The largest eigenvalue of real symmetric, Hermitian and Hermitian self-dual random matrix models with rank one external source, part I

Dong Wang

Introduction and statement of results

In this paper we will be concerned with the distribution of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)} in the following ensembles of matrices {M}\{M\}:

The set of n×nn\times n real symmetric matrices, with the probability distribution function (p.d.f.)

The set of n×nn\times n Hermitian matrices, with the p.d.f.

The set of 2n×2n2n\times 2n self-dual Hermitian matrices, with the p.d.f.

Note that in these three external source models, the distributions of eigenvalues of MM are unchanged if An,β\mathbf{A}_{n,\beta} (or A^n,β\hat{\mathbf{A}}_{n,\beta}) is changed into QAn,βQ−1Q\mathbf{A}_{n,\beta}Q^{-1} (or QA^n,βQ−1Q\hat{\mathbf{A}}_{n,\beta}Q^{-1}), where QQ is in the orthogonal group O(n)O(n), unitary group U(n)U(n) and compact symplectic group Sp(n)Sp(n) for β=1,2,4\beta=1,2,4 respectively. Since we are only concerned with the distribution of eigenvalues of MM, we assume An,β\mathbf{A}_{n,\beta} (or A^n,β\hat{\mathbf{A}}_{n,\beta}) to be diagonal without loss of generality. To make our presentation uniform for all values of β\beta, we let V(x)V(x) be a fixed function and

be an n×nn\times n diagonal matrix. We assume that Vβ(x)V_{\beta}(x) (or V^β(x)\hat{V}_{\beta}(x)) and An,β\mathbf{A}_{n,\beta} (or A^n,β\hat{\mathbf{A}}_{n,\beta}) are defined from V(x)V(x) and An\mathbf{A}_{n} such that

Writing a 2n×2n2n\times 2n self-dual Hermitian matrix into 2×22\times 2 blocks (astbstcstdst)s,t=1n\left(\begin{smallmatrix}a_{st}&b_{st}\\ c_{st}&d_{st}\end{smallmatrix}\right)^{n}_{s,t=1}, we can express it as a quaternionic Hermitian matrix (qst)s,t=1n(q_{st})^{n}_{s,t=1} whose s,ts,t-entry comes from the s,ts,t-block by

In the quaternion form, the p.d.f. of the Hermitian self-dual external source model is

with An\mathbf{A}_{n} defined in (4). The An,4\mathbf{A}_{n,4} defined in (10) corresponds to the A^n,4\hat{\mathbf{A}}_{n,4} defined in (7). In Appendix A we use the quaternion form p.d.f. (9) of the 44-external source model to streamline the derivations for all β\beta.

In this paper we concentrate on the rank 11 case, i.e.,

Random matrices are powerful tools to simulate Hamiltonians of complex systems. Different types of random matrices, namely the real symmetric (aka orthogonal), the Hermitian (aka unitary) and the Hermitian self-dual (aka symplectic) ensembles are used for physical systems with different properties of time-reversal invariance . For random matrix models without external source in all the three types of ensembles, i.e., rank β\beta-external source models, the distribution of the largest eigenvalue has been studied extensively for all the three β\beta. If β=2\beta=2, for all real analytic potentials V2(x)V_{2}(x) under mild regularity conditions, the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)} approaches e\mathbf{e}, the right-end point of the equilibrium measure of V2(x)V_{2}(x) (see (16) below), with probability 11 as n→∞n\to\infty, and the limiting distribution is the GUE Tracy-Widom distribution. See e.g. and . If β=1\beta=1, for real analytic potentials V1(x)V_{1}(x) satisfying the “one-band” condition (cf. Condition 2 in Subsection 1.2 below) and mild regularity conditions, the largest eigenvalue with probability 11 approaches e\mathbf{e} as n→∞n\to\infty, and the limiting distribution is the GOE Tracy-Widom distribution. See . If β=4\beta=4, similar result can be obtained and the limiting distribution is the GSE Tracy-Widom distribution. See .

The random matrix model with external source was proposed by Brézin and Hikami , to simulate complex systems with both random part and deterministic part. Although in all three types of random matrix ensembles the random matrix model with external source can be defined, due to technical reasons, only the Hermitian (β=2\beta=2) type has been studied for general potential functions. See e.g. and references therein.

In , the Hermitian random matrix model with rank 11 external source was studied for all real analytic potentials V2(x)V_{2}(x) under mild regularity conditions. For convex potentials, the universality of phase transition was proved. Let V2(x)V_{2}(x) be defined by V(x)V(x) as in (5). In the rank 11 22-external source model, with probability 11, as n→∞n\to\infty

where aa is the unique nonzero eigenvalue of the external source An,2=An\mathbf{A}_{n,2}=\mathbf{A}_{n}, and x0(a)x_{0}(a) is a continuous increasing function in a∈(12V′(e),∞)a\in(\frac{1}{2}V^{\prime}(\mathbf{e}),\infty) such that x0(a)→ex_{0}(a)\to\mathbf{e} as a→12V′(e)a\to\frac{1}{2}V^{\prime}(\mathbf{e}), see (16) and (29). If a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} is the GUE Tracy-Widom distribution, and if a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}) the limiting distribution is Gaussian. For the double scaling a=12V′(e)+αn1/3a=\frac{1}{2}V^{\prime}(\mathbf{e})+\frac{\alpha}{n^{1/3}}, the limiting distribution is the generalized Tracy-Widom distribution. If the potential is not convex, then new phenomena may occur. The “critical value” may be less than 12V′(e)\frac{1}{2}V^{\prime}(\mathbf{e}), and there may be “secondary critical values”. The largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)} may converge to two or more points if aa takes such values. The results were also obtained by Bertola, Buckingham, Lee and Pierce in and independently.

For real symmetric and Hermitian self-dual matrix models with external source, known results are limited to special potentials. Let V1(x)V_{1}(x) and V^4(x)\hat{V}_{4}(x) be defined by V(x)V(x) as in (5), the rank 11 11-external source model with Gaussian potential (V(x)=x2V(x)=x^{2} on the real line) and Laguerre potential (V(x)=x−clog⁡(x)V(x)=x-c\log(x) on half of real line) are studied in e.g. , , and . The limiting location of the largest eigenvalue is given by formula (12), the same as in the corresponding rank 11 22-external source model, where aa is the nonzero eigenvalue of An\mathbf{A}_{n} and An,1\mathbf{A}_{n,1} is defined by (6). If a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}), then the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} is Gaussian, with variance twice of that in the corresponding Hermitian (β=2\beta=2) external source model. If a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} is the GOE Tracy-Widom distribution. The rank 11 44-external source model with Laguerre potential is studied in , where the limiting location of the largest eigenvalue is found to be given by formula (12), the same as in the corresponding rank 11 22-external source model, where aa is the nonzero eigenvalue of An\mathbf{A}_{n} and A^n,4\hat{\mathbf{A}}_{n,4} is defined by (7). If a>12V′(e)a>\frac{1}{2}V^{\prime}(\mathbf{e}), then the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} is Gaussian, with variance half of that in the corresponding Hermitian (β=2\beta=2) external source model. If a<12V′(e)a<\frac{1}{2}V^{\prime}(\mathbf{e}), the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} is the GSE Tracy-Widom distribution. In the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} when a=12V′(e)a=\frac{1}{2}V^{\prime}(\mathbf{e}) is also obtained.

In the recent preprint , Bloemendal and Virág obtained the limiting distribution of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)} when the potential is Gaussian or Laguerre, for all β\beta and for all aa. When aa is at or near 12V′(e)\frac{1}{2}V^{\prime}(\mathbf{e}), they described the limiting distribution function of ξmax⁡(n)\xi_{\max}{(n)} via the unique solution to a PDE. The recent preprint by Mo indicates a new approach to study the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} in the rank 11 11-external source model with Laguerre potential when aa is at or near 12V′(e)\frac{1}{2}V^{\prime}(\mathbf{e}), see also . The contour integral formula in [25, Theorem 1] is equivalent to that of Proposition 2.2 in this paper with β=1\beta=1 and Laguerre potential (cf. Remark A.1). In , Mo further simplified the integrand in the contour integral formula, (see [25, Theorem 3],) and he applied it in the asymptotic analysis in to obtain a result similar to that in . In this paper, we take a different approach to apply Proposition 2.2 in asymptotic analysis. The reader may also compare our paper with the paper by Benaych-Georges and Nadakuditi, where they considered a different kind of low rank perturbations of large random matrices.

In this paper, we consider the rank 11 β\beta-external source models with general potential Vβ(x)V_{\beta}(x) (or V^β(x)\hat{V}_{\beta}(x)) which are defined by V(x)V(x). The conditions satisfied by V(x)V(x) will be given in Subsection 1.2. We find that the “critical value” is independent of β\beta, and for all β=1,2,4\beta=1,2,4 find the limiting location of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)} when aa, the nonzero eigenvalue of An\mathbf{A}_{n}, is not equal to the critical value. When aa is greater than the critical value, we also find the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)}.

Besides the asymptotic results summarized above, in Appendix A we also have an algebraic result: the definition of the β\beta-external source model with general β>0\beta>0. Here we note that the analytic method presented in this paper can be used to study the rank 11 β\beta-external source model with general β\beta.

2 Assumptions on V​(x)𝑉𝑥V(x)

Throughout this paper, we assume four conditions on V(x)V(x), the function in (5) and (10). The first is

V(x)V(x) is a polynomial of degree 2l2l and with positive leading coefficient.

The equilibrium measure μ\mu associated to V(x)V(x) is supported on a single interval J=[b1,b2]J=[b_{1},b_{2}].

For the function V(x)V(x) satisfying Conditions 1 and 2, the equilibrium measure μ\mu has the form

where χJ\chi_{J} is the indicator function and h(x)h(x) is a polynomial of degree 2l−22l-2. The next condition assumed on V(x)V(x) is

The function h(x)h(x) in the formula (13) of the equilibrium measure μ\mu of V(x)V(x) has only non-real zeros.

The equilibrium measure dμ=Ψ(x)dxd\mu=\Psi(x)dx is characterized by the conditions

Conditions 1–3 are assumed to apply Proposition 4.1 in our paper, and they are not used anywhere else in this paper. If Proposition 4.1 can be proved under weaker conditions, e.g. the conditions assumed in [22, Theorem 1] Mariya Shcherbina informed the author that Proposition 4.1 can be proved under the consitions assumed in [22, Theorem 1] through private communication., these conditions can be weakened accordingly.

Functions VV satisfying all Conditions 1–4 also satisfy the assumptions of VV in [3, Formulas (6)–(8)]. Thus all the results in on VV can be applied in this paper.

If V(x)V(x) is a convex polynomial with positive leading coefficient, V(x)V(x) satisfies Conditions 1–3 by [21, Proposition 3.1], and it is straightforward to verify that V(x)V(x) satisfies Condition 4.

3 Preliminary notations

To state the results in this paper, we need a few more notations. We follow the notational convention in to denote the right edge of the support of the equilibrium measure

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

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

The properties of g(x)\mathbf{g}(x) used in this paper is summarized below (see [3, Formula (30)]).

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

The convexity of g(x)\mathbf{g}(x) on (e,∞)(\mathbf{e},\infty) yields that for u>c(a)u>c(a),

It is proved in [3, Lemma 1.2] that AV\mathcal{A}_{V} is an open, semi-infinite interval. From AV\mathcal{A}_{V} we define

It is also proved in [3, Lemma 1.2] that ac>0\mathbf{a}_{c}>0.

For a>aca>\mathbf{a}_{c} and a∉JVa\not\in\mathcal{J}_{V}, there is a unique x0(a)∈(c(a),∞)x_{0}(a)\in(c(a),\infty) such that (cf. [3, Lemma 1.3])

For a>aca>\mathbf{a}_{c} and a∈JVa\in\mathcal{J}_{V}, there are r≥2r\geq 2 and c(a)<x1(a)<x2(a)<⋯<xr(a)c(a)<x_{1}(a)<x_{2}(a)<\dots<x_{r}(a) such that

We define the set of secondary critical values as JV∖{ac}\mathcal{J}_{V}\setminus\{\mathbf{a}_{c}\} (cf. [3, Definition 1.3] ).

If the potential VV is convex for x≥ex\geq\mathbf{e}, JV=∅\mathcal{J}_{V}=\emptyset. See [3, Remark 1.2].

4 Statement of main results

Let V(x)V(x) be a function that satisfies Conditions 1–4. For any nn and β=1,2,4\beta=1,2,4, let the nn-dimensional β\beta-external source models be defined by p.d.f.s (1), (2) and (3) respectively, with potentials Vβ(x)V_{\beta}(x) (or V^β(x)\hat{V}_{\beta}(x)) given by (5) and external sources An,β\mathbf{A}_{n,\beta} (or A^n,β\hat{\mathbf{A}}_{n,\beta}) given by (4), (6) and (7). We assume that An\mathbf{A}_{n} has only one nonzero eigenvalue aa, as in (11). In each nn-dimensional β\beta-external source model, let ξmax⁡(n)\xi_{\max}{(n)} be the largest eigenvalue of the random matrix. The theorems below are stated uniformly for all β\beta-external source models (β=1,2,4\beta=1,2,4). In the case β=1\beta=1, we assume that the dimension nn is even. For β=1\beta=1 and nn is odd, the theorems below also hold, and we discuss it briefly in Appendix A. First we show the limiting location of the largest eigenvalue.

The following hold for each fixed aa as n→∞n\to\infty:

If 0<a<ac0<a<\mathbf{a}_{c}, or a=ac=12V′(e)a=\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V}, ξmax⁡(n)→e\xi_{\max}(n)\to\mathbf{e} with probability 11.

If a>aca>\mathbf{a}_{c} and ac∉JV\mathbf{a}_{c}\not\in\mathcal{J}_{V}, then ξmax⁡(n)→x0(a)\xi_{\max}(n)\to x_{0}(a) with probability 11, where x0(a)x_{0}(a) is defined in (29).

If a>aca>\mathbf{a}_{c} and a∈JVa\in\mathcal{J}_{V}, then there exist r≥2r\geq 2 and x1(a)x_{1}(a), …, xr(a)x_{r}(a) defined in (30). Under the assumption that G′′(xj(a))≠0\mathbf{G}^{\prime\prime}(x_{j}(a))\neq 0 for all j=1,…,rj=1,\dots,r, then ξmax⁡(n)\xi_{\max}(n) converges to xj(a)x_{j}(a) with nonzero probability pj,β(0)p_{j,\beta}(0) for j=1,…,rj=1,\dots,r. Here pj,β(0)p_{j,\beta}(0) are defined in (168) and ∑j=1rpj,β(0)=1\sum^{r}_{j=1}p_{j,\beta}(0)=1.

If a<0a<0, Theorem 1.1(a) still holds, and the method of proof is similar to that in the 0<a<ac0<a<\mathbf{a}_{c} case. Since when a<0a<0 there is no interesting phase transition phenomenon for the distribution of the largest eigenvalue (while there is a similar one of the smallest eigenvalue) and the proof is long and parallel to the a>0a>0 case, we skip further discussions about the a<0a<0 case.

If a>aca>\mathbf{a}_{c}, we have the limiting distribution of the largest eigenvalue. If aa is not at or near secondary critical values, we have the following result that strengthens Theorem 1.1(b).

The following hold for a>aca>\mathbf{a}_{c} and a∉JVa\not\in\mathcal{J}_{V} as n→∞n\to\infty.

where Φ(T):=12π∫−∞Te−12ξ2dξ\Phi(T):=\frac{1}{\sqrt{2\pi}}\int^{T}_{-\infty}e^{-\frac{1}{2}\xi^{2}}d\xi denotes the cumulative distribution function of standard normal distribution.

If a>aca>\mathbf{a}_{c} is at or near a secondary critical value, we have the following result that shows the double scaling case and strengthens Theorem 1.1(c).

Suppose that a0>aca_{0}>\mathbf{a}_{c} and a0∈JVa_{0}\in\mathcal{J}_{V}. Assume that G(x;a0)\mathbf{G}(x;a_{0}) attains its maximum at r≥2r\geq 2 points x1(a0)<x2(a0)<⋯<xr(a0)x_{1}(a_{0})<x_{2}(a_{0})<\dots<x_{r}(a_{0}) in (c(a0),∞)(c(a_{0}),\infty), and G′′(xi(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{i}(a_{0});a_{0})\neq 0 for all i=1,2,…,ri=1,2,\dots,r, then for

where pi,β(α)p_{i,\beta}(\alpha) (i=1,…,ri=1,\dots,r) are defined in (168) and ∑j=1rpj,β(α)=1\sum^{r}_{j=1}p_{j,\beta}(\alpha)=1. Furthermore, pr,β(α)→1p_{r,\beta}(\alpha)\to 1 as α→∞\alpha\to\infty and p1,β(α)→1p_{1,\beta}(\alpha)\to 1 as α→−∞\alpha\to-\infty.

The phenomenon of Theorem 1.3 occurs for some quartic potential VV that satisfies Conditions 1–4. For example, V(x)=0.02093x4−0.16736x3+0.37448x2+0.11418xV(x)=0.02093x^{4}-0.16736x^{3}+0.37448x^{2}+0.11418x.

In the case that a>aca>\mathbf{a}_{c}, a∈JVa\in\mathcal{J}_{V} and G′′(xj(a);a)=0\mathbf{G}^{\prime\prime}(x_{j}(a);a)=0 at at least one maximizer xj(a)x_{j}(a) of G(x;a)\mathbf{G}(x;a) in (c(a),∞)(c(a),\infty), we show hereafter an example when the number of maximizers of G(x;a)\mathbf{G}(x;a) in (c(a),∞)(c(a),\infty) is r=2r=2. The result for general case is similar.

Suppose that a0>aca_{0}>\mathbf{a}_{c} and a0∈JVa_{0}\in\mathcal{J}_{V}. Assume that G(x;a0)\mathbf{G}(x;a_{0}) attains its maximum at two points x1(a0)<x2(a0)x_{1}(a_{0})<x_{2}(a_{0}) in (c(a0),∞)(c(a_{0}),\infty), with G′′(x1(a0);a0)≠0\mathbf{G}^{\prime\prime}(x_{1}(a_{0});a_{0})\neq 0, G(2k)(x2(a0);a0)≠0\mathbf{G}^{(2k)}(x_{2}(a_{0});a_{0})\neq 0 and G(j)(x2(a0);a0)=0\mathbf{G}^{(j)}(x_{2}(a_{0});a_{0})=0 for j=1,…,2k−1j=1,\dots,2k-1. Then for

The limiting distribution of the largest eigenvalue when a≤aca\leq\mathbf{a}_{c}, as well as the limiting location of the largest eigenvalue when aa is at or near ac<12V′(e)\mathbf{a}_{c}<\frac{1}{2}V^{\prime}(\mathbf{e}), will be analyzed in a subsequent paper.

The paper is organized as follows. In Section 2, we calculate the limiting p.d.f. of the largest eigenvalue in the rank 11 β\beta-external source model as n→∞n\to\infty, based on Proposition 2.1. In Section 3, we prove Theorems 1.1, 1.2 1.3 and 1.4. The proof of Proposition 2.1 is in Section 4.

The starting point of the asymptotic analysis in this paper is Proposition 2.2, the contour integral formula of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)}. Since its proof is combinatorial, we postpone it to Appendix A. In this appendix we also propose a definition of the β\beta-external source model for any β>0\beta>0. In Appendix B we show that the results in this paper agree with those in when β=2\beta=2.

The p.d.f. of the largest eigenvalue

where Zm,β\mathbf{Z}_{m,\beta} is the normalization constant. Suppose F(x1,…,xm)F(x_{1},\dots,x_{m}) is an integrable function with respect to the measure μm,β\mu_{m,\beta} defined in (38), define the expectation of FF with respect to μm,β\mu_{m,\beta} by

Then we can state the technical tool in the asymptotic analysis of this section:

where Rβ(u)R_{\beta}(u) is defined in (192).

where Rβ(u,w0)R_{\beta}(u,w_{0}) is defined in (191).

Let ϵ\epsilon be a small positive constant. For all ww such that dist⁡(w,(−∞,e])≥ϵ\operatorname{dist}(w,(-\infty,\mathbf{e}])\geq\epsilon and ∣w∣≤ϵ−1\lvert w\rvert\leq\epsilon^{-1},

where the factor O(1)O(1) is bounded uniformly in ww.

This proposition is a corollary of a theorem of Johansson [21, Theorem 2.4], and we put off its proof to Section 4.

For the asymptotic analysis in this section, we define four types of contours: Σs1,s2x\Sigma^{x}_{s_{1},s_{2}}, Πsx\Pi^{x}_{s}, Γsx\Gamma^{x}_{s} and IsxI^{x}_{s}, where xx is a real parameter and s1s_{1}, s2s_{2} and ss are positive parameters. We assume s2>s1/2s_{2}>s_{1}/\sqrt{2} for Σs1,s2x\Sigma^{x}_{s_{1},s_{2}} and allow s=∞s=\infty in Γsx\Gamma^{x}_{s}. The contours Πsx\Pi^{x}_{s} and Σs1,s2x\Sigma^{x}_{s_{1},s_{2}} will be used in Subsections 2.1 and 2.2 respectively. The contours IsxI^{x}_{s} and Γsx\Gamma^{x}_{s} represent the local parts of Πsx\Pi^{x}_{s} and Σs1,s2x\Sigma^{x}_{s_{1},s_{2}} around the point xx respectively, which will turn out to be the saddle point in the asymptotic analysis.

See Figures 4, 4, 4 and 4 for these contours. For any real number rr, we define

The asymptotic analysis in this section is based on the contour integral representation of the p.d.f. of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)}:

Let ξmax⁡(n)\xi_{\max}{(n)} be the largest eigenvalue in the nn-dimensional rank 11 β\beta-external source model for β=1,2,4\beta=1,2,4, where the potential Vβ(x)V_{\beta}(x) (or V^β(x)\hat{V}_{\beta}(x)) is defined by (5) from V(x)V(x), and the external source matrix An,β\mathbf{A}_{n,\beta} (or A^n,β\hat{\mathbf{A}}_{n,\beta}) is defined by (6) (or (7)) from An\mathbf{A}_{n} in (11) with a>0a>0. Then for any integer nn if β=2,4\beta=2,4 and for even integer nn if β=1\beta=1,

where C^n,β\hat{C}_{n,\beta} is a constant, Zn−1,β(u,w)Z_{n-1,\beta}(u,w) is defined in (40), and C\mathcal{C} is either Σs1,s2x\Sigma^{x}_{s_{1},s_{2}} defined in (51) or Πsx\Pi^{x}_{s} defined in (52) with x>ux>u.

The proof of Proposition 2.2 is in Appendix A.

Let LL be a positive number. For sufficiently large nn, the contour IL/nc(a)I^{c(a)}_{L/\sqrt{n}} is part of Ππ1c(a)\Pi^{c(a)}_{\pi_{1}}. By Proposition 2.1(b), for w=c(a)+it/n∈IL/nc(a)w=c(a)+it/\sqrt{n}\in I^{c(a)}_{L/\sqrt{n}}, the integrand in the contour integral of (56) satisfies

Using the asymptotic formula (57), we have the result

and ϵ1(L,n)\epsilon_{1}(L,n) is small if LL and nn are large. To be precise, for all ϵ>0\epsilon>0, there is an L1>0L_{1}>0 such that for all L>L1L>L_{1}, ∣ϵ1(L,n)∣<ϵ\lvert\epsilon_{1}(L,n)\rvert<\epsilon for nn large enough.

For ww in a bounded subset of Ππ1c(a)∖IL/nc(a)\Pi^{c(a)}_{\pi_{1}}\setminus I^{c(a)}_{L/\sqrt{n}}, we use Proposition 2.1(c) and estimate the integrand of the contour integral of (56)

If w(t)∈Ππ1c(a)∖IL/nc(a)w(t)\in\Pi^{c(a)}_{\pi_{1}}\setminus I^{c(a)}_{L/\sqrt{n}} with t≥π1t\geq\pi_{1}, i.e., ww is in the ray from c(a)+iπ1c(a)+i\pi_{1} to −∞-\infty, we have

If π1\pi_{1} is large enough, we have that for all t∈[π1,∞)t\in[\pi_{1},\infty) and all x∈Jx\in J, there exists c1>0c_{1}>0 such that

For 0<t≤π10<t\leq\pi_{1}, like (62) and (63), we have

where c2c_{2} is a positive constant depending on π1\pi_{1}.

where the factor O(1)O(1) is bounded uniformly in LL. Substituting the Taylor expansion (210) of p(x;u,w)p(x;u,w) into (66), we find

By (66) and (67), we find that ϵ2(L,n)\epsilon_{2}(L,n) is small if LL and nn are large. To be precise, for any ϵ>0\epsilon>0, there exists L2>0L_{2}>0 such that for all L>L2L>L_{2}, ∣ϵ2(L,n)∣<ϵ\lvert\epsilon_{2}(L,n)\rvert<\epsilon for sufficiently large nn.

Hence substituting (69) into (40), we have

Similar to (206) and (201), we have (see Remark 4.1)

where g(u)\mathbf{g}(u) is defined in (17), H(c(a);a)\mathbf{H}(c(a);a) is defined in (21), and

Let LL be a positive number. For sufficiently large nn, the contour ΓL/nu+n−1\Gamma^{u+n^{-1}}_{L/n} is part of Σσ1,σ2u+n−1\Sigma^{u+n^{-1}}_{\sigma_{1},\sigma_{2}}. By Proposition 2.1(a), for w=u+z/n∈ΓL/nu+n−1w=u+z/n\in\Gamma^{u+n^{-1}}_{L/n} the integrand in the contour integral of (56) satisfies

Using Hankel’s contour integral expression of Gamma function (See [1, 6.1.4]), we find

Comparing the integral on the right-hand side of (80) with the left-hand side of (81), we write analogous to (58) that

and the term ϵ3(L,n)\epsilon_{3}(L,n) is small if LL and nn are large. To be precise, for any ϵ>0\epsilon>0, there is an L3>0L_{3}>0 such that for all L>L3L>L_{3}, ∣ϵ3(L,n)∣<ϵ\lvert\epsilon_{3}(L,n)\rvert<\epsilon for sufficiently large nn.

If w=w(t)∈Σσ1,σ2u+n−1w=w(t)\in\Sigma^{u+n^{-1}}_{\sigma_{1},\sigma_{2}} and 0≤t≤σ10\leq t\leq\sigma_{1}, i.e., ww is in the line segment between u+n−1u+n^{-1} and u+n−1+e3πi4σ1u+n^{-1}+e^{\frac{3\pi i}{4}}\sigma_{1}, we have

By (24), we know that H′(u;a)\mathbf{H}^{\prime}(u;a) is a positive number. If σ1\sigma_{1} is small enough, for all t∈[0,σ1]t\in[0,\sigma_{1}] and all x∈Jx\in J

Hence for 0≤t≤σ10\leq t\leq\sigma_{1}, substituting (85) in (84), we find with the help of (24)

If w=w(t)∈Σσ1,σ2u+n−1w=w(t)\in\Sigma^{u+n^{-1}}_{\sigma_{1},\sigma_{2}} and t≥σ2+(1−2/2)σ1t\geq\sigma_{2}+(1-\sqrt{2}/2)\sigma_{1}, i.e., ww is in the ray from u+n−1−σ1/2+iσ2u+n^{-1}-\sigma_{1}/\sqrt{2}+i\sigma_{2} to −∞-\infty, like (62) we have

If σ2\sigma_{2} is large enough, like (63) we have that for all t∈[σ2+(1−2/2)σ1,∞)t\in[\sigma_{2}+(1-\sqrt{2}/2)\sigma_{1},\infty) and all x∈Jx\in J, if nn is large enough

Substituting (88) into (87), we find that like (88), for t≥σ2+(1−2/2)σ1t\geq\sigma_{2}+(1-\sqrt{2}/2)\sigma_{1}

If w=w(t)∈Σσ1,σ2u+n−1w=w(t)\in\Sigma^{u+n^{-1}}_{\sigma_{1},\sigma_{2}} and σ1≤t≤σ2+(1−2/2)σ1\sigma_{1}\leq t\leq\sigma_{2}+(1-\sqrt{2}/2)\sigma_{1}, i.e., ww is in the line segment between u+n−1+e3πi4σ1u+n^{-1}+e^{\frac{3\pi i}{4}}\sigma_{1} and u+n−1−σ1/2+iσ2u+n^{-1}-\sigma_{1}/\sqrt{2}+i\sigma_{2} we have

where the last factor O(1)O(1) is bounded uniformly in LL. Substituting the Taylor expansion (207) of p(x;u,w)p(x;u,w) into (61), we find that like (67)

By (91) and (92), we find that ϵ4(L,n)\epsilon_{4}(L,n) is small if LL and nn are large. To be precise, for any ϵ>0\epsilon>0, there is an L4>0L_{4}>0 such that for all L>L4L>L_{4}, ∣ϵ4(L,n)∣<ϵ\lvert\epsilon_{4}(L,n)\rvert<\epsilon for sufficiently large nn.

where G(u;a)\mathbf{G}(u;a) is defined in (20), Mβ(u)\mathcal{M}_{\beta}(u) is defined in (83) and Cn,β\mathbf{C}_{n,\beta} is defined in (78).

The inequality (98) is a straightforward consequence of the definitions (40) and (41) of Zn−1,β(u,w)Z_{n-1,\beta}(u,w) and Z^n−1,β(u,w)\hat{Z}_{n-1,\beta}(u,w).

Like (64), we have that for π2\pi_{2} large enough, for all t>π2t>\pi_{2} and x∈Jx\in J, there exists c1′>0c^{\prime}_{1}>0 such that (cf. (63) and (64))

For all 0<t≤π10<t\leq\pi_{1} and x∈Jx\in J, we have like (65) and (90) that

On the other hand, we assume that π4\pi_{4} is large enough such that for all x<ex<\mathbf{e},

Using the estimate (116) and (117) of Zn−1,β(u,w)Z_{n-1,\beta}(u,w), we find by direct calculation

Thus similar to (116), we have by (122) that for w∈Π1u+1w\in\Pi^{u+1}_{1}

Using the estimates (123) and (124) of Zn−1,β(u,w)Z_{n-1,\beta}(u,w), we have like (118)

Proofs of Theorems 1.1, 1.2, 1.3 and 1.4

In this section we prove the main theorems in this paper. We divide the proofs into three subsections. In Subsection 3.1, we consider the case that 0<a<ac0<a<\mathbf{a}_{c} and the case that a=ac=12V′(e)a=\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V}, and prove Theorem 1.1(a). In Subsection 3.2, we consider the case that a>aca>\mathbf{a}_{c} and a∉JVa\not\in\mathcal{J}_{V}, and prove Theorems 1.2 and 1.1(b). In Subsection 3.3, we consider the case that a>aca>\mathbf{a}_{c} and a∈JVa\in\mathcal{J}_{V} and prove Theorems 1.3, 1.1(c) and 1.4.

First we consider the case that 0<a<ac0<a<\mathbf{a}_{c}. Let ϵ\epsilon be a small positive number, such that e+ϵ<c(a)\mathbf{e}+\epsilon<c(a) and e+ϵ−1>c(a)\mathbf{e}+\epsilon^{-1}>c(a). Furthermore we assume that ϵ\epsilon is small enough such that the inequalities (127), (129) and (131) hold.

The condition 0<a<ac0<a<\mathbf{a}_{c} implies the inequality H(c(a);a)>Gmax⁡(a)\mathbf{H}(c(a);a)>\mathbf{G}_{\max}(a), see (25)–(30) and [3, Lemma 1.2(d)]. We assume that

We assume that for u,v∈[c(a)−ϵ,c(a)+ϵ]u,v\in[c(a)-\epsilon,c(a)+\epsilon]

We assume that for u≥e+ϵ−1u\geq\mathbf{e}+\epsilon^{-1},

By (128), (130), (132), (134), we find that

Let ϵ′<ϵ/2\epsilon^{\prime}<\epsilon/2 be a small positive number such that

The probabilities (135), (136) and (137) imply that the conditional probability

Since [e+ϵ′,e+ϵ′]∪(e−ϵ,e+2ϵ′)∈[e−ϵ,e+ϵ][\mathbf{e}+\epsilon^{\prime},\mathbf{e}+\epsilon^{\prime}]\cup(\mathbf{e}-\epsilon,\mathbf{e}+2\epsilon^{\prime})\in[\mathbf{e}-\epsilon,\mathbf{e}+\epsilon], (138) implies that

Taking ϵ\epsilon arbitrarily small, we prove Theorem 1.1(a) when 0<a<ac0<a<\mathbf{a}_{c}.

The case when a=ac=12V′(e)a=\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V} is similar. Let ϵ\epsilon be a small enough positive number. Since a=12V′(e)a=\frac{1}{2}V^{\prime}(\mathbf{e}), we have c(a)=ec(a)=\mathbf{e}. Since a=ac∉JVa=\mathbf{a}_{c}\notin\mathcal{J}_{V}, there exists ϵ′>0\epsilon^{\prime}>0 depending on ϵ\epsilon such that for all u>e+ϵu>\mathbf{e}+\epsilon, G(u;a)<H(e;a)−ϵ′\mathbf{G}(u;a)<\mathbf{H}(\mathbf{e};a)-\epsilon^{\prime}. Thus like (128), for u∈[c(a)+ϵ,e+ϵ−1]u\in[c(a)+\epsilon,\mathbf{e}+\epsilon^{-1}] we have

When ϵ\epsilon is small enough, (132) and (134) also hold. Then by arguments similar to (135)–(139), we prove Theorem 1.1(a) when a=ac=12V′(e)a=\mathbf{a}_{c}=\frac{1}{2}V^{\prime}(\mathbf{e}) and ac∉JV\mathbf{a}_{c}\notin\mathcal{J}_{V}.

Let ϵ\epsilon be a small enough positive constant such that the maximizer x0(a)x_{0}(a) of G(x;a)\mathbf{G}(x;a) in [c(a),∞)[c(a),\infty) is less than e+ϵ−1\mathbf{e}+\epsilon^{-1}, and the inequalities (141), (145) and (147) are satisfied.

First we consider the case that ac<a<12V′(e)\mathbf{a}_{c}<a<\frac{1}{2}V^{\prime}(\mathbf{e}), i.e., c(a)>ec(a)>\mathbf{e}. We assume that

We assume that for all u∈[e−ϵ,e+ϵ]u\in[\mathbf{e}-\epsilon,\mathbf{e}+\epsilon]

We assume that for all u∈[c(a)−ϵ,c(a)+ϵ]u\in[c(a)-\epsilon,c(a)+\epsilon]

We assume that for u≥e+ϵ−1u\geq\mathbf{e}+\epsilon^{-1},

By (142), (144), (146), (148) and (150), we find that

In the case that a≥12V′(e)a\geq\frac{1}{2}V^{\prime}(\mathbf{e}), i.e., c(a)=ec(a)=\mathbf{e}, we find that inequalities (144), (148) and (150) still hold, and the estimate (151) holds with c(a)=ec(a)=\mathbf{e}.

For u∈[c(a)+ϵ,e+ϵ−1]u\in[c(a)+\epsilon,\mathbf{e}+\epsilon^{-1}], we have the asymptotic formula (97) and x0(a)x_{0}(a) is the unique maximum of G(x;a)\mathbf{G}(x;a) in [c(a)+ϵ,e+ϵ−1][c(a)+\epsilon,\mathbf{e}+\epsilon^{-1}]. If we further assume that G′′(x0(a);a)≠0\mathbf{G}^{\prime\prime}(x_{0}(a);a)\neq 0, by the standard Laplace’s method we have that

The probabilities (151), (152) and (153) imply Theorem 1.2(a).

If the second derivative of G(x;a)\mathbf{G}(x;a) vanishes at x0(a)x_{0}(a), due to the analyticity of G(x;a)\mathbf{G}(x;a), there exists k>1k>1 such that G(j)(x0(a);a)=0\mathbf{G}^{(j)}(x_{0}(a);a)=0 for j=1,…,2k−1j=1,\dots,2k-1 and G(2k)(x0(a);a)≠0\mathbf{G}^{(2k)}(x_{0}(a);a)\neq 0. By the Laplace’s method we have

The probabilities (151), (154) and (155) imply Theorem 1.2(b). Finally, Theorem 1.2 implies Theorem 1.1(b).

Let a0>aca_{0}>\mathbf{a}_{c}, and ϵ\epsilon be a small positive constant such that the inequalities (142), (144), (146), (148) and (150) hold with a=a0a=a_{0}. It is easy to verify that there exists a positive number ϵˉ\bar{\epsilon} depending on ϵ\epsilon such that if we take a=a0+ϵ′a=a_{0}+\epsilon^{\prime} with ϵ′∈[−ϵˉ,ϵˉ]\epsilon^{\prime}\in[-\bar{\epsilon},\bar{\epsilon}], the inequalities (142), (144), (146), (148) and (150) still hold with the same ϵ\epsilon. Thus the estimate of probability (151) still holds with a=a0+ϵ′a=a_{0}+\epsilon^{\prime}. If we further assume that

First we assume that a0∈JVa_{0}\in\mathcal{J}_{V} and G(x;a0)\mathbf{G}(x;a_{0}) has r≥2r\geq 2 maximizers x1(a0)<x2(a0)<⋯<xr(a0)x_{1}(a_{0})<x_{2}(a_{0})<\dots<x_{r}(a_{0}) in (c(a0),∞)(c(a_{0}),\infty), and all of them are less than e+ϵ−1\mathbf{e}+\epsilon^{-1}. Further we assume that for all i=1,…,ri=1,\dots,r

For xx around xi(a0)x_{i}(a_{0}) (i=1,…,ri=1,\dots,r), we denote

Let ϵi\epsilon_{i} (i=1,…,ri=1,\dots,r) be small enough constant numbers such that xi(a0)x_{i}(a_{0}) is the unique maximum of G(x;a0)\mathbf{G}(x;a_{0}) in [xi(a0)−ϵi,xi(a0)+ϵi][x_{i}(a_{0})-\epsilon_{i},x_{i}(a_{0})+\epsilon_{i}]. Applying the standard Laplace’s method to (97), near xi(a0)x_{i}(a_{0}) (i=1,2i=1,2), we obtain that

There exists ϵ′′>0\epsilon^{\prime\prime}>0 depending on ϵ1,…,ϵr\epsilon_{1},\dots,\epsilon_{r} such that for sufficiently large nn

From (168) we immediately find ∑j=1rpj,β(α)=1\sum^{r}_{j=1}p_{j,\beta}(\alpha)=1. By (167) and (168) we find that lim⁡α→∞pr,β(α)=1\lim_{\alpha\to\infty}p_{r,\beta}(\alpha)=1 and lim⁡α→−∞p1,β(α)=1\lim_{\alpha\to-\infty}p_{1,\beta}(\alpha)=1.

Therefore Theorem 1.3 is proved. Theorem 1.1(c) is a consequence of Theorem 1.3 with α=0\alpha=0.

Next we consider the case that r=2r=2 and for k>1k>1

Let ϵi\epsilon_{i} (i=1,2i=1,2) be small enough constant numbers such that xi(a0)x_{i}(a_{0}) is the unique maximum of G(x;a0)\mathbf{G}(x;a_{0}) in [xi(a0)−ϵi,xi(a0)+ϵi][x_{i}(a_{0})-\epsilon_{i},x_{i}(a_{0})+\epsilon_{i}]. Applying the standard Laplace’s method to (97), near x1(a0)x_{1}(a_{0}), we obtain similar to (163) and (164) that

Applying the Laplace’s method to (97), near x2(a0)x_{2}(a_{0}), we obtain

Also there exists ϵ′′>0\epsilon^{\prime\prime}>0 depending on ϵ1\epsilon_{1} and ϵ2\epsilon_{2} such that the estimate (166) holds. The probabilities (158), (166), (177), (178), (179), (180) show that the probability that ξmax⁡(n)\xi_{\max}{(n)} is in [x1−ϵ1,x1+ϵ1][x_{1}-\epsilon_{1},x_{1}+\epsilon_{1}] or [x2−ϵ2,x2+ϵ2][x_{2}-\epsilon_{2},x_{2}+\epsilon_{2}] approaches 11 as n→∞n\to\infty.

Proof of Proposition 2.1

The proof of Proposition 2.1 is based on a theorem of Johansson . For the convenience of readers we state it bellow.

[21, Theorem 2.4] Suppose the function VV satisfies Conditions 1–3, and μ\mu is the equilibrium measure associated to VV. Let ff be a real function that satisfies conditions (i)–(iii) below, with s=2s=2 if β=2\beta=2 and s=17/2s=17/2 if β≠2\beta\neq 2. Then there are a quadratic functional AA on ff and a signed measure ν\nu on supp⁡(μ)=J=[b1,b2]\operatorname{supp}(\mu)=J=[b_{1},b_{2}] which do not depend on nn, such that as n→∞n\to\infty

The quadratic functional AA is defined by

From the quadratic functional AA, we define the inner product ⟨⋅,⋅⟩A\langle\cdot,\cdot\rangle_{A} by

The explicit formula of ν(x)\nu(x) is more complicated and is given in [21, Formula (3.54)]. The conditions mentioned in Proposition 4.1 are (see [21, Page 157])

For any x0>0x_{0}>0, there is an α>0\alpha>0 such that hψx0∈Hs+αh\psi_{x_{0}}\in H^{s+\alpha}, where HsH^{s}, s>0s>0, is the standard L2L^{2} Sobolev space, and ψx0∈C∞\psi_{x_{0}}\in C^{\infty} is the function such that ψx0(x)=1\psi_{x_{0}}(x)=1 if ∣x∣≤x0\lvert x\rvert\leq x_{0}, ψx0(x)=0\psi_{x_{0}}(x)=0 if ∣x∣≥x0+1\lvert x\rvert\geq x_{0}+1 and 0≤ψx0(x)≤10\leq\psi_{x_{0}}(x)\leq 1.

The function Rβ(u,w)R_{\beta}(u,w) appearing in Proposition 2.1 is defined by

To facilitate the proof of Proposition 2.1, we define

where cc is a parameter no greater than uu. When c=uc=u, Zm,β(u,w;c)Z_{m,\beta}(u,w;c) and Z^m,β(u,w;c)\hat{Z}_{m,\beta}(u,w;c) become Zm,β(u,w)Z_{m,\beta}(u,w) and Z^m,β(u,w)\hat{Z}_{m,\beta}(u,w).

The proof of Proposition 2.1 is as follows. Recall that e\mathbf{e} is the right edge of JJ, the support of the equilibrium measure. Let cˉ=(e+u)/2\bar{c}=(\mathbf{e}+u)/2. We write

In case (a) where ww is given by (46), we assume the results

and find that (47) is the consequence of (196), (197), (198) and (199).

In case (b) where ww is given by (48), we assume the results

We still have (199), and (49) is the consequence of (200), (201), (202) and (199).

Below we prove the asymptotic formulas (196), (197), (198), (200), (201) and (203).

In the proof, cc stands for cˉ=(e+u)/2\bar{c}=(\mathbf{e}+u)/2 or uu.

f1(x)f_{1}(x) and f2(x)f_{2}(x) satisfy the conditions (i)–(iii) mentioned in Proposition 4.1.

f1(x)=f2(x)=p(x;u,w)f_{1}(x)=f_{2}(x)=p(x;u,w) for x≤ex\leq\mathbf{e}.

f1(x)≥p(x;u,w)f_{1}(x)\geq p(x;u,w) for x∈(e,c)x\in(\mathbf{e},c).

There exists x0∈(e,c)x_{0}\in(\mathbf{e},c) such that f2(x)≤p(x;u,w)f_{2}(x)\leq p(x;u,w) for x∈(e,x0)x\in(\mathbf{e},x_{0}) and f1(x)−f2(x)≥log⁡2f_{1}(x)-f_{2}(x)\geq\log 2 for x≥x0x\geq x_{0}.

As a consequence of the properties of f1(x)f_{1}(x) and f2(x)f_{2}(x), we have

By Proposition 4.1, we have for both i=1,2i=1,2 that

Thus by the sandwich inequality (204) and (194) we obtain

By (206), we complete the proof of (203) with c=uc=u. Let ww be given in (46), we have uniformly for all x≤ex\leq\mathbf{e} that

and we obtain the proof of (197) with c=cˉc=\bar{c} and the proof of (196) with c=uc=u. Let ww be given in (48), we have uniformly for all x≤ex\leq\mathbf{e} that

and we obtain the proof of (201) with c=cˉc=\bar{c} and the proof of (200) with c=uc=u. ∎

By the same method, we can evaluate E⁡n−1,β(F^n−1,β(x1,…,xn−1;u))\operatorname{E}_{n-1,\beta}(\hat{F}_{n-1,\beta}(x_{1},\dots,x_{n-1};u)) where F^n−1,β\hat{F}_{n-1,\beta} is defined in (71).

We consider (−∞,cˉ)n−1(-\infty,\bar{c})^{n-1} as a probability space with the probability measure

where dμn−1,β(x1,…,xn−1)d\mu_{n-1,\beta}(x_{1},\dots,x_{n-1}) is defined in (38). Let Sn−1,βwS^{w}_{n-1,\beta} be a random variable on (−∞,cˉ)n−1(-\infty,\bar{c})^{n-1} such that

where the range of the argument is taken to be (−π,π](-\pi,\pi].

for any v>ev>\mathbf{e}. For ww given in (46), we will show

Assuming (216) and (217), we find that Sn−1,βwS^{w}_{n-1,\beta} converges in probability to −βt2∫dμ(x)u−x-\frac{\beta t}{2}\int\frac{d\mu(x)}{u-x}, and (198) is proved. Assuming (218) and (219), we find that Sn−1,βw+βt2n∫dμ(x)w0−xS^{w}_{n-1,\beta}+\frac{\beta t}{2}\sqrt{n}\int\frac{d\mu(x)}{w_{0}-x} converges in probability to , and (202) is proved.

To prove (216), we denote for x<cˉx<\bar{c} the function

gβ(x;w)g_{\beta}(x;w) depends on nn, but we suppress that dependence to economize on notation. Let ww be given by (46), uniformly for all x<cˉx<\bar{c}

where we use (201) in the last line. Using the Cauchy-Schwartz inequality, we find (for notational simplicity, we write Gr,β(x1,…,xn−1;u,w;cˉ)G_{r,\beta}(x_{1},\dots,x_{n-1};u,w;\bar{c}) as Gr,βG_{r,\beta} if there is no confusion)

Hence log⁡E⁡n−1,β(Gr,β(x1,…,xn−1;u,w;cˉ))\log\operatorname{E}_{n-1,\beta}(G_{r,\beta}(x_{1},\dots,x_{n-1};u,w;\bar{c})) is a convex function in rr. For any ϵ>0\epsilon>0, by (224)

Taking ϵ→0\epsilon\to 0, by (225), (227) and (221) we have

To prove (217), we consider the moment-generating function of n(Sn−1,βw−E⁡(Sn−1,βw))n(S^{w}_{n-1,\beta}-\operatorname{E}(S^{w}_{n-1,\beta})). By (223) we have

where in the last step we use (221). The convergence of moment-generating function (231) implies (217).

To prove (218), we denote for x<cˉx<\bar{c} the function

To prove (219), we consider the moment-generating function of n(Sn−1,βw−E⁡(Sn−1,βw))\sqrt{n}(S^{w}_{n-1,\beta}-\operatorname{E}(S^{w}_{n-1,\beta})). Like (230) and (231), we have the convergence of moment-generating function

The author thanks Mark Adler, Jinho Baik, Kenneth D. T-R McLaughlin and Peter J. Forrester for helpful comments, and anonymous referees for careful reading and valuable suggestions on presentation.

The goal of this appendix is two-fold. We prove Proposition 2.2 and also propose the definition of the β\beta-external source model.

The strategy in this appendix has appeared in [25, Appendix] independently for the purpose of proof of [25, Theorem 1]. Since we are concerned with β=1,2,4\beta=1,2,4 cases and furthermore all β>0\beta>0, we give full detail in this appendix.

By change of variables and calculation of Jacobian (cf. [24, Chapter 3]), it follows from (1), (2) and (9) that the joint p.d.f.s of the eigenvalues λ1,…,λn\lambda_{1},\dots,\lambda_{n} of MM in the three β\beta-external source models (β=1,2,4\beta=1,2,4) are given by

Recall that in combinatorics, a partition κ=(κ1,κ2,… )\kappa=(\kappa_{1},\kappa_{2},\dots) is a sequence of non-negative integers in decreasing order, and containing only finitely many non-zero terms. We denote l(κ)l(\kappa) as the number of non-zero terms of κ\kappa, and write κ⊢k\kappa\vdash k if ∑i=1l(κ)κi=k\sum^{l(\kappa)}_{i=1}\kappa_{i}=k.

Jack polynomials Cκ(α)(x1,…,xn)C^{(\alpha)}_{\kappa}(x_{1},\dots,x_{n}) are nn-variable symmetric polynomials indexed by partition κ\kappa and the parameter α\alpha. For general references of Jack polynomials, see and . In this paper, we take the “C”-normalization of Jack polynomials , such that

The Jack polynomials with parameters 2,1,122,1,\frac{1}{2} are Zonal spherical functions. See [23, Chapter VII]. Cκ(2)C^{(2)}_{\kappa} are the well known Zonal polynomial in statistics , Cκ(1)C^{(1)}_{\kappa} are the complex Zonal polynomials, and are better known as Schur polynomials, and Cκ(1/2)C^{(1/2)}_{\kappa} are the quaternionic Zonal polynomials.

The integral in (237) can be expanded in Jack polynomials:

Let β=1,2,4\beta=1,2,4 and Gβ(n)G_{\beta}(n) be O(n)O(n), U(n)U(n) and Sp(n)Sp(n) respectively. If An,β\mathbf{A}_{n,\beta} is defined by (4), (6) and (10) and Λn\Lambda_{n} is defined by (238), then

where An=2βAn,β=diag⁡(a1,…,an)\mathbf{A}_{n}=\frac{2}{\beta}\mathbf{A}_{n,\beta}=\operatorname{diag}(a_{1},\dots,a_{n}) as defined in (4). Furthermore, by general theory of Zonal spherical functions (e.g. [20, Proposition 5.5])

After expanding enℜTr⁡(An,βQΛnQ−1)e^{n\Re\operatorname{Tr}(\mathbf{A}_{n,\beta}Q\Lambda_{n}Q^{-1})} into power series of ℜTr⁡(An,βQΛn,βQ−1)\Re\operatorname{Tr}(\mathbf{A}_{n,\beta}Q\Lambda_{n,\beta}Q^{-1}), we prove (240) by (242) and (243). ∎

In case that An=diag⁡(a,0,…,0)\mathbf{A}_{n}=\operatorname{diag}(a,0,\dots,0), (240) is much simplified by the property of Jack polynomials:

[31, Proposition 2.5] If the number of nonzero variables among a1,…,ana_{1},\dots,a_{n} is less than l(κ)l(\kappa), then Cκ(α)(a1,…,an)=0C^{(\alpha)}_{\kappa}(a_{1},\dots,a_{n})=0 for any α>0\alpha>0.

Therefore, in the case An=diag⁡(a,0,…,0)\mathbf{A}_{n}=\operatorname{diag}(a,0,\dots,0),

C(k)(2/β)(a,0,…,0)C^{(2/\beta)}_{(k)}(a,0,\dots,0) and C(k)(2/β)(1,…,1)C^{(2/\beta)}_{(k)}(1,\dots,1) can be calculated explicitly [16, Table 5]

By [31, Proposition 2.1] and the conversion between the “J”-normalization and “C”-normalization [16, Table 6], we have the identity of formal series in aa

Hence we obtain by Cauchy’s integral formula and (245)

where the contour is taken to be a small circle around such that all λj−1\lambda^{-1}_{j} (j=1,…,nj=1,\dots,n) are in the exterior of the contour. By (245) and (248), we obtain

Note that (249) is valid for all β>0\beta>0.

Suppose β\beta is a positive number. Let mm be an integer and ξ∈(0,1]\xi\in(0,1], such that

where the contour is large enough so that all λj\lambda_{j} are in its interior, and is in its interior if ξ≠1\xi\neq 1. Here

is the Pochhammer symbol (“rising factorial”), and

is the Kummer’s (confluent hypergeometric) function. See [1, 13.1.2]. Alternatively, for ξ≠1\xi\neq 1

where γ(s,z)\gamma(s,z) is the incomplete gamma function (cf. [1, 6.5.12]), and for ξ=1\xi=1

We note that in the cases β=2,4\beta=2,4, or in the case that β=1\beta=1 and nn is even, ξ=1\xi=1 and m=β2n−1m=\frac{\beta}{2}n-1. Thus by (237), (244), (249) and (251), we have

where Cˉn,β\bar{C}_{n,\beta} is a constant, and the contour encloses all λj\lambda_{j} in its interior.

If a>0a>0 and max⁡1≤j≤nλj≤u\max_{1\leq j\leq n}\lambda_{j}\leq u, the contour in (256) can be taken as Σs1,s2z\Sigma^{z}_{s_{1},s_{2}} defined in (51) or Πsz\Pi^{z}_{s} defined in (52), where z>uz>u. From the joint p.d.f. of λj\lambda_{j}, it is straightforward to find the p.d.f. formula (56) of the largest eigenvalue ξmax⁡(n)\xi_{\max}{(n)}. Thus Proposition 2.2 is proved.

If β=1\beta=1 and nn is odd, similarly we obtain that the joint p.d.f. of The eigenvalues in nn-dimensional 11-external source model is

In Section 2 we compute the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} based on (256). Since the asymptotic property of M(1,12,z)M(1,\frac{1}{2},z) is similar to that of ez=M(1,1,z)e^{z}=M(1,1,z) for large zz, we can compute the limiting distribution of ξmax⁡(n)\xi_{\max}{(n)} based on (259) by the same method that we use in Section 2. Hence we can prove that Theorems 1.1, 1.2, 1.3 and 1.4 hold when β=1\beta=1 and nn is odd.

Inspired by the Coulomb gas interpretation of the distribution of eigenvalues in random matrix models (see ), we generalize the β\beta-external source model to any β>0\beta>0 as the probability distribution of nn points on the real line, such that

where VV is the potential and a1,…,ana_{1},\dots,a_{n} are external source parameters. By (237) and (240), (258) gives the distribution of eigenvalues of the random matrix models with external source with β=1,2,4\beta=1,2,4. But for other value of β\beta, it has no matrix interpretation. By Proposition A.2, (245) (247) and (251), we find that if one external source parameter is aa and all others are , the distribution of the right-most point in the general β\beta-external source model is

where ξ\xi is defined by (250). It is of interest to compare this formula with the rank 11 spiked Gaussian and Laguerre β\beta ensembles studied in . In the very recent preprint , Forrester obtained similar formulas for β\beta-Wishart ensembles.

where CC is a constant independent of uu, and, if J=[b1,b2]J=[b_{1},b_{2}],

To make the notations simpler, we assume J=J= in the proof of (260). The generalization to arbitrary JJ is straightforward.

From formula (83), (192) and (188), we have that

The right-hand side of (262) is divided into the product of three terms. The first one is a constant, and we compute the other two terms below.

First we compute the third term in (262). Exchanging the order of integration, we have

To evaluate F(u,s)F(u,s), we note (with the change of variable x=sin⁡θx=\sin\theta)

and it implies that F(u,s)→0F(u,s)\to 0 as u→∞u\to\infty. Thus from (265) and (266)

Next we compute the second term in (262). For the equilibrium measure dμ(x)=Ψ(x)dxd\mu(x)=\Psi(x)dx on its support $$, By [15, Formula 6.135], we have

Thus by (271), (272) and exchanging the order of integration,

Thus by (276), (277), (278) and the identity

By the property [15, Formulas 6.143 and 6.144]

we further simplify the second factor on the right-hand of (262) as

Substituting (270) and (283) into (262), we obtain

and prove (260) in the case that J=J=. The general case can be proved by a simple rescaling.

References