{A_{1}(\alpha)+\cdots+A_{r}(\alpha)} where Ai(α)A_{i}(\alpha) is defined in (158). The situation when ac∈JV\mathbf{a}_{c}\in\mathcal{J}_{V} in Theorem 1.3(b) is similar. In this case, the maximum of G(x;ac)\mathbf{G}(x;\mathbf{a}_{c}) in (c(ac),∞)(c(\mathbf{a}_{c}),\infty) is attained at x1(ac)<x2(ac)<⋯<xr(ac)x_{1}(\mathbf{a}_{c})<x_{2}(\mathbf{a}_{c})<\cdots<x_{r}(\mathbf{a}_{c}) for some r≥2r\geq 2 (see (39)). Assume that G′′(xi(ac);ac)≠0\mathbf{G}^{\prime\prime}(x_{i}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0 for all i=1,⋯ ,ri=1,\cdots,r. Then with Ci(α)C_{i}(\alpha), i=1,⋯ ,ri=1,\cdots,r, defined by (144) with x0(ac)x_{0}(\mathbf{a}_{c}) replaced by xi(ac)x_{i}(\mathbf{a}_{c}), set pj,n(i)(α):=Ci(α)C0+C1(α)+⋯+Cr(α)p_{j,n}^{(i)}(\alpha):=\frac{C_{i}(\alpha)}{C_{0}+C_{1}(\alpha)+\cdots+C_{r}(\alpha)}, i=1,⋯ ,ri=1,\cdots,r, where C0C_{0} is defined by (143). Then (47) holds with pj,n(α)p_{j,n}(\alpha) replaced by pj,n(0)(α):=1−pj,n(1)(α)−⋯−pj,n(r)(α)p^{(0)}_{j,n}(\alpha):=1-p^{(1)}_{j,n}(\alpha)-\dots-p^{(r)}_{j,n}(\alpha). The limit in (48) is replaced by

The second exceptional case is when ac∈JV\mathbf{a}_{c}\in\mathcal{J}_{V} in Theorem 1.3, case 1. This case is given in the following Theorem. In this case, there are two natural scalings in aa.

Let VV be a potential such that ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}). Suppose that ac∈JV\mathbf{a}_{c}\in\mathcal{J}_{V}. Assume that G(x;ac)\mathbf{G}(x;\mathbf{a}_{c}) attains its maximum at the unique point x0(ac)∈(c(ac),∞)x_{0}(\mathbf{a}_{c})\in(c(\mathbf{a}_{c}),\infty) and G′′(x0(ac);ac)≠0\mathbf{G}^{\prime\prime}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0. Then the following holds.

where α\alpha is in a compact subset of (−∞,0)(-\infty,0), we have

where pj,n(α′)p_{j,n}(\alpha^{\prime}) is defined in (280). As a function of α\alpha, pj,n(α′)p_{j,n}(\alpha^{\prime}) is decreasing and satisfies pj,n(α′)→0p_{j,n}(\alpha^{\prime})\to 0 as α′→∞\alpha^{\prime}\to\infty and pj,n(α′)→1p_{j,n}(\alpha^{\prime})\to 1 as α′→−∞\alpha^{\prime}\to-\infty for each fixed nn. Also for each fixed α\alpha, pj,n(α)p_{j,n}(\alpha) is in a compact subset of (0,1)(0,1) independent of nn.

If the maximum of G(x;ac)\mathbf{G}(x;\mathbf{a}_{c}) is attained at more than one point, then (58) should be changed in a natural way as in (53).

The third exceptional case is when the double derivative of G(x;a)\mathbf{G}(x;a) vanishes at its maximizers. Then the function G(x)G(x) is replaced by its higher analogue, and the scalings in the interval and aa are also changed accordingly. Concretely, in Theorem 1.2(b), if G′′(x0(a))=0\mathbf{G}^{\prime\prime}(x_{0}(a))=0, then since x0(a)x_{0}(a) is the maximum point, there exists k>1k>1 such that G(2k)(x0(a))<0\mathbf{G}^{(2k)}(x_{0}(a))<0 and G(j)(x0(a))=0\mathbf{G}^{(j)}(x_{0}(a))=0 for all j=1,2,⋯ ,2k−1j=1,2,\cdots,2k-1. Then (43) is changed to

where the interval J^nT(x∗;k)\hat{J}_{n}^{T}(x_{*};k) is defined by

In Theorem 1.3(b), Theorem 1.4 and Theorem 1.5, aa is scaled as a=a0+αna=a_{0}+\frac{\alpha}{n}. When G′′(xi(a0);a0)=0\mathbf{G}^{\prime\prime}(x_{i}(a_{0});a_{0})=0, (i=0i=0 in Theorems 1.3(b) and 1.5, and i=1,2i=1,2 in Theorem 1.4,) then this scaling also needs to be changed. For example, Theorem 1.4 is changed to the following theorem.

Let a0∈JV∖{ac}a_{0}\in\mathcal{J}_{V}\setminus\{\mathbf{a}_{c}\} be a secondary critical value. Assume that G(x;a0)\mathbf{G}(x;a_{0}) attains its maximum Gmax⁡(a0)\mathbf{G}_{\max}(a_{0}) at two points x1(a0)<x2(a0)x_{1}(a_{0})<x_{2}(a_{0}) in (c(a),∞)(c(a),\infty). Suppose that G′′(x1(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{1}(a_{0});a_{0})\neq 0, and for some k>1k>1, and suppose that G(2k)(x2(a0);a0)≠0\mathbf{G}^{(2k)}(x_{2}(a_{0});a_{0})\neq 0 and G(i)(x2(a0);a0)=0\mathbf{G}^{(i)}(x_{2}(a_{0});a_{0})=0 for all i=1,…,2k−1i=1,\dots,2k-1. Then for

where the interval J^nT(x;k)\hat{J}_{n}^{T}(x;k) is defined by (60), pj,n(1)(α)p^{(1)}_{j,n}(\alpha) and pj,n(2)(α)p^{(2)}_{j,n}(\alpha) are defined in (182), and pj,n(1)(α)+pj,n(2)(α)=1p^{(1)}_{j,n}(\alpha)+p^{(2)}_{j,n}(\alpha)=1. As a function of α\alpha, pj,n(1)(α)p^{(1)}_{j,n}(\alpha) is decreasing and satisfies pj,n(1)(α)→0p^{(1)}_{j,n}(\alpha)\to 0 as α→∞\alpha\to\infty and pj,n(1)(α)→1p^{(1)}_{j,n}(\alpha)\to 1 as α→−∞\alpha\to-\infty for each fixed nn. Also for each fixed α\alpha, pj,n(1)(α)p^{(1)}_{j,n}(\alpha) is in a compact subset of (0,1)(0,1) independent of nn.

The changes needed for Theorem 1.3(b), and Theorem 1.5 are analogous. Also it may happen that the two or more of the exceptional cases occur simultaneously. Then one needs simply combine the results together in a straightforward way, and we skip the details.

We also remark that one can obtain the convergence in probability 1 as in (3) from the above theorems together with the fact that all of the limiting distributions decay rapidly at the tails.

An explicit example of a potential such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}) can be constructed as follows. We use the potential defined in [18, Formula (4.14)] (we change the original notation ee into eˉ\bar{e} here):

From results in [18, Section 4], it is known that Veˉ,ϵV_{\bar{e},\epsilon} is a regular potential with the support of the equilibrium measure given by [−2+O(ϵ),2+O(ϵ)][-2+O(\epsilon),2+O(\epsilon)]. For all x>e=2+O(ϵ)x>\mathbf{e}=2+O(\epsilon), (15) holds. However, at x=eˉx=\bar{e},

for some E(ϵ)E(\epsilon) satisfying E(ϵ)=O(ϵ)E(\epsilon)=O(\epsilon) and E(ϵ)>0E(\epsilon)>0. Hence for any aa, G(eˉ;a)−H(eˉ;a)=O(ϵ)\mathbf{G}(\bar{e};a)-\mathbf{H}(\bar{e};a)=O(\epsilon). Now there exists a∈(0,12V′(e))a\in(0,\frac{1}{2}V^{\prime}(\mathbf{e})) such that c(a)∈(e,eˉ)c(a)\in(\mathbf{e},\bar{e}) since the minimizer c(a)c(a) of H(x;a)\mathbf{H}(x;a) is continuous in a∈(0,∞)a\in(0,\infty), decreases strictly in a∈(0,12V′(e))a\in(0,\frac{1}{2}V^{\prime}(\mathbf{e})), lim⁡a↓0c(a)=+∞\lim_{a\downarrow 0}c(a)=+\infty and c(12V′(e))=ec(\frac{1}{2}V^{\prime}(\mathbf{e}))=\mathbf{e} (see the sentence after Definition 1.1). Since H(c(a);a)<H(eˉ;a)\mathbf{H}(c(a);a)<\mathbf{H}(\bar{e};a), we have G(eˉ;a)>H(c(a);a)\mathbf{G}(\bar{e};a)>\mathbf{H}(c(a);a) if ϵ\epsilon is small enough. Then a∈AVa\in\mathcal{A}_{V} and ac<12Veˉ,ϵ′(e)\mathbf{a}_{c}<\frac{1}{2}V_{\bar{e},\epsilon}^{\prime}(\mathbf{e}) for each fixed eˉ>2\bar{e}>2 if ϵ>0\epsilon>0 is small enough.

The paper is organized as follows. The outline of the proof of theorems is given in Section 2. The results on the orthonormal polynomials and the kernel Kn−j,nK_{n-j,n} are summarized in Section 6. The proofs of the theorems are given in Sections 3, 4 and 5. We consider three cases, ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}), ac>12V′(e)\mathbf{a}_{c}>\frac{1}{2}V^{\prime}(\mathbf{e}) and ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) separately. Throughout this paper we only consider a>0a>0. The a<0a<0 case is discussed briefly in the end of Section 2.

We would like to thank Marco Bertola, Robbie Buckingham, Seung-Yeop Lee and Virgil Pierce for keeping us informed of the progress of their work. The work of Jinho Baik was supported in part by NSF grants DMS075709.

Outline of the proof

be the orthonormal polynomial of degree jj with respect to the weight e−nV(x)e^{-nV(x)}. Here take γj(n)>0\gamma_{j}(n)>0 to make pjp_{j} unique. Set

be the Christoffel-Darboux kernel. Define the constant

We study two kinds of intervals E=InTE=I_{n}^{T} and E=JnT(x∗)E=J_{n}^{T}(x_{*}), x∗>ex_{*}>\mathbf{e}.

Then it follows that, since the operator norm of (1−χInTKn−j,nχInT)−1(1-\chi_{I_{n}^{T}}K_{n-j,n}\chi_{I_{n}^{T}})^{-1} is uniformly bounded from Corollary 6.3 (c), and ψn−j→0\psi_{n-j}\to 0 in L2(InT)L^{2}(I_{n}^{T}) from (332), that

Then since (1−χ[T,∞)Kn−j,nχ[T,∞))−1→(1−χ[T,∞)KAiry⁡χ[T,∞))−1(1-\chi_{[T,\infty)}\mathcal{K}_{n-j,n}\chi_{[T,\infty)})^{-1}\to(1-\chi_{[T,\infty)}K_{\operatorname{Airy}}\chi_{[T,\infty)})^{-1} in operator norm from (343) and n−1/6ψn−j(e+β−1n−2/3ξ)−Bj,n(e)Ai⁡(ξ)→0n^{-1/6}\psi_{n-j}(\mathbf{e}+\beta^{-1}n^{-2/3}\xi)-\mathcal{B}_{j,n}(\mathbf{e})\operatorname{Ai}(\xi)\to 0 in L2([T,∞))L^{2}([T,\infty)) by Corollary 6.1(d), we find that if uj,n−un→0u_{j,n}-u_{n}\to 0 in L2([T,∞))L^{2}([T,\infty)), then

In Sections 3, 4 and 5 we only consider a>0a>0. When a<0a<0, the largest eigenvalue in the spiked source model defined by (21) has the same distribution as the negative value of the smallest eigenvalue of the spiked source model that is defined by the same formula but with the potential function V^(x)=V(−x)\hat{V}(x)=V(-x) and the external source matrix −An−j+1-\mathbf{A}_{n-j+1}. Since V^(x)\hat{V}(x) is regular as long as V(x)V(x) is, and the non-zero eigenvalue of −An−j+1−\mathbf{A}_{n-j+1} is positive, the analysis in this paper applies for that spiked source model. We need to keep track of the smallest eigenvalue in the new spiked source model, and it can be done in the same way that we analyze the largest one. It can be checked that the limiting distribution of the smallest eigenvalue is not affected by the positive external source eigenvalue aa, corresponding to the a<0a<0 case of Theorem 1.2(a). We skip any further remarks.

Note that (Cφn−j)(z)enaz→0(C\varphi_{n-j})(z)e^{naz}\to 0 exponentially as ℜ(z)→−∞\Re(z)\to-\infty since a>0a>0. Therefore, we can deform the contour and obtain

where, with a constant CΓ>12aC_{\Gamma}>\frac{1}{2a},

The contours are oriented as indicated in Figure 5. Therefore we find

Let δ\delta be given in Proposition 6.1. Let ϵ<min⁡{c(a)−e,2δ}\epsilon<\min\{c(a)-\mathbf{e},2\delta\} be a small enough positive constant, independent of nn, such that all maximizers of G(x;a)\mathbf{G}(x;a) in [c,∞)[c,\infty) are in the interval (e+ϵ,∞)(\mathbf{e}+\epsilon,\infty). Recall the asymptotics of (Cφn−j)(z)(C\varphi_{n-j})(z) summarized in Section 6. Since the contours Γ±\Gamma_{\pm} lie in BδB_{\delta} (in Figure 10) in Section 6, from the asymptotic formula (320) for (Cφn−j)(z)(C\varphi_{n-j})(z),

We now use the method of steepest-descent to evaluate the integral asymptotically. By Lemma 1.1, H′(c(a);a)=0\mathbf{H}^{\prime}(c(a);a)=0 and H′′(c(a);a)>0\mathbf{H}^{\prime\prime}(c(a);a)>0. It is straightforward to check, with the help of the formula of g(x)\mathbf{g}(x) in (14), that for z(t)=c+itz(t)=c+it, t>0t>0, the function ℜH(z(t);a)\Re\mathbf{H}(z(t);a) in tt satisfies

Also for z(t)=c+iCΓ−t∈Γ+z(t)=c+iC_{\Gamma}-t\in\Gamma_{+}, t≥0t\geq 0,

is negative for all t≥0t\geq 0 if CΓ>1/(2a)C_{\Gamma}>1/(2a). Hence ℜH(z;a)\Re\mathbf{H}(z;a) decreases as zz moves along Γ+\Gamma_{+} counterclockwise. Similarly ℜH(z;a)\Re\mathbf{H}(z;a) increases as zz moves along Γ−\Gamma_{-} counterclockwise. Therefore Γ+∪Γ−‾\overline{\Gamma_{+}\cup\Gamma_{-}} is a curve of steep-descent for H\mathbf{H} with the saddle point at z=cz=c. The fact that z=cz=c is a saddle point of H\mathbf{H} is the reason that we have split the integral in (80) at cc.

Now consider the second integral in (85). From the asymptotics (318) for φn−j\varphi_{n-j} in BδB_{\delta},

Using that Mj,nM_{j,n} is uniformly bounded in any compact subset of [e+ϵ,∞)[\mathbf{e}+\epsilon,\infty), and Mj,n(y)=O(y−j)M_{j,n}(y)=O(y^{-j}) as y→∞y\to\infty, and using that G(y;a)→−∞\mathbf{G}(y;a)\to-\infty at least linearly, we obtain the trivial estimate that

where Gmax⁡(a):=max⁡{G(y;a)∣y≥c(a)}\mathbf{G}_{\max}(a):=\max\{\mathbf{G}(y;a)\mid y\geq c(a)\}. Together with (89), we obtain the following result. Recall the properties of G\mathbf{G} and H\mathbf{H} in Subsection 1.4.

Suppose that a<aca<\mathbf{a}_{c}. Then H(c;a)>Gmax⁡(a)\mathbf{H}(c;a)>\mathbf{G}_{\max}(a). Therefore, (89) is exponentially larger than (91) and we obtain

Suppose that ac<a<12V′(e)\mathbf{a}_{c}<a<\frac{1}{2}V^{\prime}(\mathbf{e}) (assuming that VV is such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e})). Then Gmax⁡(a)>H(c;a)\mathbf{G}_{\max}(a)>\mathbf{H}(c;a) and hence (91) is exponentially larger than (89). Suppose that a∉JVa\notin\mathcal{J}_{V} and let x0=x0(a)∈(c(a),∞)x_{0}=x_{0}(a)\in(c(a),\infty) be the unique point Gmax⁡(a)\mathbf{G}_{\max}(a) is attained. If G′′(x0;a)≠0\mathbf{G}^{\prime\prime}(x_{0};a)\neq 0, using the Laplace’s method applied to (90) (using the properties of Mj,nM_{j,n} in Proposition 6.1 (a)), we obtain

If G′′(x0;a)=0\mathbf{G}^{\prime\prime}(x_{0};a)=0 and G(2k)(x0;a)≠0\mathbf{G}^{(2k)}(x_{0};a)\neq 0, G(j)(x0;a)=0\mathbf{G}^{(j)}(x_{0};a)=0 for j=1,⋯ ,2k−1j=1,\cdots,2k-1, then the Laplace’s method implies that

When a∈JVa\in\mathcal{J}_{V}, the contributions to (91) at each maximizer should be added. Examples of this case are in (155) and (174).

If a=aca=\mathbf{a}_{c} (note that since we assumed a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), this implies that VV is such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e})), then H(c;ac)=Gmax⁡(ac)\mathbf{H}(c;\mathbf{a}_{c})=\mathbf{G}_{\max}(\mathbf{a}_{c}). If we further assume that ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V} and G′′(x0(ac);ac)≠0\mathbf{G}^{\prime\prime}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0, (89) and (91) are of same order. Then by Laplace’s method applied to (91),

We can consider a double scaling case when

This can be written in the following way. Let cc be any constant such that c>ec>\mathbf{e}. We will take c=c(a)c=c(a) as in Definition 1.1 in the subsequent sections for asymptotic analysis, but the following result holds for any c>ec>\mathbf{e}.

By the same calculation that leads to (85), (100) equals

Using the partial fraction formula and the definition of the Cauchy transformation again, this equals

where the identity (326) is used in the last line. Hence the first sum on the right-hand-side of (103) satisfies

2.2 For x≥𝐞+ϵ𝑥𝐞italic-ϵx\geq\mathbf{e}+\epsilon:

𝐞italic-ϵx\geq\mathbf{e}+\epsilon: Take c=c(a)c=c(a) as in Definition 1.1 in the formula of Lemma 3.1. Fix ϵ>0\epsilon>0 small enough so that [c,∞)⊂[e+ϵ,∞)[c,\infty)\subset[\mathbf{e}+\epsilon,\infty).

From (336), the second integral over (c,∞)(c,\infty) in (108) is

On the other hand, for the integral over Γ+∪Γ−\Gamma_{+}\cup\Gamma_{-}, (318) and (320) imply that

Thus using the fact that cc is the saddle point of H(z)\mathbf{H}(z), we have that the first integral over Γ+∪Γ−\Gamma_{+}\cup\Gamma_{-} in (108) is

On the other hand, for Γn−j(a)\Gamma_{n-j}(a), we have from (85), (86), (89) and (90) that

Note that we also have a matching lower bound. Comparing the estimate (113) of Γn−j(a)\mathbf{\Gamma}_{n-j}(a) and two estimates (109) and (112), we find that Qj,n(x)=O((1+∣x∣)−j)Q_{j,n}(x)=O((1+\lvert x\rvert)^{-j}) uniformly for x≥e+ϵx\geq\mathbf{e}+\epsilon if ∣x−c∣≥ϵ′\lvert x-c\rvert\geq\epsilon^{\prime} for a positive constant ϵ′\epsilon^{\prime}. Note that in this case the error term in (106) does not contain n\sqrt{n}.

Now let xx satisfy ∣x−c∣<ϵ′\lvert x-c\rvert<\epsilon^{\prime}. In this case, we start with the formula (101) with a different choice of cc. We replace cc by c±n−1/2c\pm n^{-1/2} and let (Γ+)±∪(Γ−)±(\Gamma_{+})^{\pm}\cup(\Gamma_{-})^{\pm} be a contour deformed from Γ+∪Γ−\Gamma_{+}\cup\Gamma_{-} by a semicircle of radius n−1/2n^{-1/2} to the right/left, respectively, as illustrated in Figures 7 and 7. Here we take the ++ sign if x−c≥0x-c\geq 0 and take the −- sign if x−c<0x-c<0. Then

2.3 For x𝑥x near 𝐞𝐞\mathbf{e}:

Let TT be a fixed constant and let ϵ\epsilon be a small positive constant such that 0<ϵ<min⁡{c−e,δ0}0<\epsilon<\min\{c-\mathbf{e},\delta_{0}\} where δ0\delta_{0} is the constant in Proposition 6.1 and its corollaries in Section 6. Define the interval

For a given x∈ET,ϵx\in E_{T,\epsilon}, define ξ\xi by the relation

We have for all 0<a<V′(e)/20<a<V^{\prime}(\mathbf{e})/2,

uniformly in x∈ET,ϵx\in E_{T,\epsilon} and in nn.

We use the formula (101). From (339) and (330), the integral over (c,∞)(c,\infty) in (101) is

On the other hand, substituting (331) and (320) into (102), the integrand of the first integral over Γ+∪Γ−\Gamma_{+}\cup\Gamma_{-} in (101) is

for all x∈ET,ϵx\in E_{T,\epsilon} and z∈Γ±z\in\Gamma_{\pm} since ∣x−z∣>c−e−ϵ>0|x-z|>c-\mathbf{e}-\epsilon>0. Thus the the first integral over Γ+∪Γ−\Gamma_{+}\cup\Gamma_{-} in (101) is

Substituting (119) and (121) into (101) and noting that 1(c,∞)(x)=01_{(c,\infty)}(x)=0 for x∈ET,ϵx\in E_{T,\epsilon}, we obtain

Comparing with (113) as in the previous subsection, we obtain (118). ∎

3 Proof of Theorem 1.1(a) and Theorem 1.2(a)

Recall the outline of the proof described in Section 2. The proof proceed exactly same for both convex and non-convex potentials. The only important assumption is that 0<a<ac0<a<\mathbf{a}_{c}.

Since H(x)>H(c)\mathbf{H}(x)>\mathbf{H}(c) for all x>cx>c and H(x)→∞\mathbf{H}(x)\to\infty fast by Lemma 1.1, this term is larger than O(n(1+∣x∣)−j)O(\sqrt{n}(1+|x|)^{-j}). Inserting this into (106), we obtain

On the other hand, for x∈ET,ϵ:=[e+TβN+1n2/3,e+ϵ]x\in E_{T,\epsilon}:=[\mathbf{e}+\frac{T}{\beta_{N+1}n^{2/3}},\mathbf{e}+\epsilon] (see (116)), we have from Lemma 3.3 that

where ξ\xi is defined by (117). Similarly, for x≥e+ϵx\geq\mathbf{e}+\epsilon,

Theorem 1.1(a) and Theorem 1.2(a) are proved.

The proof of Theorem 1.2(b) is divided into three cases, a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}) and a=12V′(e)a=\frac{1}{2}V^{\prime}(\mathbf{e}). The first case is in this subsection. The second case is in Section 4. The third case is discussed at the beginning of Section 5.

We assume that a∈(ac,12V′(e))a\in(\mathbf{a}_{c},\frac{1}{2}V^{\prime}(\mathbf{e})) and a∉JVa\notin\mathcal{J}_{V}. Let x0=x0(a)x_{0}=x_{0}(a) be the unique maximizer of G(x)\mathbf{G}(x) in (c,∞)(c,\infty) as in Lemma 1.3. We assume that G′′(x0)≠0\mathbf{G}^{\prime\prime}(x_{0})\neq 0. See Remark 3.1 at the end of this subsection for a discussion when G′′(x0)=0\mathbf{G}^{\prime\prime}(x_{0})=0 (see (59)).

Lemma 1.1(a) and (b) imply that H(x)\mathbf{H}(x) increases monotonically in x>cx>c and H(x)>G(x)\mathbf{H}(x)>\mathbf{G}(x) for all x>ex>\mathbf{e}. Hence there exists ϵ′>0\epsilon^{\prime}>0 such that H(x)>G(x0)\mathbf{H}(x)>\mathbf{G}(x_{0}) for all x>x0−ϵ′x>x_{0}-\epsilon^{\prime}. In particular, H(x)>G(x0)\mathbf{H}(x)>\mathbf{G}(x_{0}) for x∈JnT(x0)x\in J_{n}^{T}(x_{0}). Therefore (106) yields, noting that H(x)→∞\mathbf{H}(x)\to\infty fast enough by Lemma 1.1(e),

Inserting the explicit asymptotics (93) for Γn−j(a)\mathbf{\Gamma}_{n-j}(a) into (134), we have for x>x0−ϵ′x>x_{0}-\epsilon^{\prime} where ϵ′\epsilon^{\prime} is the positive constant mentioned above, and in particular for x∈JnT(x0)x\in J_{n}^{T}(x_{0}) that

From the assumptions for the Theorem 1.2, G(x)\mathbf{G}(x) in (c,∞)(c,\infty) has the unique maximum at x=x0x=x_{0} and G(x)=G(x0)+12G′′(x0)(x−x0)2+O(∣x−x0∣3)\mathbf{G}(x)=\mathbf{G}(x_{0})+\frac{1}{2}\mathbf{G}^{\prime\prime}(x_{0})(x-x_{0})^{2}+O(|x-x_{0}|^{3}) for xx close to x0x_{0} where G′′(x0)<0\mathbf{G}^{\prime\prime}(x_{0})<0. Also Mj,n(x)M_{j,n}(x), Mj,n′(x)M^{\prime}_{j,n}(x) and 1/Mj,n(x)1/M_{j,n}(x) are bounded uniformly in nn for xx in a compact subset of (e,∞)(\mathbf{e},\infty) and Mj,n(x)=Mj,n(x)(1+o(1))M_{j,n}(x)=\mathcal{M}_{j,n}(x)(1+o(1)) from Proposition 6.1(a),. Hence the standard Laplace’s method applies and we obtain

When G′′(x0)=0\mathbf{G}^{\prime\prime}(x_{0})=0, the Gaussian function e−12ξ2e^{-\frac{1}{2}\xi^{2}} in (137) is replaced by a higher-order function such as e−ξ2ke^{-\xi^{2k}}(k>1k>1). The rest of the proof is very similar. The result is the limit theorem as in (59).

5 Proof of Theorem 1.3(b)

Let VV be a potential such that ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\not\in\mathcal{J}_{V}. We assume that G′′(x0(ac);ac)≠0\mathbf{G}^{\prime\prime}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0. Let

where (we omit the dependence of C0C_{0} and C1(α)C_{1}(\alpha) on nn and jj to make the notations simple)

The constants C0C_{0} and C1(α)C_{1}(\alpha) are positive from Proposition 6.1. If α\alpha is fixed, C0C_{0}, C1(α)C_{1}(\alpha), C0−1C^{-1}_{0} and C1−1(α)C^{-1}_{1}(\alpha) are uniformly bounded in nn. Set

From the definition, pj,n(α)p_{j,n}(\alpha) is a decreasing function in α\alpha, pj,n(α)→0p_{j,n}(\alpha)\to 0 as α→∞\alpha\to\infty and pj,n(α)→1p_{j,n}(\alpha)\to 1 as α→−∞\alpha\to-\infty for each fixed nn. Also for a fixed α\alpha, pj,n(α)p_{j,n}(\alpha) is in a compact subset of (0,1)(0,1) uniformly in nn. Note that when the support of the equilibrium consists of one interval, then C0C_{0} and C1(α)C_{1}(\alpha) are independent of nn, and hence so is pj,n(α)p_{j,n}(\alpha). We prove formulas (48) and (47) in Theorem 1.3 separately.

where pj,n(0)(α)p^{(0)}_{j,n}(\alpha) is defined in (145). The estimate (139) follows from the same calculations in Subsection 3.4, and we obtain from (76) that

We now prove (47). When aa is given by (141), the estimate (124) still holds. Similar to (146), we obtain by estimates (142), (124) and (118) that

We prove Theorem 1.4 when a0<12V′(e)a_{0}<\frac{1}{2}V^{\prime}(\mathbf{e}). The case when a0≥12V′(e)a_{0}\geq\frac{1}{2}V^{\prime}(\mathbf{e}) will be discussed in Sections 4 and 5.

Let a0∈(ac,12V′(e))a_{0}\in(\mathbf{a}_{c},\frac{1}{2}V^{\prime}(\mathbf{e})) and a0∈JVa_{0}\in\mathcal{J}_{V}. Hence a0a_{0} is a secondary critical point. In this case, the maximum of G(x;a0)\mathbf{G}(x;a_{0}), x∈(c,∞)x\in(c,\infty), is attained at more than one point. The case when the maximum of G(x;a0)\mathbf{G}(x;a_{0}) is attained at more than two points can be attained by a straightforward extension and this yields (52). We omit the details in that case.

Denote the two maximizers of G(x;a0)\mathbf{G}(x;a_{0}) by x1:=x1(a0)x_{1}:=x_{1}(a_{0}) and x2:=x2(a0)x_{2}:=x_{2}(a_{0}). Let x1(a0)<x2(a0)x_{1}(a_{0})<x_{2}(a_{0}). Assume that

The case when one of the derivative vanishes is discussed in Subsection 3.7. Let

Therefore, as in (93) we obtain as n→∞n\to\infty (note that G(x1;a0)=G(x2;a0)\mathbf{G}(x_{1};a_{0})=\mathbf{G}(x_{2};a_{0}) and xi:=xi(a0)x_{i}:=x_{i}(a_{0}))

With this asymptotics of Γn−j(a)\mathbf{\Gamma}_{n-j}(a), the rest of the analysis is similar to (135), and we obtain for x∈JnT(x1)x\in J_{n}^{T}(x_{1}),

Like C0C_{0} in (143) and C1(α)C_{1}(\alpha) in (144), Ai(α)A_{i}(\alpha) is positive and is of finite distance away from uniformly in nn. For each i=1,2i=1,2, if we set

The properties of pj,n(i)(α)p_{j,n}^{(i)}(\alpha) stated in Theorem 1.4 can be easily checked.

Thus Theorem 1.4 when a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}) is proved.

We prove Theorem 1.6 when a0<12V′(e)a_{0}<\frac{1}{2}V^{\prime}(\mathbf{e}). The case when a0≥12V′(e)a_{0}\geq\frac{1}{2}V^{\prime}(\mathbf{e}) will be discussed in Sections 4 and 5.

Under the assumption of Theorem 1.6, for some k>1k>1

We consider the double-scaling situation when

The analysis is similar to Subsection 3.6. For each i=1,2i=1,2, we have, as in (154),

As in (156), for x∈JnT(x1)x\in J_{n}^{T}(x_{1}),

From the definition, the properties of pj,n(i)(α)p^{(i)}_{j,n}(\alpha) in Theorem 1.6 follow easily.

Thus it follows as in (162) and (163) that

and Theorem 1.6 when a0<12V′(e)a_{0}<\frac{1}{2}V^{\prime}(\mathbf{e}) is proven.

Note that if a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}), then a>aca>\mathbf{a}_{c}. In this section, we prove Theorem 1.1(b) and Theorems 1.2(b), 1.4 and 1.6 for the case when aa (or a0a_{0}) >12V′(e)>\frac{1}{2}V^{\prime}(\mathbf{e}). After a small change at the first step, the analysis is the same as in the case when ac<a<12V′(e)\mathbf{a}_{c}<a<\frac{1}{2}V^{\prime}(\mathbf{e}) discussed in Subsection 3.4,3.6 and 3.7. The proof of Theorem 1.1 (b) is identical to the proof of Theorem 1.2 (b).

Note that c(a)=ec(a)=\mathbf{e} in this case (see Definition 1.1). Since G′(e)>0\mathbf{G}^{\prime}(\mathbf{e})>0 when a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}), Gmax⁡(a):=max⁡{G(x;a):x∈[e,∞)}\mathbf{G}_{\max}(a):=\max\{\mathbf{G}(x;a):x\in[\mathbf{e},\infty)\} satisfies Gmax⁡(a)>G(e)=H(e)\mathbf{G}_{\max}(a)>\mathbf{G}(\mathbf{e})=\mathbf{H}(\mathbf{e}). Let ϵ>0\epsilon>0 be small enough so that all the maximizers of G\mathbf{G} are in (e+2ϵ,∞)(\mathbf{e}+2\epsilon,\infty) and

Let a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}). As n→∞n\to\infty while j=O(1)j=O(1),

As in (85), we write Γn−j(a)=Γn−j(a;n)\mathbf{\Gamma}_{n-j}(a)=\mathbf{\Gamma}_{n-j}(a;n) as

where, for a large enough but fixed positive constant CΓˉC_{\bar{\Gamma}}, (cf. the contour Γ\Gamma defined in (84))

and Γˉ−\bar{\Gamma}_{-} is the reflected image of Γˉ+\bar{\Gamma}_{+} about the real axis. The contours are oriented as indicated in Figure 8.

As in (86), by using (320) for (Cφn−j)(z)(C\varphi_{n-j})(z), the contour integral over Γˉ\bar{\Gamma} in (190) satisfies

On the other hand, consider the second integral in (190):

By using the Laplace’s method, we find an estimate similar to (91). Hence we find that (194) is exponentially larger than (193) due to the assumption (187). Thus (188) is proven.

Using this formula, due to the property of the H(x;a)\mathbf{H}(x;a) on Γˉ±\bar{\Gamma}_{\pm} and G(x;a)\mathbf{G}(x;a) on (e+ϵ,∞)(\mathbf{e}+\epsilon,\infty), the analysis of the proof of Lemma 3.2 applies without any changes. If we restrict x≥e+2ϵx\geq\mathbf{e}+2\epsilon, then the error term O(n(1+∣x∣)−j)O(\sqrt{n}(1+|x|)^{-j}) in (106) can be replaced by O((1+∣x∣)−j)O((1+|x|)^{-j}) since ∣x−z∣≥ϵ|x-z|\geq\epsilon for z∈Γˉ±z\in\bar{\Gamma}_{\pm} as in the first part of the proof of Lemma 3.1. We skip the details. ∎

First, suppose that a=12V′(e)>aca=\frac{1}{2}V^{\prime}(\mathbf{e})>\mathbf{a}_{c}. Then Gmax⁡(a):=max⁡{G(x;a)∣x∈[e,∞)}\mathbf{G}_{\max}(a):=\max\{\mathbf{G}(x;a)\mid x\in[\mathbf{e},\infty)\} satisfies Gmax⁡(a)>H(e)=G(e)\mathbf{G}_{\max}(a)>\mathbf{H}(\mathbf{e})=\mathbf{G}(\mathbf{e}) (recall Definition 34 and (33)). This property is enough to prove Lemma 4.1 and the analysis of Section 4 applies without any change. Hence we obtain the proof of Theorem 1.2(b), 1.4 and 1.6 when a=12V′(e)>aca=\frac{1}{2}V^{\prime}(\mathbf{e})>\mathbf{a}_{c}. Combining the results of the previous two sections, we have proved all theorems except for Theorems 1.1(b), 1.3(a) and 1.5.

Theorem 1.1(b) and Theorem 1.3(a) share the same proof and this is given in Subsection 5.1. The proof of Theorem 1.5 is in Subsection 5.2.

Let VV be a potential such that ac=12V′(e)\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}). We assume that ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V}. (This holds under the assumption of convexity of Theorem 1.1(a).) Then G(e;ac)>G(x;ac)\mathbf{G}(\mathbf{e};\mathbf{a}_{c})>\mathbf{G}(x;\mathbf{a}_{c}) for all x>ex>\mathbf{e}. We consider a double-scaling situation when

Here Bj,n(z)\mathcal{B}_{j,n}(z) is given in (322). Note that Bj,n(e)\mathcal{B}_{j,n}(\mathbf{e}) is in a compact subset of (0,∞)(0,\infty) independent of nn.

In the proof of Lemma 3.1 when a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), we have taken the contour Γ±\Gamma_{\pm} to pass the point c=c(a)c=c(a) at which ℜH(z;a)\Re\mathbf{H}(z;a), z∈Γ±z\in\Gamma_{\pm}, takes its maximum (see (85)). Near this point, we had H(z;a)−H(c(a);a)∼κ(z−c(a))2\mathbf{H}(z;a)-\mathbf{H}(c(a);a)\sim\kappa(z-c(a))^{2} for some constant κ>0\kappa>0. This quadratic term changes when a=ac=12V′(e)a=\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}). In this case, c(ac)=ec(\mathbf{a}_{c})=\mathbf{e}, and (note (30))

With the above preliminary computation in mind, we defineHere, the exact shape and the angle of the contour from z=ez=\mathbf{e} is not important. For example, we can use the contour that extends straightly upward from z=ez=\mathbf{e} as in Figure 5 with cc replaced by e\mathbf{e}. The local behavior H(z;ac)−H(e;ac)∼κ(z−e)3/2\mathbf{H}(z;\mathbf{a}_{c})-\mathbf{H}(\mathbf{e};\mathbf{a}_{c})\sim\kappa(z-\mathbf{e})^{3/2} near z=ez=\mathbf{e} shows that ℜH(z)\Re\mathbf{H}(z) decays as zz travels vertically away from e\mathbf{e} at least locally. One can check ℜH(z)\Re\mathbf{H}(z) indeed decreases as zz moves away from e\mathbf{e} along on the entire curve. Our choice of the contour Σ\Sigma is made for the convenience of the formulas that appear later. the contours Σ±\Sigma_{\pm} as (see Figure 9)

where ω:=e2πi/3\omega:=e^{2\pi i/3}. Here ϵ\epsilon is a fixed constant chosen to satisfy the condition (215) below, and CΣC_{\Sigma} is a positive fixed constant large enough, say, greater than 1/(2a)1/(2a). As in (85), we have

We first consider the part of the first integral in (202) over Σ2+ess⁡\Sigma^{\operatorname{ess}}_{2+}. Inserting the asymptotics (324) for (Cφn−j)(z)(C\varphi_{n-j})(z), there are two terms, one involving Ai⁡(ω2Φ(z))\operatorname{Ai}(\omega^{2}\Phi(z)) and the other involving Ai⁡′(ω2Φ(z))\operatorname{Ai}^{\prime}(\omega^{2}\Phi(z)). We compute each of the integrals using the change of variables z↦ξz\mapsto\xi defined by

This change of variables and the double scaling (196) imply that

uniformly in z∈Σ2+ess⁡z\in\Sigma^{\operatorname{ess}}_{2+}, where (recall Lemma 1.1(c))

as defined in (198). Therefore, using the property (310) of Φ(z)\Phi(z), and noting that ∣z−e∣≤n−11/21|z-\mathbf{e}|\leq n^{-11/21}, the two integrals involving Ai⁡(ω2Φ(z))\operatorname{Ai}(\omega^{2}\Phi(z)) and Ai⁡′(ω2Φ(z))\operatorname{Ai}^{\prime}(\omega^{2}\Phi(z)) satisfy

Observe that the integrals involving Ai⁡(ξ)\operatorname{Ai}(\xi) and Ai⁡′(ξ)\operatorname{Ai}^{\prime}(\xi) are convergent as these functions decay faster than exponential functions as ξ→+∞\xi\to+\infty. From these, we find that

Now consider Σ2+∖Σ2+ess⁡\Sigma_{2+}\setminus\Sigma^{\operatorname{ess}}_{2+}. By the property (310) of Φ(z)\Phi(z), we have that for ∣z−e∣<1\lvert z-\mathbf{e}\rvert<1, there exists c1>0c_{1}>0 such that

Hence the asymptotics of Ai⁡(ξ)\operatorname{Ai}(\xi) and Ai⁡′(ξ)\operatorname{Ai}^{\prime}(\xi) as ξ→∞\xi\to\infty ([1, 10.4.59 and 10.4.61]) imply that z∈Σ2+z\in\Sigma_{2+}, if ∣z−e∣≤β(1−(3/4)2/3)/c1|z-\mathbf{e}|\leq\beta(1-(3/4)^{2/3})/c_{1}, then

Also for ∣z−e∣<1\lvert z-\mathbf{e}\rvert<1, there exists c2>0c_{2}>0 such that (cf. (205))

Hence if we take ϵ\epsilon in (201) small enough so that

then combining (213) and (214), we have, for n≥(8α)14/β7n\geq(8\alpha)^{14}/\beta^{7},

For the rest of Σ+\Sigma_{+}, by a direct calculation as in the inequalities (87) and (88), we find that ℜ(H(z;a))\Re(H(z;a)) decreases strictly as zz travels away from e+ωϵ\mathbf{e}+\omega\epsilon along Σ2′+∪Σ3\Sigma_{2^{\prime}+}\cup\Sigma_{3}. Also by direct calculation we verify that

where ϵˉ′\bar{\epsilon}^{\prime} is a positive constant depending on ϵ\epsilon. Since H(z;a)−H(z;ac)=βαn1/3z→0\mathbf{H}(z;a)-\mathbf{H}(z;\mathbf{a}_{c})=\frac{\beta\alpha}{n^{1/3}}z\to 0 as n→∞n\to\infty for a fixed zz, the difference (217) with ac\mathbf{a}_{c} replaced by aa is also bounded below by 12ϵˉ′\frac{1}{2}\bar{\epsilon}^{\prime} for large enough nn. Thus, from Proposition 6.1(b),

Combining (209), (216) and (218), we obtain

The integral over Σ−\Sigma_{-} can be evaluated in a similar way. Alternatively we can use the symmetry (Cφn−j)(zˉ)=−(Cφn−j)(z)‾(C\varphi_{n-j})(\bar{z})=-\overline{(C\varphi_{n-j})(z)}. We have

For the integral over (e,∞)(\mathbf{e},\infty) in (202), we again consider three intervals (e,e+n−11/21](\mathbf{e},\mathbf{e}+n^{-11/21}], (e+n−11/21,e+ϵ)(\mathbf{e}+n^{-11/21},\mathbf{e}+\epsilon) and [e+ϵ,∞)[\mathbf{e}+\epsilon,\infty), and proceed as before. We now use the asymptotics (322) for φn−j(z)\varphi_{n-j}(z) in the first two intervals and (318) for the third one. Note the similarity of (322) and (324). The calculation is similar and we obtain

Combining (219), (220) and (221), we find

Let 0<ϵ<2δ00<\epsilon<2\delta_{0} be the constant in (201), satisfying the condition (215). For x∈ET,ϵ/2:=[e+β−1n−2/3T,e+ϵ/2]x\in E_{T,\epsilon/2}:=[\mathbf{e}+\beta^{-1}n^{-2/3}T,\mathbf{e}+\epsilon/2], we have

where ξ\xi is defined by the relation x=e+β−1n−2/3ξx=\mathbf{e}+\beta^{-1}n^{-2/3}\xi as in (117), QnQ_{n} is given in (198) and Cα(ξ)C_{\alpha}(\xi) is defined in (18). For x≥e+ϵ/2x\geq\mathbf{e}+\epsilon/2, we have

Note that ξ∈[T,∞)\xi\in[T,\infty). Let Cˉ<T\bar{C}<T be a real number, and set Cn:=β−1n−2/3CˉC_{n}:=\beta^{-1}n^{-2/3}\bar{C}. For x∈InTx\in I_{n}^{T} (hence x>e+Cnx>\mathbf{e}+C_{n}), we have, as in Lemma 3.1,

Here Σ±+Cn\Sigma_{\pm}+C_{n} denotes the contour Σ±\Sigma_{\pm} translated by CnC_{n}. For example, Σ++Cn=(Σ2++Cn)∪(Σ2′++Cn)∪(Σ3+Cn)\Sigma_{+}+C_{n}=(\Sigma_{2+}+C_{n})\cup(\Sigma_{2^{\prime}+}+C_{n})\cup(\Sigma_{3}+C_{n}), cf. (200). We divide the proof of Lemma 5.2 into two parts.

First we consider the integral over Σ++Cn\Sigma_{+}+C_{n} in (226). For x∈ET,ϵ/2x\in E_{T,\epsilon/2} and z∈Σ2++Cnz\in\Sigma_{2+}+C_{n}, from (322) and (324),

Observe that Wi(x,z)−Wi(x,x)x−z=O(1)\frac{W_{i}(x,z)-W_{i}(x,x)}{x-z}=O(1), i=1,2i=1,2. For

using the estimates (211) and (212) for Ai⁡(ω2Φ(z))\operatorname{Ai}(\omega^{2}\Phi(z)) and Ai⁡′(ω2Φ(z))\operatorname{Ai}^{\prime}(\omega^{2}\Phi(z)), and analogous estimates for Ai⁡(Φ(x))\operatorname{Ai}(\Phi(x)) and Ai⁡′(Φ(x))\operatorname{Ai}^{\prime}(\Phi(x)), we find that (noting that the ξ\xi in (211) and (212) are slightly different from the ξ\xi and η\eta in (230))

for xx and zz in (230). For z∈(Σ2′++Cn)∪(Σ3++Cn)z\in(\Sigma_{2^{\prime}+}+C_{n})\cup(\Sigma_{3+}+C_{n}), noting that ∣x−z∣≥1/ϵ|x-z|\geq 1/\epsilon, a straightforward calculation using (322) and (320) implies that

The estimates for the integral over the contour Σ−+Cn\Sigma_{-}+C_{n} can be obtained either by Schwarz reflection principle or by a similar calculation. We find

For the integral over (e+Cn,∞)(\mathbf{e}+C_{n},\infty) in (226), we need asymptotics of Kn−j,n(x,y)K_{n-j,n}(x,y). For x∈ET,ϵ/2x\in E_{T,\epsilon/2} and y∈(e+Cn,e+ϵ)y\in(\mathbf{e}+C_{n},\mathbf{e}+\epsilon), setting x=e+β−1n−2/3ξx=\mathbf{e}+\beta^{-1}n^{-2/3}\xi and y=e+β−1n−2/3ηy=\mathbf{e}+\beta^{-1}n^{-2/3}\eta, we have

This follows from the analysis similar to that of (231). A weaker estimate is in (341), which is actually enough for our purpose. Hence for x∈ET,ϵ/2x\in E_{T,\epsilon/2},

Now consider the integral over (e+ϵ,∞)(\mathbf{e}+\epsilon,\infty). By the estimate (339) of Kn−j,n(x,y)K_{n-j,n}(x,y) for x∈ET,ϵ/2x\in E_{T,\epsilon/2} and y∈(e+ϵ,∞)y\in(\mathbf{e}+\epsilon,\infty) and the identity

where we require ℜη<ℜξ\Re\eta<\Re\xi in (242) and (242). This can be verified by using Ai⁡′′(z)=zAi⁡(z)\operatorname{Ai}^{\prime\prime}(z)=z\operatorname{Ai}(z) and the asymptotics [1, 10.4.59 and 10.4.61] of Ai⁡(z)\operatorname{Ai}(z) and Ai⁡′(z)\operatorname{Ai}^{\prime}(z) as z→∞z\to\infty. Using the above Airy function identities, we find that

From these results and (226), (233), (234) and (240), we find that for x∈ET,ϵ/2x\in E_{T,\epsilon/2},

Now the sum of three integrals inside the parentheses equals eα3/3e^{\alpha^{3}/3} (cf. (223)), for all tt. In order to see this, first note that the sum is independent of tt since its derivative with respect to tt equals from the Airy function identity

Then set t=0t=0 and call the sum S(α)S(\alpha). Taking the derivative of S(α)S(\alpha) with respect to α\alpha and using (248) and the differential equation for the Airy function, we find that S′(α)=α2S(α)S^{\prime}(\alpha)=\alpha^{2}S(\alpha). Now by noting that S(0)=1S(0)=1 since ∫0∞Ai⁡(ηˉ)dηˉ=1/3\int_{0}^{\infty}\operatorname{Ai}(\bar{\eta})d\bar{\eta}=1/3, we obtain that S(α)=eα3/3S(\alpha)=e^{\alpha^{3}/3}. Hence

uniformly for x∈ET,ϵ/2x\in E_{T,\epsilon/2}. Therefore using (197) we find that

uniformly for x=e+β−1n−2/3ξ∈ET,ϵ/2x=\mathbf{e}+\beta^{-1}n^{-2/3}\xi\in E_{T,\epsilon/2}. In the last line, we used the identity

Let x≥e+ϵ/2x\geq\mathbf{e}+\epsilon/2. Using (338) and (214), a straightforward estimate implies that

For the integral on Σ±+Cn\Sigma_{\pm}+C_{n}, the calculation is easier than the proof of (224) since ∣x−z∣≥ϵ/2|x-z|\geq\epsilon/2. Straightforward estimates using Proposition 6.1 imply that

1.3 Proof

From Lemma 5.2 and Proposition 6.1, and using (214) to estimate 1Qnen(ax−V(x)/2)−eαξ\frac{1}{Q_{n}}e^{n(ax-V(x)/2)}-e^{\alpha\xi}, we obtain

for x=e+βn2/3ξ∈ET,ϵ/2x=\mathbf{e}+\beta n^{2/3}\xi\in E_{T,\epsilon/2}. For x≥e+ϵ/2x\geq\mathbf{e}+\epsilon/2,

The calculation is similar to Subsubsection 5.1.2 and we skip the details. Thus

Hence Theorem 1.1(b) and Theorem 1.3(a) are proved.

2 Proof of Theorem 1.5

Note that G(x0(ac);ac)=G(e;ac)>G(x;ac)\mathbf{G}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})=\mathbf{G}(\mathbf{e};\mathbf{a}_{c})>\mathbf{G}(x;\mathbf{a}_{c}) for all x∈(e,∞)∖{x0(ac)}x\in(\mathbf{e},\infty)\setminus\{x_{0}(\mathbf{a}_{c})\}. For aa given in either (54) or (56), let x0(a)x_{0}(a) be the point near x0(ac)x_{0}(\mathbf{a}_{c}) such that G(x;a)\mathbf{G}(x;a) achieves its local maximum. The point x0(a)x_{0}(a) is well defined as long as ∣a−ac∣\lvert a-\mathbf{a}_{c}\rvert is small enough. Note that for a≥aca\geq\mathbf{a}_{c}, x0(a)x_{0}(a) is same as in the definition of x0(a)x_{0}(a) in Lemma 1.3. However, for a<aca<\mathbf{a}_{c}, x0(a)x_{0}(a) is not defined in Lemma 1.3. We extend the definition of x0(a)x_{0}(a) here for a<aca<\mathbf{a}_{c} when a−aca-\mathbf{a}_{c} is small enough.

where aa is in a compact subset of (−∞,0)(-\infty,0). Since we assume G′′(x0(ac);ac)≠0G^{\prime\prime}(x_{0}(\mathbf{a}_{c});\mathbf{a}_{c})\neq 0, we have x0(a)−x0(ac)=O(∣a−ac∣)=O(n−1/3)x_{0}(a)-x_{0}(\mathbf{a}_{c})=O(|a-\mathbf{a}_{c}|)=O(n^{-1/3}). We also have, as in (97), using ∂∂aG(x;a)=x\frac{\partial}{\partial a}\mathbf{G}(x;a)=x,

Hence since G(e;a)=G(e;ac)+(a−ac)e\mathbf{G}(\mathbf{e};a)=\mathbf{G}(\mathbf{e};\mathbf{a}_{c})+(a-\mathbf{a}_{c})\mathbf{e} by the definition of G\mathbf{G},

We first evaluate Γn−j(a)\mathbf{\Gamma}_{n-j}(a) as in Lemma 5.1. Note that in Subsection 5.1.1, we used properties of H(z;a)\mathbf{H}(z;a) for the integrals over Σ±\Sigma_{\pm} and properties of G(x;a)\mathbf{G}(x;a) for the integral over (e,∞)(\mathbf{e},\infty). Since there is no change in the properties of H(z;a)\mathbf{H}(z;a), the integrals over Σ+\Sigma_{+} and Σ−\Sigma_{-} are computed exactly the same as given by (219) and (220). For the integral over (e,∞)(\mathbf{e},\infty), note that the main contribution to (221) was from the part of yy near e\mathbf{e} since G(y;a)\mathbf{G}(y;a) takes its maximum for yy near e\mathbf{e}. However, now due to (263) we need to add a contribution from yy near x0(a)x_{0}(a). By using the standard Laplace’s method as in (99), the contribution to the integral near x0(a)x_{0}(a) equals

for all large enough nn since α<0\alpha<0. Hence we find that

as in Lemma 5.1. Adding the integrals on the contours Σ±\Sigma_{\pm}, we obtain

However, due to (266), this is again QnO(n−1/3e−35∣ξ∣3/2)Q_{n}O(n^{-1/3}e^{-\frac{3}{5}\lvert\xi\rvert^{3/2}}) as in (238) . Therefore the result (224) still holds for x∈ET,ϵ/2x\in E_{T,\epsilon/2}. For x∈(e+ϵ/2,∞)x\in(\mathbf{e}+\epsilon/2,\infty), the estimates (254) and (252) hold without any change. Moreover, it is straightforward to check that (253) still holds. Therefore (225) holds for x≥e+ϵ/2x\geq\mathbf{e}+\epsilon/2. Therefore, Lemma 5.2 holds without any changes.

by (266). This implies that (256) holds without a change. Similarly, it is straightforward to check that (259) holds. Therefore, we obtain (260) and Theorem 1.5(a) is proved.

2.2 Proof of Theorem 1.5(b)

First we consider Γn−j(a)\mathbf{\Gamma}_{n-j}(a). There are two changes from the previous subsubsection. The first is that since α\alpha defined in (261) and α′\alpha^{\prime} defined in (271) are related as α=β−1n−2/3α′\alpha=\beta^{-1}n^{-2/3}\alpha^{\prime}, we have α→0\alpha\to 0 and hence in (219), (220) and (265), we have α=0\alpha=0 in the integrals involving the Airy function. The second is that (267) does not follows from (265) since (266) no longer holds. Instead, due to (273), (265) implies that

Hence adding (219) and (220) (with α=0\alpha=0), we obtain

The formulas (278) and (279) are different from (224) and (225) only by the factor pj,n(α′)p_{j,n}(\alpha^{\prime}).

We now prove the theorem. First, consider (58). From (279) and (330), we obtain

by using (272) and (273). Also, for x∈JnT(x0(ac))x\in J_{n}^{T}(x_{0}(\mathbf{a}_{c})), by (336) and (279)

The first term is calculated as in Subsubsection 5.2.1 with the only change that the prefactor pj,n(α′)p_{j,n}(\alpha^{\prime}) is multiplied:

Summary of asymptotics of orthogonal polynomials and the Christoffel-Darboux kernel

Fix δ>0\delta>0 small enough. Let (see Figure 10)

where e\mathbf{e} is the rightmost end-point of the support of the equilibrium measure. Comparing with notations in , AδA_{\delta} is the circle Dϵ,aN+1D_{\epsilon,a_{N+1}} with δ\delta corresponding to the radius ϵ\epsilon. in [17, Figure 1.4]. As in [17, Figure 1.4], AδA_{\delta} is divided into four regions I, II, III and IV. Let ΣR\Sigma_{R} be the contour in [17, Figure 4.9]. We assume that the boundary of AδA_{\delta} is a part of ΣR\Sigma_{R} and BδB_{\delta} is outside of the lens-shaped regions, cf. [17, Formula (4.116)].

Several notations from are used in this section, and we summarize them in Table 1. Other notations may be slightly different but should be clear.

By following the procedure of , we find asymptotics of YY. Noting the symmetry

The outer parametrix Mj,n(∞)(z)M^{(\infty)}_{j,n}(z) solves the Riemann-Hilbert problem (cf. [17, Formulas (4.24)–(4.26)])

Note that the dependence on jj in the asymptotics as z→∞z\to\infty. The solution of this Riemann-Hilbert problem can be solved as in [17, Lemma 4.3]). Setting

The asymptotics (293) especially implies the asymptotics of γn−j\gamma_{n-j}. Since (cf. [16, Formulas (3.10) and (3.11)])

See [17, Formulas (1.62) and (1.63)] for the cases j=1j=1 and j=0j=0.

Now consider z∈Aδz\in A_{\delta}. Then the analysis of the local parametrix as in [17, Section 4.3] implies that (cf. [17, (4.119)–(4.121)] )

for zz is in regions I and IV in [17, Figure 1.4],

for zz is in regions II in [17, Figure 1.4], and

for zz is in regions III in [17, Figure 1.4]. Here the local parametrix (Mj,n)p(M_{j,n})_{p} is given by (cf. [17, Formulas (4.75) and (4.76)])

where Φ(z)\Phi(z) denotes ΦaN+1(z)\Phi_{a_{N+1}}(z) in . We note that by definition

with β\beta defined in (22) (see [17, Equations (1.34), (1.35), (4.74)]).

We now summarize the asymptotics the orthonormal polynomials and their Cauchy transformations. For notational convenience, we denote for z∈Bδz\in B_{\delta}

There exists δ0>0\delta_{0}>0 such that for each fixed δ∈(0,δ0]\delta\in(0,\delta_{0}], the following holds as n→∞n\to\infty and j=O(1)j=O(1).

where Mj,n(z)M_{j,n}(z) is an analytic function in BδB_{\delta} and

uniformly in zz and nn. The function Mj,nM_{j,n} satisfies that (i) Mj,n(z)=O(z−j)M_{j,n}(z)=O(z^{-j}) uniformly in nn as z→∞z\to\infty, (ii) in any compact subset K∈BδK\in B_{\delta}, Mj,n(z)M_{j,n}(z), Mj,n′(z)M^{\prime}_{j,n}(z) and 1/Mj,n(z)1/M_{j,n}(z) are O(1)O(1) uniformly in nn and z∈Kz\in K, and (iii) Mj,n(x)>0\mathcal{M}_{j,n}(x)>0 and Mj,n(x)>0M_{j,n}(x)>0 for all real x>ex>\mathbf{e}.

where Bj,n(z)B_{j,n}(z) and Dj,n(z)D_{j,n}(z) are analytic functions in AδA_{\delta} and

uniformly in zz and nn. The functions Bj,nB_{j,n} and Dj,nD_{j,n} satisfy (i) Bj,n(z)B_{j,n}(z), Dj,n(z)D_{j,n}(z), Bj,n′(z)B^{\prime}_{j,n}(z), Dj,n′(z)D^{\prime}_{j,n}(z), 1/Bj,n(z)1/B_{j,n}(z) and 1/Dj,n(z)1/D_{j,n}(z) are O(1)O(1) uniformly in nn and z∈Aδz\in A_{\delta} and (ii) Bj,n(x)>0\mathcal{B}_{j,n}(x)>0 and Bj,n(x)>0B_{j,n}(x)>0 for x∈(e−δ,e+δ)x\in(\mathbf{e}-\delta,\mathbf{e}+\delta).

By formulas (300) and (301) of Mj,n(∞)(z)M^{(\infty)}_{j,n}(z), the properties of the theta function θ\theta and the definition of dd, we have that for p,q=1,2p,q=1,2, the functions (Mj,n(∞))pq(z)(M^{(\infty)}_{j,n})_{pq}(z) and (Mj,n(∞))pq(z)−1(M^{(\infty)}_{j,n})_{pq}(z)^{-1} are uniformly bounded for zz in any compact subset K⊂BδK\subset B_{\delta} and the functions

We use the following identity in the analysis. It is straightforward to derive from the Riemann-Hilbert problem of Yk(z;n)Y_{k}(z;n) that det⁡Yk(z;n)≡1\det Y_{k}(z;n)\equiv 1. This implies that

Taking k=n−jk=n-j and using asymptotic formulas (322), (324) and (325) in (326), with the help of [1, 10.4.11 and 10.4.12]

Proposition 6.1 implies the following asymptotic properties of ψn−j\psi_{n-j}. These are used in the main analysis extensively.

Let ET,ϵ:=[e+β−1n−2/3T,e+ϵ]E_{T,\epsilon}:=[\mathbf{e}+\beta^{-1}n^{-2/3}T,\mathbf{e}+\epsilon] be the interval defined in (116). For x∈ET,ϵx\in E_{T,\epsilon},

Let InT:=[e+β−1n−2/3T,∞)I_{n}^{T}:=\left[\mathbf{e}+\beta^{-1}n^{-2/3}T,\infty\right) be the interval defined in (23). Then

Also for every xˉ\bar{x} in (e+ϵ,∞)(\mathbf{e}+\epsilon,\infty), there is ϵ′>0\epsilon^{\prime}>0 such that

As n→∞n\to\infty, vj,n(ξ):=ψn−j(e+β−1n−2/3ξ)v_{j,n}(\xi):=\psi_{n-j}(\mathbf{e}+\beta^{-1}n^{-2/3}\xi) satisfies

For (b), note that T≤ξ≤ϵn2/3T\leq\xi\leq\epsilon n^{2/3}. Thus, ∣Ai⁡(ξ)∣≤Ce−23∣ξ∣3/2|\operatorname{Ai}(\xi)|\leq Ce^{-\frac{2}{3}|\xi|^{3/2}}and ∣Ai⁡′(ξ)∣≤C(∣ξ∣1/4+1)e−23∣ξ∣3/2≤C′n1/6e−23∣ξ∣3/2|\operatorname{Ai}^{\prime}(\xi)|\leq C(|\xi|^{1/4}+1)e^{-\frac{2}{3}|\xi|^{3/2}}\leq C^{\prime}n^{1/6}e^{-\frac{2}{3}|\xi|^{3/2}} for some constants C,C′>0C,C^{\prime}>0. From (322) and the behavior of Φ(z)\Phi(z) in AϵA_{\epsilon}, we obtain the estimate with the factor 23\frac{2}{3} changed to a smaller constant which can be made arbitrarily close to 23\frac{2}{3} if we take ϵ\epsilon smaller. To be definite, we fix this constant as 35\frac{3}{5}.

For (c), by the asymptotics (330) and (331) of ψn−1\psi_{n-1}, we find

Item (d) follows from Proposition 6.1 (c). ∎

The above asymptotics for ψn−j\psi_{n-j} yields the asymptotics for the Christoffel-Darboux kernel Kn−j,n(x,y)K_{n-j,n}(x,y).

For x,y∈(e+ϵ/2,∞)x,y\in(\mathbf{e}+\epsilon/2,\infty),

where ξ:=βn2/3(x−e)\xi:=\beta n^{2/3}(x-\mathbf{e}) and η:=βn2/3(y−e)\eta:=\beta n^{2/3}(y-\mathbf{e}).

For x∈(e+ϵ,∞)x\in(\mathbf{e}+\epsilon,\infty) and y∈ET,ϵ/2y\in E_{T,\epsilon/2},

For x∈ET,ϵ/2x\in E_{T,\epsilon/2} and y∈(e+ϵ,∞)y\in(\mathbf{e}+\epsilon,\infty),

All estimates above are uniform in x,yx,y in their domains and in nn.

Item (c) and (d) follow directly the asymptotics (330) and (331) of ψn−j\psi_{n-j}, and the Christoffel-Darboux formula (69) of Kn−j,n(x,y)K_{n-j,n}(x,y), noting that x−yx-y never vanishes.

For x,y∈(e+ϵ/2,∞)x,y\in(\mathbf{e}+\epsilon/2,\infty), (330) implies that

Since Mj,nM_{j,n} and its derivatives are uniformly bounded, we obtain (a) .

Item (b) follows from a similar calculation but using the asymptotics (322). The calculation is direct and is the same as [14, Formula (3.8)]. ∎

We also need the following results for the Christoffel-Darboux kernel.

for all x,y∈InTx,y\in I_{n}^{T} as n→∞n\to\infty, where ξ:=(x−e)βn2/3\xi:=(x-\mathbf{e})\beta n^{2/3} and η:=(y−e)βn2/3\eta:=(y-\mathbf{e})\beta n^{2/3}.

Define the operator Kn−j,n\mathcal{K}_{n-j,n} by kernel

The operator norms of \big{(}1-\chi_{I_{n}^{T}}K_{n-j,n}\chi_{I_{n}^{T}}\big{)}^{-1} are bounded uniformly in nn. As a corollary, The operator norms of

are also bounded uniformly in nn and in xˉn\bar{x}_{n} as long as xˉn\bar{x}_{n} are in a compact subset of (e,∞)(\mathbf{e},\infty).

for any xˉ\bar{x} is in a compact subset of (e,∞)(\mathbf{e},\infty).

The proof of a result similar to (a) for the non-varying weight is given in [14, Formula (3.8)] . The varying weight case is proved in the same way. Note that our CC is the cc in [14, Formula (3.8)], which can be assumed to be an arbitrarily large positive number.

The proof of a result similar to (b) for the non-varying weight is given in the proof of the β=2\beta=2 case in [14, Corollary 1.4] . The varying weight case is proved in the same way.

References