The rank 1 real Wishart spiked model

M. Y. Mo

Introduction

In many of these applications, one has to deal with data in which both NN and MM are large, while the ratio M/NM/N is finite and non-zero. In this case, the sample covariance matrix YY becomes a poor approximation for the covariance matrix Σ\Sigma. However, since it is often reasonable to approximate the data by NN-variate gaussian random variables, a comparison between the eigenvalue distribution of the sample covariance matrix and Wishart matrices with a known covariance matrix will give a good estimate for the spectrum of the true covariance matrix Σ\Sigma. In particular, in applications to principle component analysis, one would like to study the asymptotic behavior of the largest eigenvalue of YY as NN, M→∞M\rightarrow\infty with M/N→γ2≥1M/N\rightarrow\gamma^{2}\geq 1 fixed.

For many statistical data with large NN and MM and M/NM/N finite, it was noted in that the eigenvalue distribution of the sample covariance matrix is well-approximated by the Marchenko-Pastur law inside a bulk region (See ,, , , .)

where χ[b−,b+]\chi_{[b_{-},b_{+}]} is the characteristic function for the interval [b−,b+][b_{-},b_{+}] and b±=(1±γ−1)2b_{\pm}=(1\pm\gamma^{-1})^{2}. However, outside of the bulk region, there are often a finite number of large eigenvalues at isolated locations. This behavior prompted the introduction of spiked models in , which are Wishart matrices with a covariance matrix Σ\Sigma such that only finitely many eigenvalues of Σ\Sigma are different from one. These non-trivial eigenvalues in Σ\Sigma will then be responsible for the spikes that appear in the eigenvalue distribution of the sample covariance matrix . The number of these non-trivial eigenvalues in Σ\Sigma is called the rank of the spiked model.

Of particular interest is a phase transition that arises in the largest eigenvalue distributions when the first of these spikes starts leaving the bulk region. This phenomenon was first studied in for the complex Wishart spiked model and then in for the rank 1 quarternionic Wishart spiked model. Let 1+τ1+\tau be the non-trivial eigenvalue in Σ\Sigma, in both cases, it was shown that the phase transition in the largest eigenvalue distribution occurs when τ=γ−1\tau=\gamma^{-1}. Their results are expressed in terms of the Hastings-McLeod solution of the Painlevé II equation, which is the unique solution to the Painlevé II equation

In particular, they have proved the following.

For −1<τ≤γ−1-1<\tau\leq\gamma^{-1}, the largest eigenvalue distribution is given by

where TWβ(ζ)TW_{\beta}(\zeta) is the Tracy-Widom distribution.

where erf(ζ)erf(\zeta) is the error function.

The functions TWβTW_{\beta} are called the Tracy-Widom distributions in the literature and they give the largest eigenvalue distributions for the real (β=1\beta=1), complex (β=2\beta=2) and quarternionic (β=4\beta=4) Wishart ensembles with Σ=I\Sigma=I, as well as the largest eigenvalue distributions for a large class of random matrix models.

Note that in , the phase transition was in fact computed for spiked models of any finite rank. These previous results naturally divides the range of the non-trivial eigenvalue 1+τ1+\tau into 3 regimes, which are illustrated in Figure 1.

The subcritical regime: When −1<τ<γ−1-1<\tau<\gamma^{-1}, the perturbation in Σ\Sigma is not strong enough to form a spike in the eigenvalue distribution of YY and the largest eigenvalue distribution in the Wishart matrix is not affected by this non-trivial eigenvalue. For real Wishart ensembles, this case was studied in and it was shown that the largest eigenvalue distribution remains the same as the case when Σ=I\Sigma=I. The result of also applies to much more general sample covariance matrices that are not necessarily Gaussian.

The critical regime: When 1−γ−1τ=O(M−13)1-\gamma^{-1}\tau=O\left(M^{-\frac{1}{3}}\right), the perturbation is just strong enough to form a spike and a phase transition occurs in the largest eigenvalue distribution. The result in for the complex phase transition in fact extends to the whole regime where the authors showed that the largest eigenvalue distribution is described by a function F2(ζ,w)F_{2}(\zeta,w) which equals TW12(ζ)TW_{1}^{2}(\zeta) when w=0w=0. The critical regime for the real case is the subject of this paper. It was also studied recently in using a completely different approach.

The super-critical regime: When τ>1\tau>1, the perturbation in Σ\Sigma is strong enough to form a spike and the largest eigenvalue is located at the spike instead of the edge of the bulk region. For rank 1 real Wishart spiked model, this was studied in . The results in has also been generalized to a large class of rank 1 spiked perturbed random matrix models in .

Despite having the most applications, the phase transition for real Wishart spiked model has not been solved until very recently . The main goal of this paper is to obtain the asymptotic largest eigenvalue distribution for the rank 1 real Wishart spiked model in the critical regime. In a recent paper , the asymptotic largest eigenvalue distribution for the rank 1 real Wishart ensemble was obtained by using a completely different approach to ours. In , the authors first use the Housefolder algorithm to reduce a Wishart matrix into tridiagonal form. Such tridiagonal matrix is then treated as a discrete random Schrödinger operator and by taking an appropriate scaling limit, the authors obtained a continuous random Schrödinger operator on the half-line. By doing so, the authors in bypass the problem of determining the eigenvalue j.p.d.f. for the real Wishart ensemble and obtain the largest eigenvalue distribution in the asymptotic limit. In , the largest eigenvalue distribution is characterized in several different ways, one of which is the solution of a PDE.

(Theorem 1.7 of ) Let w=(N(1+γ−1)2)13(1−γτ)∈(−∞,∞)w=\left(\frac{N}{(1+\gamma^{-1})^{2}}\right)^{\frac{1}{3}}(1-\gamma\tau)\in(-\infty,\infty), then the following boundary value problem

has a unique solution Fβ(ζ,w)F_{\beta}(\zeta,w) and

where β=1\beta=1, 22 and 44 for the real, complex and quarternionic Wishart ensembles respectively.

The distribution also has another characterization which requires more set up to explain. We will refer the readers to for more details. The above result in in fact also extends to the spiked perturbations of Gaussian ensembles in random matrix theory and to their general β\beta analogues, which are defined in .

On the other hand, the approach in this paper uses orthogonal polynomial techniques that are closer to those in and and we obtain a characterization of the largest eigenvalue distribution in the critical regime in terms of Painlevé transcendents. It will be very interesting see how these two representations of the largest eigenvalue distribution can be converted into one another. We will now state our results and outline the method used in the paper.

Statement of result

We will now explain the approach used in this paper.

Let λj\lambda_{j} be the eigenvalues of the Wishart matrix, then the j.p.d.f. for the real Wishart ensemble is given by

where gTdgg^{T}dg is the Haar measure on O(N)O(N) and ZM,NZ_{M,N} is a normalization constant. The j.p.d.f. for complex and quarternionic Wishart ensembles are similar

A major difficulty in the asymptotic analysis of the real Wishart ensembles is to find a simple expression for the j.p.d.f. in terms of its eigenvalues. For complex Wishart ensembles, the integral over U(N)U(N) in the expression of the j.p.d.f. can be evaluated using the Harish-Chandra Itzykson Zuber formula to obtain a compact determinantal formula for the j.p.d.f. in terms of the eigenvalues λj\lambda_{j}. This has led to the results in and results on the largest eigenvalue distributions for more general complex Wishart ensembles , . In the quarternonic case, although the Harish-Chandra and Itzykson Zuber formula does not apply, the integral over Sp(N)Sp(N) in the j.p.d.f. can still be evaluated using Zonal polynomial expansion to obtain a determinantal formula for the j.p.d.f. in the rank 1 case . In the real case, however, neither of these methods apply and so far there has not been any simple formula for the j.p.d.f. that allows the asymptotic analysis in the real case. Our first result is a contour integral formula that would allow the asymptotic analysis of the rank 1 real Wishart spiked model.

Assuming NN is even. Let the non-trivial eigenvalue in the covariance matrix Σ\Sigma be 1+τ1+\tau and suppose τ≠0\tau\neq 0. Then the j.p.d.f. of the eigenvalues in the rank 1 real Wishart spiked model with covariance matrix Σ\Sigma is given by

We will present two different proofs of this in the paper. The first one is a geometric proof which involves choosing a suitable set of coordinates on O(N)O(N) and decompose the Haar measure into two parts so that the integral in (2.1) can be evaluated. This will be achieved in Sections 3.1 and 3.2. The second proof is an algebraic proof that uses the Zonal polynomial expansion to verify the formula in Theorem 2.1. This proof will be given in Appendix A where integral formulae of the form (2.2) for the complex and quarternionic Wishart ensembles will also be derived.

The integral formula derived here is very similar to a more general formula in , in which the matrix integral over O(N)O(N) is given by

Shortly after the first part of this paper, which contains (2.2) appeared in the preprint server ArXiv, we learnt that D. Wang has also derived (2.2) independently and use it for the asymptotic analysis in the super-critical regime .

From the expression of the j.p.d.f., we see that the largest eigenvalue distribution is given by

and Γ\Gamma is a close contour that encloses the interval [0,z][0,z].

We can analyze the integrand as in , , and . By an identity of Brujin , we can express the multiple integral as a Pfaffian.

where rj(x)r_{j}(x) is an arbitrary sequence of degree jj monic polynomials and <f,g>1\left<f,g\right>_{1} is the skew product

where χ=χ[z,∞)\chi=\chi_{[z,\infty)} and KK is the operator whose kernel is given by

and S1(x,y)S_{1}(x,y) and IS1(x,y)IS_{1}(x,y) are the kernels

Then we can write these down in terms of Laguerre polynomials.

Let LkL_{k} be the degree kk monic Laguerre polynomial with respect to the weight w0(x)w_{0}(x)

If <L2k−1,L2k−2>1≠0\left<L_{2k-1},L_{2k-2}\right>_{1}\neq 0, then the skew orthogonal polynomials π2k,1\pi_{2k,1} and π2k+1,1\pi_{2k+1,1} both exist and π2k,1\pi_{2k,1} is unique while π2k+1,1\pi_{2k+1,1} is unique up to an addition of a multiple of π2k,1\pi_{2k,1}. Moreover, we have <L2k,L2k−1>1=0\left<L_{2k},L_{2k-1}\right>_{1}=0 and the skew orthogonal polynomials are given by

Next, by representing skew orthogonal polynomials as multi-orthogonal polynomials and write them in terms of the solution of a Riemann-Hilbert problem as in , we can apply the results of and to express the kernel S1(x,y)S_{1}(x,y) as a finite rank perturbation of the Christoffel Darboux kernel of the Laguerre polynomials.

Suppose <LN−1,LN−2>1<LN−3,LN−4>1≠0\left<L_{N-1},L_{N-2}\right>_{1}\left<L_{N-3},L_{N-4}\right>_{1}\neq 0. Let S1(x,y)S_{1}(x,y) be defined by (2.8) and choose the sequence of monic polynomials rj(x)r_{j}(x) such that rj(x)r_{j}(x) are arbitrary degree jj monic polynomials that are independent on tt and rj(x)=πj,1(x)r_{j}(x)=\pi_{j,1}(x) for j=N−2,N−1j=N-2,N-1. Then we have

where K2(x,y)K_{2}(x,y) is the kernel of the Laguerre polynomials

The largest eigenvalue distribution of the rank 1 real Wishart ensemble can be written in the following integral form.

for some constant c0c_{0} and KK is the operator with kernel given by (2.8). The integration contour Γ\Gamma is a close contour that encloses the interval [0,z][0,z] in the anti-clockwise direction.

These results so far are valid for all NN and MM and are exact. As NN, M→∞M\rightarrow\infty, the integral expression (2.13) can be used for the asymptotic analysis to obtain the largest eigenvalue distribution when the phase transition occur. In this paper, we will demonstrate the asymptotic analysis for the case where M/N→γ2=1M/N\rightarrow\gamma^{2}=1, but the analysis can also be applied to the case of any finite γ\gamma.

In the asymptotic limit, the tt integral in (2.13) can be computed using steepest descent analysis. In fact, we shall see that when t≠b+t\neq b_{+}, the integrand in (2.13) is of order

where ρ(s)\rho(s) is given in (1.1). The saddle point tsaddlet_{saddle} of this equation does not belong to the bulk region [b−,b+][b_{-},b_{+}] unless τ\tau is at the critical value τc=γ−1\tau_{c}=\gamma^{-1}. When τ<τc\tau<\tau_{c}, the steepest descent contour Γ\Gamma can be deformed such that it does not intersect [b−,b+][b_{-},b_{+}]. In this case, tt will always be of finite distance from [b−,b+][b_{-},b_{+}] and the factor (t−x)−12(t-x)^{-\frac{1}{2}} in w(x)w(x) will have no effect on the asymptotics of the kernel S1S_{1} at the edge point b+b_{+}. In this case, the kernel at the edge point will be given by the Airy kernel.

where ξ1=(x−b+)γM23(1+γ)43\xi_{1}=\left(x-b_{+}\right)\frac{\gamma M^{\frac{2}{3}}}{(1+\gamma)^{\frac{4}{3}}} and ξ2=(y−b+)γM23(1+γ)43\xi_{2}=\left(y-b_{+}\right)\frac{\gamma M^{\frac{2}{3}}}{(1+\gamma)^{\frac{4}{3}}} are finite.

In the critical case, however, the main contribution to the contour integral (2.13) comes from a small neighborhood of t=b+t=b_{+} and the factor (t−x)−12(t-x)^{-\frac{1}{2}} in w(x)w(x) will now significantly alter the behavior of the kernel S1S_{1} and change it from the Airy kernel to into a more complicated kernel. This gives rise to the phase transition and a new distribution function. Our next result is the representation of this new distribution function in terms of the Hastings-McLeod solution of the Painlevé II equation. First let us define some functions that will appear in our formula.

Let ψ(u,T)=(T−u)12\psi(u,T)=(T-u)^{\frac{1}{2}} and Hj(u,T)=Ai(j)(u)ψ−1(u,T)H_{j}(u,T)=Ai^{(j)}(u)\psi^{-1}(u,T) and let S10\mathcal{S}_{10}, S11\mathcal{S}_{11} be

Define the function S(T)\mathcal{S}(T) to be

where the contour of integration in the first term remains in the upper half plane and S11,±\mathcal{S}_{11,\pm} are the boundary values of S11\mathcal{S}_{11} as it approaches the real axis in the upper/lower half plane.

and define h⃗j\vec{h}_{j} to be the vector h⃗j=(0,0,0,ϕjψ)T\vec{h}_{j}=\left(0,0,0,\frac{\phi_{j}}{\psi}\right)^{T} for j=0,1,2j=0,1,2 and h⃗j=0\vec{h}_{j}=0 for j=3j=3 and j=4j=4, where ϕ0\phi_{0} is the Hastings-McLeod solution of Painlevé II (1.3) and

Let v⃗j\vec{v}_{j} be the vector that satisfies the linear system of ODEs with the following boundary condition

Then the largest eigenvalue distribution at the phase transition is given by

Suppose NN is even. Let w=(N4)13(1−τ)∈(−∞,∞)w=\left(\frac{N}{4}\right)^{\frac{1}{3}}(1-\tau)\in(-\infty,\infty) and let ζ=(z−4)(N/4)23\zeta=(z-4)\left(N/4\right)^{\frac{2}{3}}, then as N,M→∞N,M\rightarrow\infty such that M/N→γ2=1M/N\rightarrow\gamma^{2}=1, the largest eigenvalue distribution at the phase transition is given by

The distribution in Theorem 2.4 is expressed in terms of integrals of the Airy function, together with the functions vjkv_{jk}, which are solutions of linear ODEs with known boundary conditions. The coefficients of the ODEs satisfied by the vjkv_{jk} are given in terms of the Hastings-McLeod solutions and its derivatives and are therefore known functions.

The distribution in Theorem 2.4 can also be expressed in terms of an integral involving the solution of a Riemann-Hilbert problem. (see Appendix B) With the recent advancement in the numerical computation of Riemann-Hilbert problems , this representation may be useful for the numerical computation of the distribution in Theorem 2.4.

In obtaining the main result in Theorem 2.4, we have obtained some other results which may also be of interest to mathematicians and physicists working in random matrix theory.

One applications of the orthogonal polynomial approach developed in this paper is in the studies of random matrix with a rank 1 external source. Random matrix with external source are random matrix models on the space of real symmetric, Hermitian or Hermitian self-dual N×NN\times N matrices with the following probability measure

for some real-valued function V(x)V(x) such that e−V(x)e^{-V(x)} decays fast enough as x→±∞x\rightarrow\pm\infty and a real symmetric, Hermitian or Hermitian self-dual matrix AA. The function V(x)V(x) is usually called the potential while the matrix AA is known as the external source. The real Wishart ensemble can be thought of as a special case when V(x)=x2−M−N−12Mlog⁡xV(x)=\frac{x}{2}-\frac{M-N-1}{2M}\log x. Random matrices with external source are first studied by Brézin and Hikami , and P. Zinn-Justin , as a model of systems with both random and deterministic parts. For Hermitian random matrices, the external source model can be studied using multi-orthogonal polynomial and Riemann-Hilbert techniques and there are many recent advancements in the asymptotic analysis of Hermitian external source models with non-Gaussian potential V(x)V(x) , , , , , , . In , the contour integral formula (2.2) was derived independently and was used to study real symmetric random matrix with a rank 1 external source and a large class of potential V(x)V(x). By using the linear statistics results of Johansson and a representation for the largest eigenvalue distribution that is different to (2.13), the largest eigenvalue distribution was obtained in the super-critical regime. The orthogonal polynomial approach developed in this paper can be used to extend the results in to the critical regime. In fact, for real random matrix with a rank 1 external source, the expression (2.13) for the largest eigenvalue distribution remains valid, although the kernels S1S_{1} and KK will have to be modified according to the potential. For a polynomial potential V(x)V(x), the analogue of (2.10), which expresses the kernel S1S_{1} in terms of orthogonal polynomials is well-known . By using the asymptotics of orthogonal polynomials found in and , such representation can be used to compute the asymptotics of the kernel S1S_{1}, which can then be used in (2.13) to obtain the largest eigenvalue distribution.

1.2 Orthogonal ensembles

A large part of this paper involves the analysis of an orthogonal ensemble with weight (2.4) and in doing so, we have obtained some new results for orthogonal ensembles.

in the limit N→∞N\rightarrow\infty, where Zn,β(w)Z_{n,\beta}(w) is the partition functions of the ensembles (See remark 2.4 of and remark 1.5 of )

In order to proof the universality in orthogonal and symplectic ensembles using the method in , and , one needs to show that lim⁡N→∞det⁡Q≠0\lim_{N\rightarrow\infty}\det Q\neq 0. While the leading order asymptotics of these partition functions can be found using the estimates in , their combined contributions to det⁡Q\det Q cancel in the leading order and hence higher order terms in the asymptotics of Zn,β(w)Z_{n,\beta}(w) are needed to show that lim⁡N→∞det⁡Q≠0\lim_{N\rightarrow\infty}\det Q\neq 0. At the moment, asymptotics for the sub-leading order terms of partition functions are only available for β=2\beta=2. By using a differential identity for log⁡ZN,2\log Z_{N,2}, the authors in computed the sub-leading order terms in ZN,2Z_{N,2} for the potential V(x)=x44+tx22V(x)=\frac{x^{4}}{4}+\frac{tx^{2}}{2} as N→∞N\rightarrow\infty. A combination of the method in and the differential identity (2.16) may provide a way to compute the sub-leading order terms in the partition function ZN,1Z_{N,1} and help extend the universality results in orthogonal and symplectic ensembles to more general potentials.

Another interesting observation is Corollary 4.1, in which we showed that <Lk,Lk−1>1=0\left<L_{k},L_{k-1}\right>_{1}=0 whenever kk is even. This turns out to be a very useful identity in the analysis of the phase transition when the double scaling limit t−4=T(4/N)23t-4=T\left(4/N\right)^{\frac{2}{3}} for the ensemble with weight (2.4) has to be considered. When analyzing this double scaling limit, the identity <Lk,Lk−1>1=0\left<L_{k},L_{k-1}\right>_{1}=0 leads to cancelation in the leading order terms of the kernel S1S_{1}. This enables us to show that S1S_{1} is of order N23N^{\frac{2}{3}} instead of N43N^{\frac{4}{3}}, which is essential for the scaled limit of the determinant det⁡2(I−χKχ)\det_{2}\left(I-\chi K\chi\right) to exist. We believe this type of identity will also be useful in the analysis of other double scaling limits in orthogonal ensembles.

Throughout the paper, we shall assume that NN is even and that M−N>0M-N>0.

Contour integral formula for the j.p.d.f.

In this section we will prove the integral formula for the j.p.d.f. in Theorem 2.1.

In this section, we will find a convenient set of coordinate on O(N)O(N) to evaluate the integral

that appears in the expression of the j.p.d.f. (2.1). As both Σ−1\Sigma^{-1} and YY are symmetric matrices, they can be diagonalized by matrices in O(N)O(N). We can therefore replace both Σ−1\Sigma^{-1} and YY by the diagonal matrices Σd−1\Sigma_{d}^{-1} and Λd\Lambda_{d}.

The group O(N)O(N) has two connected components, SO(N)SO(N) and O−(N)O_{-}(N) that consists of orthogonal matrices that have determinant 11 and −1-1 respectively. Let TT be the matrix

then the left multiplication by TT defines an diffeomorphism from O−(N)O_{-}(N) to SO(N)SO(N). In particular, we can write the integral over O(N)O(N) in (2.1) as

Note that gTdgg^{T}dg is also the Haar measure on SO(N)SO(N).

Let gijg_{ij} be the entries of g∈SO(N)g\in SO(N). Then the integral II can be written as

We will now find an expression of the Haar measure and use it to compute the integral I(Σ,Λ)I(\Sigma,\Lambda).

First let us define a set of coordinates on SO(N)SO(N) that is convenient for our purpose. We will then express the Haar measure on SO(N)SO(N) in terms of these coordinates.

An element g∈SO(n)g\in SO(n) can be written in the following form

In particular, the matrix VV with entries vijv_{ij} for 1≤i,j≤N−11\leq i,j\leq N-1 is in SO(N−1)SO(N-1). The following then gives a set of coordinates on SO(N)SO(N).

In the above equation, g⃗N\vec{g}_{N} is identified with the coordinates ϕj\phi_{j} in (3.2), while the matrix VV is identified with the coordinates in SO(N−1)SO(N-1) that correspond to VV. In terms of these coordinates, the left action of an element S∈SO(N)S\in SO(N) on gg is given by the following.

From the fact that G(Sg⃗N)SG(g⃗N)−1G(S\vec{g}_{N})SG(\vec{g}_{N})^{-1} is an orthogonal matrix, it is easy to check that s⃗=0\vec{s}=0 and sN=±1s_{N}=\pm 1. To determine sNs_{N}, let us consider the action of G(Sg⃗N)SG(g⃗N)−1G(S\vec{g}_{N})SG(\vec{g}_{N})^{-1} on (0,0,…,1)T(0,0,\ldots,1)^{T}. We have

We will now write the Haar measure on SO(N)SO(N) in terms of the coordinates (3.4). These coordinates give a local diffeomorphism between SO(N)SO(N) and SN−1×SO(N−1)S^{N-1}\times SO(N-1) as g⃗N∈SN−1\vec{g}_{N}\in S^{N-1} and V∈SO(N−1)V\in SO(N-1). Let dXdX be a measure on SN−1S^{N-1} that is invariant under the action of SO(N)SO(N) and VTdVV^{T}dV be the Haar measure on SO(N−1)SO(N-1), then the following measure

as dXdX is invariant under the action of SS. Therefore if we can find a measure on SN−1S^{N-1} that is invariant under the action of SO(N)SO(N), then dX∧VTdVdX\wedge V^{T}dV will give us a left invariant measure on SO(N)SO(N). Since the left invariant measure on a compact group is also right invariant, this will give us the Haar measure on SO(N)SO(N). As the metric on SN−1S^{N-1} is invariant under the action of SO(N)SO(N), it is clear that the volume form on SN−1S^{N-1} is invariant under the action of SO(N)SO(N). Let dXdX be the volume form on SN−1S^{N-1}, then from (3.7), we see that the measure dX∧VTdVdX\wedge V^{T}dV is invariant under the action of SO(N)SO(N).

Let dXdX be the volume form on SN−1S^{N-1} given by

in terms of the coordinates ϕ1,…,ϕN−1\phi_{1},\ldots,\phi_{N-1} in (3.2) and (3.4), then the Haar measure on SO(N)SO(N) is equal to a constant multiple of

where VTdVV^{T}dV is the Haar measure on SO(N−1)SO(N-1) in terms of the coordinates (3.4).

We can now compute the integral I(Σ,Λ)I(\Sigma,\Lambda).

2 Integral formula

By using the expression of the Haar measure derived in the last section, we can now write the integral I(Σ,Λ)I(\Sigma,\Lambda) as

for some constant CC, where the N−1N-1 sphere SN−1S^{N-1} in the above formula is defined by ∑j=1NgjN2=1\sum_{j=1}^{N}g_{jN}^{2}=1 and dXdX is the volume form on it. If we let gjN=xjg_{jN}=x_{j}, then the above can be written as

Therefore in terms of polar coordinates, we have

To compute the integral I(Σ,Λ)I(\Sigma,\Lambda), we use a method in the studies of random pure quantum systems (see, e.g. ). The idea is to consider the Laplace transform of the function I(Σ,Λ,t)I(\Sigma,\Lambda,t) defined by

then I(Σ,Λ,1)=I(Σ,Λ)I(\Sigma,\Lambda,1)=I(\Sigma,\Lambda). The Laplace transform of I(Σ,Λ,t)I(\Sigma,\Lambda,t) in the variable tt is given by

Taking the inverse Laplace transform, we obtain an integral expression for I(Σ,Λ)I(\Sigma,\Lambda).

where Γ\Gamma is a contour that encloses all the points τM2(1+τ)λ1,…,τM2(1+τ)λN\frac{\tau M}{2(1+\tau)}\lambda_{1},\ldots,\frac{\tau M}{2(1+\tau)}\lambda_{N} that is oriented in the counter-clockwise direction. Rescaling the variable ss to s=Mts=Mt, we obtain

This then give us an integral expression for the j.p.d.f. in Theorem 2.1.

In this section we will prove the representation of the kernel S1S_{1} in Theorem 2.2. We will do so by using the multi-orthogonal polynomial representation of skew orthogonal polynomials in and then apply the Christoffel-Darboux formula for multi-orthogonal polynomials in to write the kernel S1S_{1} as a finite sum of multi-orthogonal polynomials. We then simplify this sum further by using a result in . This gives a new proof to a well-known result of Widom .

As explain in the introduction, we need to find the skew orthogonal polynomials with the weight (2.4). Let us consider the skew orthogonal polynomials with respect to the weight ww in (2.4). We shall use the ideas in to express the skew orthogonal polynomials in terms of a linear combinations of Laguerre polynomials.

Let Qj(x)Q_{j}(x) to be the degree j+2j+2 polynomial

Then as we assume M−N>0M-N>0, it is easy to see that

Note that w0(x)w_{0}(x) is not the square of w(x)w(x). The fact that w0(x)w_{0}(x) is the weight for the Laguerre polynomials allows us to express the skew orthogonal polynomials for the weight (2.4) in terms of Laguerre polynomials.

In particular, this implies that the conditions (2.9) is equivalent to the following conditions

and the exactly same conditions for π2k+1,1(x)\pi_{2k+1,1}(x). In particular, the second condition implies the skew orthogonal polynomials can be written as

where Lj(x)L_{j}(x) are the degree jj monic Laguerre polynomials that are orthogonal with respect to the weight w0(x)w_{0}(x).

The constants γk,j\gamma_{k,j} are to be determined from the first condition in (4.3). We will now show that if <L2k−1,L2k−2>1≠0\left<L_{2k-1},L_{2k-2}\right>_{1}\neq 0, then the skew orthogonal polynomials π2k,1\pi_{2k,1} and π2k+1,1\pi_{2k+1,1} exist and that π2k,1\pi_{2k,1} is unique. First let us show that the first condition in (4.3) is equivalent to

To do this, we will first define a map ϱN\varrho_{N} from the span of L2k−1L_{2k-1} and L2k−2L_{2k-2} to the span of yy and 11.

Let P(x)P(x) be a polynomial of degree mm. Then we can write the polynomial P(x)P(x) as

where q(x)q(x) is a polynomial of degree m−2m-2 and R(x)R(x) is a polynomial of degree less than or equal to 1. By writing down the system of linear equations satisfied by the coefficients of q(x)q(x) and R(x)R(x), we see that the polynomials q(x)q(x) and R(x)R(x) are uniquely defined for any given P(x)P(x). In particular, the map f:P(x)↦R(x)f:P(x)\mapsto R(x) is a well-defined linear map from the space of polynomial to the space of polynomials of degrees less than or equal to 11. Let ϱk\varrho_{k} be the following restriction of this map.

For any polynomial P(x)P(x), let ff be the map that maps P(x)P(x) to R(x)R(x) in (4.5). Then the map ϱk\varrho_{k} is the restriction of ff to the linear subspace spanned by the orthogonal polynomials Lk,Lk−1L_{k},L_{k-1}.

If <Lk,Lk−1>1≠0\left<L_{k},L_{k-1}\right>_{1}\neq 0, then the map ϱk\varrho_{k} is invertible.

Suppose there is exists non-zero constants a1a_{1} and a2a_{2} such that

for some polynomial q(x)q(x) of degree k−2k-2, then by taking the skew product <>1\left<\right>_{1} of this polynomial with LkL_{k}, we obtain

As q(x)q(x) is of degree k−2k-2. Since <Lk−1,Lk>1≠0\left<L_{k-1},L_{k}\right>_{1}\neq 0, this shows that a2=0a_{2}=0. By taking the skew product with Lk−1L_{k-1}, we conclude that a1=0a_{1}=0 and hence the map ϱk\varrho_{k} has a trivial kernel. ∎

If kk is even, then <Lk,Lk−1>1=0\left<L_{k},L_{k-1}\right>_{1}=0.

Let q(x)q(x) be a polynomial of degree k−2k-2 that satisfies the following conditions

Assuming kk is even and let q(x)q(x) be a polynomial that satisfies (4.6). By taking the inner product <>2\left<\right>_{2} with xjx^{j}, we see that there exists non-zero constants a1a_{1} and a2a_{2} such that

Therefore by Lemma 4.1, we see that if kk is even, we will have <Lk,Lk−1>1=0\left<L_{k},L_{k-1}\right>_{1}=0. ∎

Lemma 4.1 shows that if <Li,Li−1>1≠0\left<L_{i},L_{i-1}\right>_{1}\neq 0, then there exist two independent polynomials R0(y)R_{0}(y) and R1(y)R_{1}(y) in the span of yy and 11 such that Rj(y)=ϱi(Li−j)R_{j}(y)=\varrho_{i}(L_{i-j}). Then we have

In particular, the skew product of Rj(y)R_{j}(y) with Li−lL_{i-l}, l<2l<2 is given by

As qjq_{j} is a polynomial of degree less than or equal to i−2i-2 and l<2l<2, the first term on the right hand side is zero. Therefore we have

We can now show that the skew orthogonal polynomials π2k,1\pi_{2k,1} and π2k+1,1\pi_{2k+1,1} exist if <L2k−1,L2k−2>1≠0\left<L_{2k-1},L_{2k-2}\right>_{1}\neq 0.

If <L2k−1,L2k−2>1≠0\left<L_{2k-1},L_{2k-2}\right>_{1}\neq 0, then the skew orthogonal polynomials π2k,1\pi_{2k,1} and π2k+1,1\pi_{2k+1,1} both exist and π2k,1\pi_{2k,1} is unique while π2k+1,1\pi_{2k+1,1} is unique up to an addition of a multiple of π2k,1\pi_{2k,1}. Moreover, we have <L2k,L2k−1>1=0\left<L_{2k},L_{2k-1}\right>_{1}=0 and the skew orthogonal polynomials are given by

for k≥2k\geq 2, where cc is an arbitrary constant.

Let π2k,1\pi_{2k,1} and π2k+1,1\pi_{2k+1,1} be polynomials defined by

for some constants γj,k\gamma_{j,k}. If we can show that <π2k−l,1,yj>1=0\left<\pi_{2k-l,1},y^{j}\right>_{1}=0 for j=0,1j=0,1 and l=−1,0l=-1,0, then π2k−l,1\pi_{2k-l,1} will be the skew orthogonal polynomial. Let R0R_{0} and R1R_{1} be the images of L2k−1L_{2k-1} and L2k−2L_{2k-2} under the map ϱ2k−1\varrho_{2k-1}. Then by the assumption in the Proposition, they are independent in the span of yy and 11. Therefore the conditions <π2k−l,1,yj>1=0\left<\pi_{2k-l,1},y^{j}\right>_{1}=0 are equivalent to <π2k−l,1,Rj(y)>1=0\left<\pi_{2k-l,1},R_{j}(y)\right>_{1}=0. By taking i=2k−1i=2k-1 in (4.7), we see that this is equivalent to <π2k−l,1,L2k−1−j>1=0\left<\pi_{2k-l,1},L_{2k-1-j}\right>_{1}=0. This implies

which exist and are unique as <L2k−1,L2k−2>1≠0\left<L_{2k-1},L_{2k-2}\right>_{1}\neq 0. This determines π2k,1\pi_{2k,1} uniquely. By Corollary 4.1, we have <L2k,L2k−1>1=0\left<L_{2k},L_{2k-1}\right>_{1}=0 and hence γ2k,2=0\gamma_{2k,2}=0. Similarly, the coefficients for π2k+1,1\pi_{2k+1,1} are

Again, these coefficients exist and are unique. However, as <π2k,1,π2k,1>1=0\left<\pi_{2k,1},\pi_{2k,1}\right>_{1}=0 and <π2k,1,yj>1=0\left<\pi_{2k,1},y^{j}\right>_{1}=0 for j=0,…,2k−1j=0,\ldots,2k-1, adding any multiple of π2k,1\pi_{2k,1} to π2k+1,1\pi_{2k+1,1} will not change the orthogonality conditions <π2k+1,1,yj>1=0\left<\pi_{2k+1,1},y^{j}\right>_{1}=0 that is satisfied by π2k+1,1\pi_{2k+1,1} and hence π2k+1,1\pi_{2k+1,1} is only determined up to the addition of a multiple of π2k,1\pi_{2k,1}. ∎

2 The Christoffel Darboux formula for the kernel

In , skew orthogonal polynomials were interpreted as multi-orthogonal polynomials and represented as the solution of a Riemann-Hilbert problem. This representation allows us to use the results in to derive a Christoffel-Darboux formula for the kernel (2.8) in terms of the Riemann-Hilbert problem.

Let us recall the definitions of multi-orthogonal polynomials. First let the weights w0w_{0}, w1w_{1} and w2w_{2} be

Note that the weights wl(x)w_{l}(x) are defined with the polynomials LN−3L_{N-3} and LN−4L_{N-4} instead of LN−1L_{N-1} and LN−2L_{N-2}. This is because the construction below involves the polynomial πN−2,1\pi_{N-2,1} as well as πN,1\pi_{N,1}. By taking i=N−3i=N-3 in (4.7), we see that the orthogonality conditions for πN,1\pi_{N,1} is also equivalent to

provided <LN−3,LN−4>1\left<L_{N-3},L_{N-4}\right>_{1} is also non-zero.

Then the multi-orthognoal polynomials of type II PN,lII(x)P^{II}_{N,l}(x), , , , are polynomials of degree N−1N-1 such that

More accurately, these are in fact the multi-orthogonal polynomials with indices (N−2,e⃗l)(N-2,\vec{e}_{l}), where e⃗1=(0,1)\vec{e}_{1}=(0,1) and e⃗2=(1,0)\vec{e}_{2}=(1,0).

We will now define the multi-orthogonal polynomials of type I. Let PN,lI(x)P^{I}_{N,l}(x) be a function of the following form

where BN,l(x)B_{N,l}(x) is a polynomial of degree N−3N-3 and AN,k,lA_{N,k,l} is independent on xx. Moreover, let PN,lI(x)P^{I}_{N,l}(x) satisfy

Then the polynomials BN,l(x)B_{N,l}(x) and δklx+AN,k,l\delta_{kl}x+A_{N,k,l} are multi-orthogonal polynomials of type I with indices (N,2,1)(N,2,1) for l=1l=1 and (N,1,2)(N,1,2) for l=2l=2. We will now show that PN,1IIP^{II}_{N,1} and PN,2IIP^{II}_{N,2} exist and are unique if both <LN−1,LN−2>1\left<L_{N-1},L_{N-2}\right>_{1} and <LN−3,LN−4>1\left<L_{N-3},L_{N-4}\right>_{1} are non-zero.

Suppose both <LN−1,LN−2>1\left<L_{N-1},L_{N-2}\right>_{1} and <LN−3,LN−4>1\left<L_{N-3},L_{N-4}\right>_{1} are non-zero, then the polynomials PN,1IIP^{II}_{N,1} and PN,2IIP^{II}_{N,2} exist and are unique.

Then by the first condition in (4.9), we see that

As the matrix with entries cijc_{ij} is invertible, we see that the linear equations (4.11) has a unique solution in the linear span of LN−1L_{N-1} and LN−2L_{N-2} if and only if <LN−1,LN−2>1≠0\left<L_{N-1},L_{N-2}\right>_{1}\neq 0. ∎

As we shall see, existence and uniqueness of PN,lIIP^{II}_{N,l} would imply that the multi-orthogonal polynomials of type I also exist and are unique. As in , the multi-orthogonal polynomial together with the skew orthogonal polynomials form the solution of a Riemann-Hilbert problem. Let Y(x)Y(x) be the matrix

Then by using the orthogonality conditions of skew orthogonal polynomials and multi-orthogonal polynomials, together with the jump discontinuity of the Cauchy transform, one can check that Y(x)Y(x) satisfies the following Riemann-Hilbert problem.

Similarly, multi-orthogonal polynomials of type I can also be arranged to satisfy a Riemann-Hilbert problem. Let ϵ\epsilon be the operator

First note that the functions ψj(x)=ϵ(πj,1w)\psi_{j}(x)=\epsilon(\pi_{j,1}w) for j≥2j\geq 2 can be express in the form of (4.10). By Lemma 4.1, we can write πj,1(x)\pi_{j,1}(x) as

where Bj(x)B_{j}(x) is a polynomial of degree j−2j-2.

Let X(z)X(z) be the matrix value function defined by

Then by using the orthogonality and the the jump discontinuity of the Cauchy transform, it is easy to check that X−T(z)X^{-T}(z) and Y(z)Y(z) satisfy the same Riemann-Hilbert problem and hence the multi-orthogonal polynomials of type I also exist and are unique.

We will now show that the kernel S1(x,y)S_{1}(x,y) given by (2.8) can be expressed in terms of the matrix Y(z)Y(z).

Suppose <LN−3,LN−4>1<LN−1,LN−2>1≠0\left<L_{N-3},L_{N-4}\right>_{1}\left<L_{N-1},L_{N-2}\right>_{1}\neq 0 and let the kernel S1(x,y)S_{1}(x,y) be

Then the kernel S1(x,y)S_{1}(x,y) exists and is equal to

As in , let us now expand the functions xrj(x)xr_{j}(x) and xϵ(rjw)x\epsilon(r_{j}w).

Then the coefficients cjkc_{jk} and djkd_{jk} for j,k=0,…,N−1j,k=0,\ldots,N-1 are given by

Therefore if we let C\mathcal{C} be the matrix with entries cjkc_{jk}, j,k=0,…N−1j,k=0,\ldots N-1 and D\mathcal{D} be the matrix with entries djkd_{jk} for j,k=0,…N−1j,k=0,\ldots N-1, then we have

where r(x)r(x) is the column vector with components rk(x)r_{k}(x). Now by (4.24), we see that

which are equal as μT=−μ\mu^{T}=-\mu. Now from the form of μ\mu in (4.22), we see that μN−1,j=δj,N−2hN−1,1−1\mu_{N-1,j}=\delta_{j,N-2}h_{N-1,1}^{-1}. Hence we have

Let us now consider the second term in (4.25). As in (4.17) we can write ϵ(rkw)w\epsilon(r_{k}w)w as

where qk(x)q_{k}(x) is of degree k−2k-2. Then from the form of PN,jIP_{N,j}^{I} in (4.10) and the orthogonality condition (4.9), we see that the coefficients dk,N+ld_{k,N+l}, l=1,2l=1,2 are given by

For k≠N−1k\neq N-1, the polynomial qkq_{k} is of degree less than or equal to N−4N-4, while for k=N−1k=N-1, BNB_{N} in (4.17) is a polynomial of degree N−2N-2 and hence the coefficient dk,Nd_{k,N} is zero unless k=N−1k=N-1. For k=N−1k=N-1, it is given by the leading coefficient of qN−1q_{N-1} divided by the leading coefficient of BNB_{N}. Since

we see that both the leading coefficient of qN−1(x)q_{N-1}(x) and BNB_{N} is 2M\frac{2}{M}. Hence dk,Nd_{k,N} is δk,N−1\delta_{k,N-1}. This gives us

To express the second term in (4.25) in terms of the multi-orthogonal polynomials, let us now express PN,lIIP^{II}_{N,l} in terms of the polynomials rkr_{k}. Let us write PN,lII=∑j=0N−1ajrj(x)P^{II}_{N,l}=\sum_{j=0}^{N-1}a_{j}r_{j}(x). Then we have

Hence PN,lII(x)P^{II}_{N,l}(x) can be written as

Therefore the second term in (4.25) is given by

By using the fact that Y−1(y)=XT(y)Y^{-1}(y)=X^{T}(y) and the expressions of the matrix YY (4.12) and XX (4.18), together with (4.13), we see that this is the same as (4.21). ∎

3 The kernel in terms of Laguerre polynomials

We will now use a result in to further simplify the expression of the kernel S1(x,y)S_{1}(x,y) so that its asymptotics can be computed using the asymptotics of Laguerre polynomials. Let us recall the set up in . First let Y(x)Y(x) be a matrix satisfying the Riemann-Hilbert problem

and let K1(x,y)\mathcal{K}_{1}(x,y) be the kernel given by

Let πj,2(x)\pi_{j,2}(x) be the monic orthogonal polynomials with respect to the weight w0(x)w_{0}(x). Let K0(x,y)\mathcal{K}_{0}(x,y) be the following kernel.

We can now apply Proposition 4.3 to our case. In our case, the vectors π(z)\pi(z) and v(z)v(z) are given by

while the matrix W\mathcal{W} is given by

By corollary 4.1, we see that <LN−2,LN−3>1=0\left<L_{N-2},L_{N-3}\right>_{1}=0 and hence the determinant of W\mathcal{W} is

Suppose det⁡W≠0\det\mathcal{W}\neq 0 and that the multi-orthogonal polynomials PN,lIIP^{II}_{N,l} exist. Let us now consider the vector u(z)u(z). By the Christoffel-Darboux formula, we have

where hj,0=<Lj,Lj>2h_{j,0}=\left<L_{j},L_{j}\right>_{2}. We shall show that LN−3L_{N-3} and LN−4L_{N-4} can be written in the following form

for some polynomial ql(x)q_{l}(x) of degree N−1N-1. By Lemma 4.1, we see that if <LN−3,LN−4>1≠0\left<L_{N-3},L_{N-4}\right>_{1}\neq 0, then the map ϱN−3\varrho_{N-3} in Definition 4.1 is invertible. Therefore if the restriction of the map ff in Definition 4.1 is also invertible on the span of πN+1,1\pi_{N+1,1} and πN,1\pi_{N,1}, we will be able to write LN−3L_{N-3} and LN−4L_{N-4} in the form of (4.31).

Let ff be the map in Definition 4.1 and let ϱπ\varrho_{\pi} be its restriction to the span of πN+1,1\pi_{N+1,1} and πN,1\pi_{N,1}. Then ϱπ\varrho_{\pi} is invertible.

Suppose there exist a1a_{1} and a2a_{2} such that

for some polynomial q(x)q(x) of degree at most N−1N-1. Then we have

As the degree of q(x)q(x) is at most N−1N-1, this is only possible if q(x)=0q(x)=0. ∎

The composition of ϱN−3\varrho_{N-3} and ϱπ−1\varrho_{\pi}^{-1} will therefore give us a representation of LN−3L_{N-3} and LN−4L_{N-4} in the form of (4.31). By using this representation and the fact that ql(x)q_{l}(x) is of degree at most N−1N-1, we see that

where QQ is the matrix with entries Qi,jQ_{i,j}. We will now determine the constants Qi,jQ_{i,j}.

Let πN,1\pi_{N,1} and πN+1,1\pi_{N+1,1} be the monic skew orthogonal polynomial with respect to the weight w(x)w(x) and choose πN+1,1\pi_{N+1,1} so that the constant cc in (4.8) is zero. Then the vector u(y)u(y) in (4.30) is given by

where QQ is the matrix whose entries Qi,jQ_{i,j} are given by

First let us compute the leading order coefficients of the polynomial ql(x)q_{l}(x) in (4.31). Let ql(x)=ql,N−1xN−1+ql,N−2xN−2+O(xN−3)q_{l}(x)=q_{l,N-1}x^{N-1}+q_{l,N-2}x^{N-2}+O(x^{N-3}), then we have

On the other hand, by orthogonality, we have

Let us now compute Qi,2Q_{i,2}. By taking the skew product, we have

By using the expansion (4.8) of the skew orthogonal polynomials in terms of LN−kL_{N-k}, we have

By substituting (4.36) into this, we obtain

Note that the matrix det⁡(QW−1)=M2/(4hN−1,0hN−2,0)\det(Q\mathcal{W}^{-1})=M^{2}/(4h_{N-1,0}h_{N-2,0}) and hence QW−1Q\mathcal{W}^{-1} is invertible. From Lemma 4.4 and (4.30), we obtain Theorem 2.2.

We will now further simplify the expression for the correlation kernel S1(x,y)S_{1}(x,y). First we make the following observation. From the definition (4.19) of the kernel S1S_{1}, it is easy to check that the following identity is true.

We can use this simple observation in the expression (2.10) that we obtained in the last section. First let us write the Christoffel Darboux kernel terms of the solution of a Riemann-Hilbert problem, we have

where σ3\sigma_{3} is the Pauli matrix σ3=diag⁡(1,−1)\sigma_{3}=\operatorname{diag}(1,-1), κ0,n=−2πih0,n\kappa_{0,n}=-\frac{2\pi i}{h_{0,n}} and C(f)C(f) is the Cauchy transform.

It is well-known that if the logarithmic derivative of w0w_{0} is rational, then the matrix Z(x)Z(x) in (4.39) satisfies a linear system of ODE

for some rational function A(x)A(x). By using (4.4) and the recurrence relation of the LnL_{n}

Let us now consider the derivative ∂K2(x,y)∂y\frac{\partial K_{2}(x,y)}{\partial y}. We have, from (4.38)

Similarly, ∂∂xK2(y,x)\frac{\partial}{\partial x}K_{2}(y,x) is given by

The sum of these two derivatives is therefore given by

By using the recurrence relations of the Laguerre polynomials, we obtain

Let K1(x,y)K_{1}(x,y) be the correction kernel in (2.10).

Then by using ∂S1(y,x)∂x+∂S1(x,y)∂y=0\frac{\partial S_{1}(y,x)}{\partial x}+\frac{\partial S_{1}(x,y)}{\partial y}=0 and the formula for h0,nh_{0,n},

In particular, the correction term K1(x,y)K_{1}(x,y) in the kernel can be written as

Derivative of the partition function

where S1(x,y)S_{1}(x,y) is the kernel given in (4.19).

Computing the individual determinants using the Laplace formula, we obtain

As rj(x)r_{j}(x) are independent on tt for j<N−2j<N-2, the derivative ∂tDij\partial_{t}D_{ij} is given by

for i,j<N−2i,j<N-2. For either ii or jj equal to N−2N-2 or N−1N-1, we have

Note that by orthogonality, the last two terms in the above expression are zero as ∂tπN−1,1\partial_{t}\pi_{N-1,1} is of degree N−2N-2 and ∂tπN−2,1\partial_{t}\pi_{N-2,1} is of degree N−3N-3. Applying the same argument to ∂tDi,N−2\partial_{t}D_{i,N-2}, we obtain

From this, (5.3) and the expression of the kernel in (4.19), we obtain (5.1). ∎

Asymptotic analysis

We will now use the asymptotics of the Laguerre polynomials to obtain asymptotic expression for the kernel S1(x,y)S_{1}(x,y). We will demonstrate the asymptotic analysis with the assumption that M/N→γ=1M/N\rightarrow\gamma=1. The same analysis also be applied for general γ\gamma.

Let n=N−jn=N-j, where j=O(1)j=O(1). Let us define the function φ(x)\varphi(x) to be

Similarly, the map fnf_{n} in a neighborhood of 44 is defined to be

As in , these maps are conformal inside the small discs around b±,nb_{\pm,n}, provided δ\delta is sufficiently small. In particular, they behave as follows as near b±,nb_{\pm,n}. (Recall that b−,n=0b_{-,n}=0 and b+,n=4b_{+,n}=4 when γ=1\gamma=1.)

where JαJ_{\alpha} is the Bessel function and ζ\zeta is the following

The branch cut of arccos⁡(x)\arccos(x) in the above is chosen to be (−∞,−1]∪[1,∞)(-\infty,-1]\cup[1,\infty). The constant κn\kappa_{n} is given by κn=−2πihn,0\kappa_{n}=-\frac{2\pi i}{h_{n,0}}.

Reader may notice that the asymptotic formula presented in Proposition 6.1 is different from the ones in . This is because the weight in that is relevant to us is w0(x)=xαe−4nxw_{0}(x)=x^{\alpha}e^{-4nx} and a rescaling of the variable from xx to y=4nNxy=\frac{4n}{N}x is needed to obtain the formula in Proposition 6.1 from the results in .

We will now use the asymptotic formulae in Proposition 6.1 to compute the skew products of the form <LN−j,LN−k>1\left<L_{N-j},L_{N-k}\right>_{1}. We shall follow the ideas in , and .

From (6.6), we see that as x→0x\rightarrow 0, sin⁡ζ\sin\zeta and cos⁡ζ\cos\zeta have the following behavior.

for some constants k1,jk_{1,j} and k2,jk_{2,j} that are bounded in nn. By using the asymptotic formula for the Bessel function in , we obtain the following.

Let k≥0k\geq 0 s>v≥0s>v\geq 0 and α>0\alpha>0, then as s→∞s\rightarrow\infty, we have

Let s1=O(s)s_{1}=O\left(s\right) as s→∞s\rightarrow\infty, and let B1=JαB_{1}=J_{\alpha}, B2=Jα′B_{2}=J^{\prime}_{\alpha}, then as s→∞s\rightarrow\infty, we have the following for the double integrals.

Integrating the first formula by parts, we obtain

This proves the first equation in (6.14). Integrating the second equation by parts and using Jα(0)=0J_{\alpha}(0)=0 for α>0\alpha>0, we obtain

By using the following estimates for any C>0C>0,

we obtain the second equation in (6.14). The estimate (6.15) now follows immediately from (6.14) and (6.16). ∎

We can now compute the integrals in the skew products in the Bessel region.

The single integral involving Ln(x)w(x)L_{n}(x)w(x) in the Bessel region is given by

The double integral in the Bessel region is given by

Let us first prove the single integral. We have, by (6.10),

By using the asymptotic formula for the Bessel function (, (9.2.5), (9.2.9) and (9.2.10)), we have obtain the following estimate

By using Lemma 6.1 and (6.16). We see that it is of the order

To compute the first term, note that, since

we have, by (6.20) and mean value theorem, the following

where ξu\xi_{u} is between uu and ν(u)\nu(u). As Jα(u)J_{\alpha}(u) is bounded, we have

This concludes the analysis in the Bessel region, we will now consider the integrals in the bulk region.

1.2 The Bulk region

First recall the following matching formula in the region [N2n,δ]\left[\frac{\sqrt{N}}{2n},\delta\right] from .

Uniformly for x∈[N2n,δ]x\in\left[\frac{\sqrt{N}}{2n},\delta\right], as n→∞n\rightarrow\infty,

Uniformly for x∈[4−ε,Nnc−]x\in\left[4-\varepsilon,\frac{N}{n}c_{-}\right], as n→∞n\rightarrow\infty, we have

This shows that throughout the bulk region, the function L^n(x)\hat{L}_{n}(x) in (6.10) has the following asymptotic behavior.

uniformly for x∈[N2n,Nnc−]x\in\left[\frac{\sqrt{N}}{2n},\frac{N}{n}c_{-}\right], where EE is an error term of order O(n−1(4−x)−32)+O(n−1x−12)O\left(n^{-1}(4-x)^{-\frac{3}{2}}\right)+O\left(n^{-1}x^{-\frac{1}{2}}\right). From this we can now compute the single integral.

Let c−=4−N−εc_{-}=4-N^{-\varepsilon} such that ε≤120\varepsilon\leq\frac{1}{20}. Suppose the distance from the point tt to the interval [Nn,NnC−]\left[\frac{\sqrt{N}}{n},\frac{N}{n}C_{-}\right] is greater than CN−εCN^{-\varepsilon} for some C>0C>0 and the distance from tt to is finite. Then the single integral in the bulk region is of the following order.

Since Fn=η++inφ+−π4F_{n}=\eta_{+}+in\varphi_{+}-\frac{\pi}{4}, we see that its derivative is given by

This gives us the following estimate of the order of 1/Fn′1/F_{n}^{\prime}.

We can now integrate the first term in (6.25) by parts to obtain

As the distance from tt to the bulk region is at least of order O(N−ε)O\left(N^{-\varepsilon}\right), the first term in the above equation is of order O(n5ε4−1)+O(n−78)O\left(n^{\frac{5\varepsilon}{4}-1}\right)+O\left(n^{-\frac{7}{8}}\right), which is of order O(n−78)O\left(n^{-\frac{7}{8}}\right) as ε≤1/20\varepsilon\leq 1/20. By repeating the integration by parts procedure to the second term, one can verify that it is of order at most O(n11ε4−2)O\left(n^{\frac{11\varepsilon}{4}-2}\right). This gives

Since the error term EE is of order O(n−1(4−x)−32)+O(n−1x−12)O\left(n^{-1}(4-x)^{-\frac{3}{2}}\right)+O\left(n^{-1}x^{-\frac{1}{2}}\right), we obtain the following estimate for contribution from EE.

This concludes the proof of the proposition. ∎

In particular, from the proof of Proposition 6.3, we see that

Let us now proceed to compute the double integrals. To begin with, we have the following lemma that will help us to simplify the results. (Proposition 5.12 in )

By differentiating θ(x)\theta(x) twice we see that

For some integration constant CC. By evaluating the above equation at x=4x=4, we see that C=0C=0. This proves the lemma. ∎

The lemma implies the following. (Proposition 5.13, )

Let n=N−jn=N-j, m=N−km=N-k where jj and kk are finite integers, then for x∈[Nn,Nnc−]x\in\left[\frac{\sqrt{N}}{n},\frac{N}{n}c_{-}\right], we have

As in , let us write the left hand side of (6.32) as

By repeat application of the mean value theorem, we see that the first term on the right hand side is given by

for some ξ∈[x,xn/m]\xi\in[x,xn/m]. From (6.26), we see that for x∈[Nn,Nnc−]x\in\left[\frac{\sqrt{N}}{n},\frac{N}{n}c_{-}\right], we have

As 4−x=N−ε4-x=N^{-\varepsilon} and ε≤1/20\varepsilon\leq 1/20, we have

where the last equality follows from lemma 6.3. ∎

We can now compute the double integrals in the bulk region.

The double integral inside the bulk region is of the following order.

The proof is similar to the computation in and . We have

Then by using (6.23), we see that the double integral is given by the following.

First let us compute the error terms. By changing the order of the integration, we have

where the last equality follows from (6.28). The order of the other error term can be estimated similarly. Let us now consider the leading order term. Integrating by parts, we obtain

To evaluate the second term, note that for yy in the interval [Nm,Nmc−]\left[\frac{\sqrt{N}}{m},\frac{N}{m}c_{-}\right], we have

Hence by interchanging the order of integration, we obtain

To compute the first term of J20\mathcal{J}_{20}, let us change the integration variable from xx to nmx\frac{n}{m}x. Then we obtain

Now by (6.27) and the fact that both 4−x4-x and t−nNxt-\frac{n}{N}x are of order at least n−εn^{-\varepsilon}, we obtain the follow estimate

To evaluate the integral, we use the angle addition formula for sine to obtain

The first term can be simplified using (6.32) while integration by parts shows that the second term is of order O(m−74)O\left(m^{-\frac{7}{4}}\right). This gives

As Nnc−−Nmc−\frac{N}{n}c_{-}-\frac{N}{m}c_{-} is of order m−1m^{-1}, we see that

Similarly, we can change the lower limit to Nn\frac{\sqrt{N}}{n} and add an error term of order O(m−2)O\left(m^{-2}\right). This proves the proposition. ∎

As we are only going to consider the values of mm and nn with m−n=±1m-n=\pm 1 or ±2\pm 2, we can simplify the double integrals further. First let us consider the case when m−n=±1m-n=\pm 1. A simple calculation shows that

We can now use these and residue calculation to compute the double integrals.

Then the asymptotics of the double integrals in the bulk region are given by the followings.

We shall compute the integrals using Cauchy theorem. Since (x−4)+=i4−x\left(\sqrt{x-4}\right)_{+}=i\sqrt{4-x} on [0,4]\left[0,4\right], we have, by using (6.34), the following

and similar relations for n−m=2n-m=2. The right hand side can be computed using Cauchy’s theorem and we obtain

From this and (6.33), (6.34) and (6.35), we have

This completes the proof of the Proposition. ∎

This completes the analysis in the bulk region. We will now move onto the Airy region.

1.3 The Airy region

The analysis in the Airy region is more difficult compare to the other regions as we will need to consider the case where the point tt is inside the Airy region. First let us compute the asymptotics of the function L^n(x)\hat{L}_{n}(x) in the Airy region.

As the asymptotics contain the functions Ai(fn)Ai(f_{n}) and Ai′(fn)Ai^{\prime}(f_{n}), we shall make a change of variable and write the asymptotics in terms of the function fnf_{n}. First, from the expression of fnf_{n} in Definition 6.1, we see that the map fnf_{n} is of the following order inside the Airy region.

Let us introduce the scaled variable TT to be

As TT is of finite distance from the integration contour, we have

where G1G_{1} and G2G_{2} are power series expansions in their arguments with coefficients independent on nn and NN. Note that the series expansion BB starts at power 1 while the expansion CC starts at power 2.

Let us write fn=uf_{n}=u, then by using (6.41) and (6.39), we can write L^n(x)/u′\hat{L}_{n}(x)/u^{\prime} as a series in terms of uu.

For some constants a0a_{0}, b0b_{0}, aka_{k} and bkb_{k} of the form

where ak,0a_{k,0} and bk,0b_{k,0} are independent on nn.

As the functions L^n\hat{L}_{n} are close to each other inside the Airy region, we will introduce the following function A(U)\mathcal{A}(U).

where x(U)x(U) is the inverse function of U=fN(x)U=f_{N}(x). The function A(U)\mathcal{A}(U) is regarded as a function in the variable UU. We shall express the double integrals in terms of the function A\mathcal{A}.

As in (6.39) we can write x(U)x(U) as a power series in UU (but with nn replaced by NN). In particular, we have

where Ci,n(u)\mathcal{C}_{i,n}(u) and Dn(u)\mathcal{D}_{n}(u) are power series of the form

where dk,j,l,nd_{k,j,l,n} and ci,k,j,nc_{i,k,j,n} are bounded and k≥2jk\geq 2j. In the series Ci,n(u)\mathcal{C}_{i,n}(u), both indices kk and jj start from , while in Dn(u)\mathcal{D}_{n}(u), kk and ll start from 11 and jj from . The term En(u)\mathcal{E}_{n}(u) is of the form

We are now ready to compute the single integrals. First let us show the following

Let k,j≥0k,j\geq 0, then as s±→+∞s_{\pm}\rightarrow+\infty and ∣s−∣/∣s+∣=O(1)|s_{-}|/|s_{+}|=O(1), we have

Let ν(u)\nu(u) be a function of uu such that ν(u)=O(u)\nu(u)=O(u) as u→∞u\rightarrow\infty and let v+=O(s+)v_{+}=O(s_{+}), then we have

where Ai(0)=AiAi^{(0)}=Ai and Ai(1)=Ai′Ai^{(1)}=Ai^{\prime}.

First note that, as the Airy function decays exponentially as u→∞u\rightarrow\infty,

as s+→+∞s_{+}\rightarrow+\infty. Therefore let us consider the integral in the negative real axis. Integrating by parts, we obtain

For integrals involving the derivative Ai′(u)Ai^{\prime}(u), we again note that Ai′(u)Ai^{\prime}(u) is decaying exponentially as u→+∞u\rightarrow+\infty and we again have

For the integral on the negative real axis, we perform integration by parts again and use the estimate

for some constant CC. This shows that the integral on the negative real axis is of order

This proves (6.48). The estimate (6.49) now follows immediately from (6.48) and (6.50). ∎

Let us now transform the limits in the Airy region into the variable uu. As in the previous cases, we are interested in the integral

The following is an immediate consequence of (6.44) and the estimates (6.48).

Let TT be defined as in (6.40), then the single integral in the Airy region is given by

This completes the analysis of the single integral in the Airy region. We will now analyze the double integrals.

We will change the integration variables to u=fn(x)u=f_{n}(x) and v=fm(y)v=f_{m}(y). We will denote the limits of the outer integral by u±u_{\pm} and the upper limit of the inner integral by v+v_{+}.

Let us now compute the lower limit of the inner integral. As both u=fn(x)u=f_{n}(x) and v=fm(y)v=f_{m}(y) are conformal inside the Airy region, they can be written as a series of each other. Then by (6.39) and the analogue for fmf_{m}, together with the fact that at the lower bound, y=nmxy=\frac{n}{m}x, we obtain

The following can easily be seen by writing vv as a series expansion in uu.

Let u=fn(x)u=f_{n}(x) and let ν(u)\nu(u) be the value of v=fmv=f_{m} at y=nmxy=\frac{n}{m}x, then as n,m→∞n,m\rightarrow\infty with m−nm-n finite, we have

By (6.49) and (6.44), we see that the double integral is given by

for some constants hkjh_{kj} that are independent on NN, nn and mm, where A(j,k)\mathcal{A}(j,k) are defined as follows.

First let us consider the leading order term in (6.57), which is given by A(0,0)\mathcal{A}(0,0).

Let L(u)\mathcal{L}(u) be the following function in uu.

where xN(u)x_{N}(u) is defined as the inverse function to u=fN(xN)u=f_{N}(x_{N}).

where the error term is uniform in TT as T→N23T\rightarrow N^{\frac{2}{3}}. Then A(u)\mathcal{A}(u) can be written as

The following can be derived using (6.22).

The derivatives of A(u)\mathcal{A}(u) behave as follows as u→−CN23−εu\rightarrow-CN^{\frac{2}{3}-\varepsilon} for some C>0C>0.

where k≥0k\geq 0 and xN(u)x_{N}(u) is the inverse of u=fN(x)u=f_{N}(x).

Changing the upper limit v+v_{+} into u+u_{+}, we can write the term A(0,0)\mathcal{A}(0,0) as

where ν\nu is treated as a function of uu by using Lemma 6.6.

Let us estimate the order of these terms.

Let u−/N23=O(N−ε)u_{-}/N^{\frac{2}{3}}=O\left(N^{-\varepsilon}\right). If jj is odd, then we have

The first equation can be proven using integration by parts. By (6.55), (6.61) and (6.60), we have

From (6.61), (6.55) and (6.60), the first term is of order O((u−/m23)j−42m−2)O\left(\left(u_{-}/m^{\frac{2}{3}}\right)^{\frac{j-4}{2}}m^{-2}\right). Repeating the integration by parts, we obtain (6.63).

To prove (6.64), we have, by (6.61), the following

as u→u−u\rightarrow u_{-}. After multiplying by (ν(u)−u)j+1(\nu(u)-u)^{j+1} and integrate, the error term O(uj−62m−13)O\left(u^{\frac{j-6}{2}}m^{-\frac{1}{3}}\right) gives a contribution of order O(N−43)O\left(N^{-\frac{4}{3}}\right) for j>0j>0 and O(N−23)O\left(N^{-\frac{2}{3}}\right) for j=0j=0.

The term with the cos⁡2FN\cos 2F_{N} factor can be integrated by parts using

Then by splitting the interval [u−,0][u_{-},0] into [u−,u0][u_{-},u_{0}] and [u0,0][u_{0},0] for some u0u_{0} between u−u_{-} and , and integrating the integral on [u−,u0][u_{-},u_{0}] by parts, we have

As A(u)A(j)(u)(ν−u)j+1\mathcal{A}(u)\mathcal{A}^{(j)}(u)(\nu-u)^{j+1} is integrable in [0,∞)[0,\infty) and have exponential decay at +∞+\infty, (6.64) now follows from (6.66). ∎

We would now like to combine the terms in (6.62) with the end point terms Fl\mathcal{F}_{l} in (6.36) from the double integral in the bulk region.

Let Fn−m\mathcal{F}_{n-m} be given by (6.36), then we have

From (6.36), we can write Fn−m\mathcal{F}_{n-m} in the following form. (After renaming the integration variable from xx to xNx_{N})

where ϕ(xN)=arccos⁡(xN2−1)\phi(x_{N})=\arccos\left(\frac{x_{N}}{2}-1\right). Let u=fN(xN)u=f_{N}(x_{N}). Then from the proof of Lemma 6.4, we can express ϕ(xN)\phi(x_{N}) as follows when u→u−u\rightarrow u_{-}.

Similarly, we have Fm(xN)=23(−fm)32+η+(xN)−π4F_{m}(x_{N})=\frac{2}{3}(-f_{m})^{\frac{3}{2}}+\eta_{+}(x_{N})-\frac{\pi}{4} and fm(xNn/m)=ν(fn)f_{m}(x_{N}n/m)=\nu(f_{n}). Then by Lemma 6.6 and fn(xN)=(nN)23fN(xN)=(nN)23uf_{n}(x_{N})=\left(\frac{n}{N}\right)^{\frac{2}{3}}f_{N}(x_{N})=\left(\frac{n}{N}\right)^{\frac{2}{3}}u, we obtain

as u→u−u\rightarrow u_{-}. From (6.59), we see that L2(u)\mathcal{L}^{2}(u) is given by

as u→u−u\rightarrow u_{-}. As ν−u=O(N−13)\nu-u=O\left(N^{-\frac{1}{3}}\right) and u−/N23=O(N−ε)u_{-}/N^{\frac{2}{3}}=O\left(N^{-\varepsilon}\right), we see that for k>1k>1,

as u→u−u\rightarrow u_{-}. Since ϕ(xN)=arccos⁡(xN2−1)\phi(x_{N})=\arccos\left(\frac{x_{N}}{2}-1\right) it behaves as 4−xN\sqrt{4-x_{N}} as x→4x\rightarrow 4. Therefore the function on the left hand side of (6.69) is integrable for u∈(u−,0)u\in(u_{-},0). Therefore by using ε≤1/20\varepsilon\leq 1/20, we have

for k>0k>0 and of order O(N−23)O\left(N^{-\frac{2}{3}}\right) for k=0k=0. This, together with (6.68), implies the Lemma. ∎

By (6.62), (6.68) and Lemma 6.8, 6.9, we see that A(0,0)\mathcal{A}(0,0) can be written as

By (6.55), we see that the terms in the sum involving A\mathcal{A} are of the form

Let us now compute the other terms in (6.57). These terms are of the form

for some for some constants hkjh_{kj} that are independent on NN, nn and mm.

To compute these terms, let us first prove the following.

Let FF and GG be integrable functions on [u−,u+][u_{-},u_{+}] such that FF and GG are of order e−ku32e^{-ku^{\frac{3}{2}}} as u→+∞u\rightarrow+\infty for some k>0k>0. Then we have

The lemma can be proved by integration by parts. We have

Integrating the first term by parts, we have

as FF is of order e−ku32e^{-ku^{\frac{3}{2}}} when u→+∞u\rightarrow+\infty. This implies

This, together with (6.73), implies the lemma. ∎

By taking F=A/(T−u)jF=\mathcal{A}/(T-u)^{j} and G=A/(T−u)kG=\mathcal{A}/(T-u)^{k} for A(j,k)\mathcal{A}(j,k), we have the following.

where AH(j,k)AH(j,k) and SH(j,k)SH(j,k) and Aj\mathcal{A}_{j} are given by

We can now consider the terms in (6.57). We shall first consider the terms where jj and kk are not both zero. From (6.49), we see that if j+k>2j+k>2, then the term will be of order O(N−43)O\left(N^{-\frac{4}{3}}\right). Therefore we shall only consider the cases where j+k≤2j+k\leq 2. Let us now compute the terms A(j,k)\mathcal{A}(j,k).

This can be proved by using the mean value theorem. By repeat use of mean value theorem, we have

for some ξu\xi_{u} between uu and ν(u)\nu(u). Therefore we have

Note that AjAk\mathcal{A}_{j}\mathcal{A}_{k} is of order N−13u−32−j−kN^{-\frac{1}{3}}u^{-\frac{3}{2}-j-k} as u→−∞u\rightarrow-\infty and decays exponentially as u→+∞u\rightarrow+\infty. Then by Lemma 6.6, we see that

where i=1,2i=1,2. Similarly, since j+k≥1j+k\geq 1, the function Aj(u)Ak′(ξu)\mathcal{A}_{j}(u)\mathcal{A}_{k}^{\prime}(\xi_{u}) is of order N−13u−2N^{-\frac{1}{3}}u^{-2} as u→−∞u\rightarrow-\infty and decays exponentially as u→∞u\rightarrow\infty. Hence the integral involving Aj(u)Ak′(ξu)\mathcal{A}_{j}(u)\mathcal{A}_{k}^{\prime}(\xi_{u}) is of order N−1N^{-1}. This proves the lemma. ∎

From this, (6.77) and (6.55), we can compute the terms AH(j,k)AH(j,k) and SH(j,k)SH(j,k).

Then the terms AH(j,k)AH(j,k) and SH(j,k)SH(j,k) are of order

By using this, (6.49) and (6.55), together with the formula for A(0,0)\mathcal{A}(0,0) (6.70) and (6.71), we arrive at the following.

where the terms J3j\mathcal{J}_{3j} are given by

As we shall see, the terms J31\mathcal{J}_{31} and J32\mathcal{J}_{32} will in fact not enter into the expression of the kernel K1K_{1}. What is important is the structure of equation (6.78).

Throughout this section, all the dependence on TT are through factors of (T−u)−j2(T-u)^{-\frac{j}{2}} for j>0j>0, with the exception of the function L(u)\mathcal{L}(u). From the definition of L(u)\mathcal{L}(u) in (6.59), we see that it can be written in the form (6.60)

with an error term that is uniform in TT as long as TT is not on the integration contour of uu and vv. Therefore all error terms in this section is uniform in TT as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}} on the contour Ξ+\Xi_{+} in Theorem 2.4.

1.4 The exponential region

Inside the exponential region [4+N−ε,∞)[4+N^{-\varepsilon},\infty), we have the following matching formula for the polynomials (See Lemma 4.8 of ).

For any d>0d>0 there exists a constant k>0k>0 such that, uniformly for x∈[4+N−d,∞)x\in[4+N^{-d},\infty), we have

From this, it is clear that the contribution from the exponential region is of order O(e−kN23−ε)O\left(e^{-kN^{\frac{2}{3}-\varepsilon}}\right) for some k>0k>0.

2 Asymptotics of the skew inner product

We can now compute the asymptotics of the skew inner products <Ln,Lm>1\left<L_{n},L_{m}\right>_{1}. We have

By breaking the range of these integrals into different regions, we obtain

From this and (6.17), (6.18), (6.37) and Lemma 6.12, we arrive at the following.

The product <Ln,Lm>1\left<L_{n},L_{m}\right>_{1} is given by

where J3j\mathcal{J}_{3j} are given in (6.79) and JB1\mathcal{J}_{B1}, JB2\mathcal{J}_{B2} and IjI_{j} are given by

We can simplify the expression further by the observation that <Ln,Lm>1=0\left<L_{n},L_{m}\right>_{1}=0 whenever n−m=1n-m=1 and nn is even. (See Corollary 4.1) Taking k=1k=1 and nn even in (6.82), we have

As this holds for any finite N−nN-n as long as nn is even, we obtain the following relations.

Note that although in the above equation, integration limits u±u_{\pm} depend on nn, the effect of changing these limits will only result in terms of order O(N−2524)O\left(N^{-\frac{25}{24}}\right) and hence we can consider them as fixed under the change of nn.

Let us now compute the factor κn−1κm−1\kappa_{n-1}\kappa_{m-1}. We have κn=−2πihn,0\kappa_{n}=-\frac{2\pi i}{h_{n,0}}. By (4.49), we see that hn,0/hm,0=1+O(N−1)h_{n,0}/h_{m,0}=1+O\left(N^{-1}\right). From this, Proposition 6.7 and (6.85), we see that the skew inner products that we need have the following asymptotics.

Note that, by Remark 6.2, these error terms are uniform in TT as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}}. Let us look at the behavior of the skew products when ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}} and when tt remain finite.

First by (6.83), we see that as T→∞T\rightarrow\infty, the integrals IjI_{j} are of the following orders as T→∞T\rightarrow\infty.

(The statement is clear if ∣T∣>u−|T|>u_{-}. If ∣T∣<u−|T|<u_{-}, then by breaking the range of the integral into (u−,−∣T∣12)(u_{-},-|T|^{\frac{1}{2}}) and (−∣T∣12,u+)(-|T|^{\frac{1}{2}},u_{+}) and integrate by parts the integral over (u−,−∣T∣12)(u_{-},-|T|^{\frac{1}{2}}) using (6.61), one can check that (6.87) is correct.)

By using t=4+(4N)23Tt=4+\left(\frac{4}{N}\right)^{\frac{2}{3}}T in (6.84), we see that JB3,2\mathcal{J}_{B3,2} is of the following order.

From these we obtain the behavior of the skew products as T→∞T\rightarrow\infty.

The skew products <Ln,Lm>1\left<L_{n},L_{m}\right>_{1} in (6.86) are of the following orders as T→∞T\rightarrow\infty.

We can now compute the asymptotic of the kernel.

First let us used the results in the previous sections to compute the correction term to the kernel. Let us define the variables ξ1\xi_{1} and ξ2\xi_{2} to be

We will assume that ξ1\xi_{1} and ξ2\xi_{2} are bounded from below. First we need to compute the integrals ϵ(πn,1w)\epsilon(\pi_{n,1}w), which is a linear combinations of the integrals of the LnwL_{n}w. We have

To compute the first term, let us first assume ξ2<N18\xi_{2}<N^{\frac{1}{8}}. Then we have, by the asymptotic formula of the Ln(x)L_{n}(x) inside the Airy region, and the estimates ,

for some k>0k>0, where u=fn(y)u=f_{n}(y). Note that by (6.91), we in fact have an exponential decay of order e−kξ23/2e^{-k\xi_{2}^{3/2}} in the error term above. However, the decay e−kξ2e^{-k\xi_{2}} will be sufficient for our purpose. The lower limit u(Nny)u\left(\frac{N}{n}y\right) can be expressed in terms of ξ2\xi_{2} as follows.

where j>0j>0. By using mean value theorem and (6.91), we can write the integral as

for some k>0k>0. The Lj\mathcal{L}_{j} in (6.93) are given by

On the other hand, if ξ2>N18\xi_{2}>N^{\frac{1}{8}}, then from Lemma 6.13 and the asymptotic formula for the Airy function, we see that

for some constant k>0k>0. Therefore if we choose the constant kk in (6.93) to be small enough, then (6.93) remains valid for all ξ2\xi_{2} bounded below.

Similarly, the second term in (6.92) is given by

Let u−,Nu_{-,N} be fN(c−)f_{N}(c_{-}), then changing the lower limit in the above integral into u−,Nu_{-,N} will only result in an error term of order O(N−1+3ε4)=O(N−78)O\left(N^{-1+\frac{3\varepsilon}{4}}\right)=O\left(N^{-\frac{7}{8}}\right). Similarly, changing the upper limit to +∞+\infty will only result in an exponentially small error term. We can therefore change the lower limit in the integration to u−,Nu_{-,N} and the upper limit to +∞+\infty. Let ξ2,N\xi_{2,N} be the value of ξ2\xi_{2} at u=u−,Nu=u_{-,N}, then we have

Similarly, the orthogonal polynomials Ln(x)L_{n}(x) are given by

where f1f_{1} and f2f_{2} are functions that are independent on NN, nn and TT. Then by using (4.51), we obtain the asymptotics for the correction kernel K1(x,y)K_{1}(x,y).

The coefficients Qjk\mathcal{Q}_{jk} are given by

From (6.87) and (6.88), we see that as T→∞T\rightarrow\infty, the kernel K1K_{1} has the following behavior

In fact, by using (6.86), (6.89) and (4.51), we obtain the following.

As T→∞T\rightarrow\infty and tt remains bounded, the kernel K2K_{2} and K1K_{1} become the Airy kernels in the large NN limit.

The statement for the kernel K2K_{2} follows immediately from the representation (2.11) and the Airy asymptotics of the Laguerre polynomials. To prove the statement for the correction term K1K_{1}, first note that, by (6.86), we see that

From this, (6.100), (6.95), (6.96) and (4.51), we see that in this limit, K1K_{1} is given by

By using the explicit expressions for A\mathcal{A} and Ψj\Psi_{j}, we obtain the asymptotic formula for the kernel when TT is finite.

Let TT be of order N13−cN^{\frac{1}{3}-c} for some positive 0<c≤130<c\leq\frac{1}{3}, then for ξ1\xi_{1} and ξ2\xi_{2} bounded from below, the kernel K1(ξ1,ξ2)K_{1}(\xi_{1},\xi_{2}) is given by

for some k>0k>0, where HjH_{j}, B1\mathcal{B}_{1} and B2\mathcal{B}_{2} are given by

As pointed out in , and , the eigenvalue statistics will not be affected by the rescaling

of the matrix kernel. By rescaling the kernel in this way, all the entries will have the same order in the large NN limit. From now on, we shall use this rescaled kernel and denote it also by KK.

From (6.101), we obtain the following estimate for the rescaled matrix kernel KK.

Let K∞K_{\infty} be the 2×22\times 2 matrix whose entries are given by

where K2,∞(ξ1,ξ2)K_{2,\infty}(\xi_{1},\xi_{2}) is given by

Suppose TT is of order N13−cN^{\frac{1}{3}-c} for some positive 0<c≤130<c\leq\frac{1}{3} and that ξ1\xi_{1} and ξ2\xi_{2} are bounded from below. Let K(ξ1,ξ2)K(\xi_{1},\xi_{2}) be the rescaled matrix kernel in (6.103), then there exists k>0k>0 such that

The statement for the 11th11^{th} and 22th22^{th} entries follows immediately from (6.101), the representation (2.11) and the asymptotics of the Laguerre polynomials inside the Airy region. The statement for the 12th12^{th} entry follows by replacing ϵ(Lnw)\epsilon(L_{n}w) in (6.95) by the asymptotics of the polynomials in (6.96) in the derivation of (6.97). The computation is the same as the derivation of (6.97) and we shall not carry out the details here. To obtain the results for the 21th21^{th} entry, we use the fact that ϵ(S1)(x,y)\epsilon\left(S_{1}\right)(x,y) is skew symmetric to obtain (See , , )

The statement for the 21th21^{th} entry then follows from integrating (6.101) and the asymptotic formula for K2K_{2}. ∎

A similar statement can be obtained for the Airy kernels when T→∞T\rightarrow\infty.

Let Kairy(ξ1,ξ2)K_{airy}(\xi_{1},\xi_{2}) be the following matrix kernel

Then for T→∞T\rightarrow\infty with tt finite and ξ1\xi_{1} and ξ2\xi_{2} bounded from below, there exists k>0k>0 such that the rescaled matrix kernel K(ξ1,ξ2)K(\xi_{1},\xi_{2}) in (6.103) is of the following order as N→∞N\rightarrow\infty.

In order to show that the convergence of the Fredholm determinant, we need the following bounds on the derivatives of the kernel K2K_{2}.

For TT of order N13−cN^{\frac{1}{3}-c} for some 0<c≤130<c\leq\frac{1}{3}, we have

The lemma is an immediate consequence of the following results in (, (3.8))

and KlagK_{lag} is the Christoffel Darboux kernel of the Laguerre polynomials

and x=4+ξ1(4/N)23x=4+\xi_{1}\left(4/N\right)^{\frac{2}{3}}, y=4+ξ2(4/N)23y=4+\xi_{2}\left(4/N\right)^{\frac{2}{3}}. As K2K_{2} is the conjugate to KlagK_{lag} and K2,∞K_{2,\infty} is the conjugate to K2,airyK_{2,airy},

The corresponding statement when T→∞T\rightarrow\infty follows from the same argument but with K2,∞K_{2,\infty} replaced by K2,airyK_{2,airy}.

With the estimates in Proposition 6.9 and Lemma 6.17, we can obtain the following asymptotic result for the determinant det⁡2(I−χKχ)\det_{2}\left(I-\chi K\chi\right).

Let ζ=(z−4)(N/4)23\zeta=(z-4)\left(N/4\right)^{\frac{2}{3}}, ξ1=(x−4)(N/4)23\xi_{1}=(x-4)\left(N/4\right)^{\frac{2}{3}}, ξ2=(y−4)(N/4)23\xi_{2}=(y-4)\left(N/4\right)^{\frac{2}{3}}, g(ξ)=1+ξ2g(\xi)=\sqrt{1+\xi^{2}} and G=diag⁡(g,g−1)G=\operatorname{diag}(g,g^{-1}), then as N→∞N\rightarrow\infty and TT of order up to o(N13)o\left(N^{\frac{1}{3}}\right), we have

and for T→∞T\rightarrow\infty while tt remain finite, we have

The proof of this proposition is exactly the same as the proof of Corollary 1.4 in . We shall not repeat the details of the proof here. As in , the function g(ξ)=1+ξ2g(\xi)=\sqrt{1+\xi^{2}} is to ensure that the 2-determinant exists and there is a great freedom in the choice of the g(ξ)g(\xi).

where K2(x,y)K_{2}(x,y) is the kernel given by the Laguerre polynomials (2.11) and K1(x,y)K_{1}(x,y) is the correction term on the right hand side of (2.10).

To compute the contribution from the kernel K2K_{2}, we will use the following differential identity . (See also Lemma 2.1) Let Z^\hat{Z} be the matrix related to the matrix ZZ in (4.39) by Z^=Zw0−σ32\hat{Z}=Zw_{0}^{-\frac{\sigma_{3}}{2}}. Then we have

Let Z^=Zw0−σ32\hat{Z}=Zw_{0}^{-\frac{\sigma_{3}}{2}}, where ZZ is the matrix in (4.39). Then we have

and then deform the contour of integration to obtain (6.108).

The asymptotics of the matrix Z^\hat{Z} can be found in . For x∉x\notin, the asymptotics of Z^\hat{Z} is given by

where R(x)R(x) is of the form I+O(N−1)I+O\left(N^{-1}\right) and P∞(x)P_{\infty}(x) is a matrix bounded in xx for x∉x\notin. Near the point 44, both the matrix P∞P_{\infty} and P∞−1P_{\infty}^{-1} have a forth root singularity. The derivative of R(x)R(x) is of order O(N−1)O\left(N^{-1}\right) and the derivative of P∞(x)P_{\infty}(x) remains bounded. From this, we have

As we will see, this is the part that determines where the saddle point is. Once we have done the saddle point analysis later on in this section, we will see that at the phase transition, the saddle point will be inside the Airy region. We therefore also need the asymptotics of the matrix Z^(x)\hat{Z}(x) inside the Airy region. This again, can be found in .

(, Section 5.3) The asymptotics of the matrix Z^(x)\hat{Z}(x) inside a small disc UδU_{\delta} of radius δ\delta around 44 is given by

where η±\eta_{\pm} is given by (6.8) and A(ξ)A(\xi) is the matrix

where ω=e2πi3\omega=e^{\frac{2\pi i}{3}} and the regions II, IIII, IIIIII and IVIV are given by

where the overline indicates complex conjugation. The matrix R(x)R(x) is again of the form I+O(N−1)I+O\left(N^{-1}\right). Its derivative is of order R′(x)=O(N−1)R^{\prime}(x)=O\left(N^{-1}\right).

From the behavior of the functions η±\eta_{\pm}, we see that the asymptotics of Z^(x)\hat{Z}(x) inside the Airy region is of the form

where both Pa(x)P_{a}(x) and Pa−1(x)P_{a}^{-1}(x) are bounded and analytic inside UδU_{\delta} (See ). Moreover, as fN(x)→∞f_{N}(x)\rightarrow\infty, there is a matching condition between the formula for Z^(x)\hat{Z}(x) in the Airy region and its formula in the outside region (6.109).

From this and the fact that P∞P_{\infty} is of order O((x−4)−14)O\left((x-4)^{-\frac{1}{4}}\right) as x→4x\rightarrow 4, we see that (6.110) remains valid if T=(t−4)(N/4)23T=\left(t-4\right)\left(N/4\right)^{\frac{2}{3}} is large, but with some modifications in the error term.

We shall divide the range of TT into the regimes 0<∣T∣≤N1/50<|T|\leq N^{1/5} and ∣T∣≥N1/5|T|\geq N^{1/5} and use (6.113) to for ∣T∣≥N1/5|T|\geq N^{1/5}. Let us now assume ∣T∣≤N1/5|T|\leq N^{1/5}. Then from (6.111) we obtain

The error term is uniform in TT throughout UδU_{\delta}. By using the asymptotic formula for the Airy functions, we see that the matrix A(ξ)A(\xi) has the following behavior as ξ→∞\xi\rightarrow\infty.

Therefore uniformly in UδU_{\delta}, the second term in (6.114) is of order

By (6.115), the first term in (6.114) has the following behavior as fN→∞f_{N}\rightarrow\infty.

Since fN(t)=T(1+O(T/N23))f_{N}\left(t\right)=T\left(1+O\left(T/N^{\frac{2}{3}}\right)\right), we have, by mean value theorem,

where ∣T∣≤N15|T|\leq N^{\frac{1}{5}} and ∣T0∣=N15|T_{0}|=N^{\frac{1}{5}}. For ∣T∣≥N15|T|\geq N^{\frac{1}{5}} and ∣T0∣=N15|T_{0}|=N^{\frac{1}{5}}, we have, by (6.113), the following

Since the first term is of order O(T32)+O(N13T)O\left(T^{\frac{3}{2}}\right)+O\left(N^{\frac{1}{3}}T\right), we see that for ∣T∣≥N15|T|\geq N^{\frac{1}{5}}, the first term will dominate over the error term. Summarizing, we have the following.

Uniformly for ∣T∣≤N15|T|\leq N^{\frac{1}{5}}, we have

for any ∣T0∣=N15|T_{0}|=N^{\frac{1}{5}}, where the integration contour does not cross the jump contours of the matrix AA.

Uniformly for ∣T∣>N15|T|>N^{\frac{1}{5}}, we have

where the integration contour does not cross (−∞,4](-\infty,4].

Let us now compute the contribution from the correction term K1(x,y)K_{1}(x,y). Before we compute the asymptotics, let us make a further simplification using (4.51). First by using the recurrence relation of the Laguerre polynomials (4.41), we see that

Substituting this back into (4.51), we obtain

where we have used the fact that <LN,LN−1>1=0\left<L_{N},L_{N-1}\right>_{1}=0.

The main task is to compute the products <Ln/(t−x),Lm>1\left<L_{n}/(t-x),L_{m}\right>_{1}. The analysis is very similar to those in Section 6. First note that, outside of the Airy region, the analysis in Section 6 remains the same and we have

The single and double integrals in <Ln/(t−x),Lm>1\left<L_{n}/(t-x),L_{m}\right>_{1} have the following contributions in the Bessel region.

The double integral in the Bessel region is given by

The single integral in the bulk region is given by

Let n−m=kn-m=k, then the asymptotics of the double integrals in the bulk region is given by the following.

and J2\mathcal{J}_{2} is given in (6.37).

Note that the choice of ε≤1/20\varepsilon\leq 1/20 ensures that the error terms are of the same order as before.

In the Airy region, the analysis is more different. Let us now compute these integrals inside the Airy region. As in Section 6.1.3, we have

where v0,nv_{0,n} is given in (6.47). By using mean value theorem, (6.55), we obtain the following estimate.

for some ξu\xi_{u} between uu and ν(u)\nu(u). As

we see that this term is of order O(N−43T−12)O\left(N^{-\frac{4}{3}}T^{-\frac{1}{2}}\right) as T→∞T\rightarrow\infty and ∣T∣<∣u−∣|T|<|u_{-}|. Applying similar argument to the other error terms in (6.125), we see that

Let us now determine the behavior of these terms as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}}. We have

As ∣T∣→∣u−∣|T|\rightarrow|u_{-}|, the terms A0(i,j)\mathcal{A}_{0}(i,j) is of order O(N−13T−i−j−1)O\left(N^{-\frac{1}{3}}T^{-i-j-1}\right) in TT.

Let us write the integral in the following form

Then it is clear that the third term is of order O(N−13T−i−j−1)O\left(N^{-\frac{1}{3}}T^{-i-j-1}\right) in NN and TT as ∣T∣→∣u−∣|T|\rightarrow|u_{-}|. By using the asymptotic formula (6.61) to integrate the second term by parts, we see that this term is also of order O(N−13T−i−j−1)O\left(N^{-\frac{1}{3}}T^{-i-j-1}\right). For the first term, we have, from (6.61), the following

for some constant C>0C>0 independent on TT and NN. Integrating this gives us the result. ∎

From Lemma 6.21 and the asymptotic behavior of A\mathcal{A}, we see that the various terms in the above expansion are of the following behavior as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}}.

From (6.126), we obtain the double integral inside of the Airy region.

Let us now compute the order of the following term in (6.118) inside the Airy region.

First by differentiating the identity <LN,LN−1>1=0\left<L_{N},L_{N-1}\right>_{1}=0, we can establish the following.

Let k=n−mk=n-m, then <Lnt−x,Lm>1\left<\frac{L_{n}}{t-x},L_{m}\right>_{1} is given by

The lemma follows from a straightforward calculation using (6.126) and Lemma 6.20.

As in the computation of the skew products <L2k,L2k−1>1=0\left<L_{2k},L_{2k-1}\right>_{1}=0 can be used to simplify the expressions <Lnt−x,Lm>1\left<\frac{L_{n}}{t-x},L_{m}\right>_{1}. In this case, we differentiate the identity <L2k,L2k−1>1=0\left<L_{2k},L_{2k-1}\right>_{1}=0 with respect to tt. Then we obtain

By using Lemma 6.22, we obtain the following identities.

where E1E_{1} and E2E_{2} are error terms that behave as the error terms in (6.132) and J2\mathcal{J}_{2} in the above is taken to be the expression in (6.37) with n−m=1n-m=1.

We can now compute the term D1D_{1} in (6.128). By using Lemma 6.22, we obtain the following

where the error term EE has the same order as the ones in (6.132).

Let us now show that F2−2F1\mathcal{F}_{2}-2\mathcal{F}_{1} is of order O(N−1−ε2)O\left(N^{-1-\frac{\varepsilon}{2}}\right).

From (6.36), we see that F2−2F1\mathcal{F}_{2}-2\mathcal{F}_{1} is given by

where again, ϕ=arccos⁡(x2−1)\phi=\arccos\left(\frac{x}{2}-1\right). As ϕ=4−x(1+O(x−4))\phi=\sqrt{4-x}\left(1+O\left(x-4\right)\right), we have

By the change of variable x=4+(4N)23ξx=4+\left(\frac{4}{N}\right)^{\frac{2}{3}}\xi and t=4+(4N)23Tt=4+\left(\frac{4}{N}\right)^{\frac{2}{3}}T, it is easy to see that the above integral is of order O(N−1−ϵ2)O\left(N^{-1-\frac{\epsilon}{2}}\right). Hence after integration, we obtain

Let us now consider the other terms in (6.118). Let D2D_{2} be

By using (6.86) and (4.50), we see that D2D_{2} is given by

Note that the error term O(N−2524)O\left(N^{-\frac{25}{24}}\right) is uniform in TT as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}} and its derivative is of the same order and is also uniform in TT. From this, we obtain

By using the definitions of I0I_{0}, I1I_{1} and JB2\mathcal{J}_{B2}, JB3,2\mathcal{J}_{B3,2} in Proposition 6.7, we obtain the following for D2D_{2}.

The orders of TT in the error terms indicates their behavior as ∣T∣→N23|T|\rightarrow N^{\frac{2}{3}}. Summarizing, we obtain the contribution to the derivative from the correction kernel K1(x,y)K_{1}(x,y).

Let ∣T∣<N13|T|<N^{\frac{1}{3}}. Then the contribution of K1(x,y)K_{1}(x,y) to the logarithmic derivative is given by

The fact that the integral remains bounded for tt finite follows from the estimates (6.127) and the expression (6.137).

5 Steepest descent analysis

First note that the expressions in Proposition 6.11 and 6.12 can be simplified further through integration by parts. By repeat use of integration by parts, we can write the following terms in (6.135) as

The term (−u)12π(T−u)\frac{(-u)^{\frac{1}{2}}}{\pi(T-u)} is there to ensure the convergence of the respective integrals. From the jump discontinuities and the behavior at T→∞T\rightarrow\infty, one can check that

Therefore we have, for ∣T∣<N15|T|<N^{\frac{1}{5}},

Uniformly for ∣T∣<N15|T|<N^{\frac{1}{5}}, we have

where C0C_{0} is an integration constant and S11\mathcal{S}_{11} is given by (6.138), while S10\mathcal{S}_{10} is

6 Saddle point analysis

For τ∈(−1,0)\tau\in(-1,0), we have tsaddle∈(−∞,0)t_{saddle}\in(-\infty,0) and for 0<τ<1/40<\tau<1/4, we have and tsaddle∈[4,∞)t_{saddle}\in[4,\infty). Hence the saddle point tsaddlet_{saddle} will not intersect the bulk region (0,4)(0,4) for any value of τ≠±1\tau\neq\pm 1. In this case, we can deform the contour Γ\Gamma such that it does not intersect the interval $andbyProposition6.10,weseethatthekernelsand by Proposition 6.10, we see that the kernelsK_{1}andandK_{2}becometherespectiveAirykernelsforallbecome the respective Airy kernels for allt\in\Gamma$. The largest eigenvalue distribution in this case becomes

for some function f1(t)f_{1}(t) independent on zz and f2(t,z)f_{2}(t,z) of order o(1)o(1). This gives us the Tracy Widom distribution for the largest eigenvalue. This is a known result in .

However, when τ=1\tau=1, saddle point coincides with the right edge point. In this case, the main contribution of the integral in tt will come from a neighborhood of t=4t=4 and the kernels will become significantly different from the Airy kernel. This is the case when the phase transition happens. Let us now find the steepest descent contour in this case.

We can therefore choose our integration contour as in Figure 2 to obtain

Let w=(N4)13(1−τ)∈(−∞,∞)w=\left(\frac{N}{4}\right)^{\frac{1}{3}}(1-\tau)\in(-\infty,\infty) and let ζ=(z−4)(N/4)23\zeta=(z-4)\left(N/4\right)^{\frac{2}{3}}, then as N→∞N\rightarrow\infty, the largest eigenvalue distribution is given by

In the above formula, the integration should be understood as a sum of integrations performed over the contours Ξ+\Xi_{+} and Ξ−\Xi_{-}, where Ξ±\Xi_{\pm} are the intersections of Ξ\Xi with the upper/lower half plane. Near the intersection point T0T_{0}, the boundary values of the integrand in the upper/lower half planes are to be taken when performing these integrals.

Fredholm determinant

Let S1,∞S_{1,\infty} be the operator with the kernel S1,∞=K1,∞+K2,∞S_{1,\infty}=K_{1,\infty}+K_{2,\infty}, DD the differential operator, ϵ\epsilon the operator with kernel ϵ(ξ1−ξ2)\epsilon(\xi_{1}-\xi_{2}) and χ\chi the multiplication by χ[ζ,∞)\chi_{[\zeta,\infty)}, where ζ=(z−4)(N/4)23\zeta=(z-4)\left(N/4\right)^{\frac{2}{3}}. Then by Proposition 6.10, we would like to consider the determinant of the following operator.

then by using det⁡(I−AB)=det⁡(I−BA)\det\left(I-AB\right)=\det\left(I-BA\right), we obtain

from this, we see that the determinant can be written as the determinant of the scalar operator

we see that the first term is equal to S1,∞ϵS_{1,\infty}\epsilon because S1,∞D=DS1,∞TS_{1,\infty}D=DS_{1,\infty}^{T}, and hence ϵS1,∞=S1,∞Tϵ\epsilon S_{1,\infty}=S_{1,\infty}^{T}\epsilon. Let us compute the second term. Let ff be an L2L^{2} function, then

These terms can be computed using integration by parts. The first term becomes

As −∂∂ξ2S1,∞(t,ξ2)=∂∂tS1,∞(ξ2,t)-\frac{\partial}{\partial\xi_{2}}S_{1,\infty}(t,\xi_{2})=\frac{\partial}{\partial t}S_{1,\infty}(\xi_{2},t), we obtain

As mentioned before, the procedure in obtaining (7.3) can be rigorously justified as in . We shall therefore treat (7.3) as a rigorous formula and refer the readers to .

Before we compute the asymptotics of this determinant, let us first recall some facts about Fredholm determinants and their relations to Painlevé equations.

Let us now recall some basic facts about operators of the form (6.106). The Airy kernel (6.106) is an integrable kernel, that is, it has the form

In this case, we have k=2k=2 and f11=−f22=Aif_{11}=-f_{22}=Ai, while f21=f12=Ai′f_{21}=f_{12}=Ai^{\prime}. Operators of these form appear often in random matrix theory and have been studied extensively in the literature. These operators were first singled out as a distinguished class in in which their properties were also studied. In random matrix theory, they were used to obtain the celebrated Tracy-Widom distribution.

Let us remind ourselves the following well-known facts about integrable operators. (See e.g. , , ) Let the kernel of an integrable operator on a contour Σ\Sigma be given by (7.4). Suppose I−KI-K is invertible, then the resolvent RR given by

is also an integrable operator with kernel given by

For our analysis, we will also need Φ2\Phi_{2} defined by Φ2=(I−K2,airyχ)−1Ai′′\Phi_{2}=\left(I-K_{2,airy}\chi\right)^{-1}Ai^{\prime\prime}. The resolvent R0χR_{0}\chi is closely related to the Hastings-McLeod solution of the Painlevé II equation. In fact, the determinant det⁡(I+R0χ)\det\left(I+R_{0}\chi\right) is well-known in the random matrix literature and is given by the Tracy-Widom distribution for the GUE .

The operator S1,∞S_{1,\infty} has kernel S1,∞=K1,∞+ψ−1K2,airyψS_{1,\infty}=K_{1,\infty}+\psi^{-1}K_{2,airy}\psi, where ψ\psi is the multiplication of the function ψ=(T−ξ)12\psi=(T-\xi)^{\frac{1}{2}}. We will also use the same notation to denote this square root function itself.

By substituting the asymptotic kernels into (7.3), we obtain

where f⊗hf\otimes h is the operator with kernel f(x)h(y)f(x)h(y). As in , the operator (1−χ)ϵχD(1-\chi)\epsilon\chi D is given by (See (16) in )

where ϵζ\epsilon_{\zeta}, ϵ∞\epsilon_{\infty}, δζ\delta_{\zeta} and δ∞\delta_{\infty} are given by

From these definitions, it is easy to see that

Now from (6.101), we see that the kernel K1,∞K_{1,\infty} is of rank 2.

We will also introduce some auxiliary functions

which will be more convenient for the purpose of deriving the ODEs. Note that, as in and , the u±,jku_{\pm,jk} can be written as

where we have used (7.8) in the above. By using the definition of the resolvent (7.5) to write R0χR_{0}\chi as R0χ=K2,airyχ(I+K2,airyχ)−1R_{0}\chi=K_{2,airy}\chi\left(I+K_{2,airy}\chi\right)^{-1}, we see that

We have the following relations between these variables.

The functions VkV_{k} and Q+,kQ_{+,k} in (7.17) can be written as

By using the definition of the resolvent (7.5), we see that (I+R0χ)K2,airy=R0(I+R_{0}\chi)K_{2,airy}=R_{0} and hence VkV_{k} can be written as

where we have used the property of integrable operators (7.8). The first equation then follows immediately from this.

By using ψ=(T−ξ)12\psi=(T-\xi)^{\frac{1}{2}}, one can easily verify the following.

The equation relating Q±,jQ_{\pm,j} and R±\mathcal{R}_{\pm} then follows from this and (7.19). ∎

By subtracting 1/2(H0,(1−χ))1/2(H_{0},(1-\chi)) times the second column, and 1/2(H1,(1−χ))1/2(H_{1},(1-\chi)) times the third column from the first column of the determinant det⁡(I−(αj,βk))\det\left(I-(\alpha_{j},\beta_{k})\right), we see that the determinant is the same as

By using (7.20), (7.15), (7.17) and (7.18), we see that the other entries (αi,βj)(\alpha_{i},\beta_{j}) can be written as

where q−,jq_{-,j} are the values of Q−,jQ_{-,j} at ζ\zeta and q−,j(∞)q_{-,j}^{(\infty)} are the values of Q−,jQ_{-,j} at ∞\infty.

Let us now derive ODEs for these functions in the variable ζ\zeta. First recall the following formula that holds for arbitrary operator KK that depends smoothly on a parameter ζ\zeta.

Applying this to the operator K2,airyχK_{2,airy}\chi, we obtain, as in , the followings.

where ρ(ξ1,ξ2)\rho(\xi_{1},\xi_{2}) is the kernel of I+R0χI+R_{0}\chi, that is, ρ(ξ1,ξ2)=δ(ξ1−ξ2)+R0(ξ1,ξ2)χ\rho(\xi_{1},\xi_{2})=\delta(\xi_{1}-\xi_{2})+R_{0}(\xi_{1},\xi_{2})\chi. Now from (6.106), we obtain the following.

This then implies the following for the derivative of ρ(ξ1,ξ2)\rho(\xi_{1},\xi_{2}).

where we have used the fact that the kernel of the operator (f⊗g)A(f\otimes g)A is the same as the kernel (f⊗ATg)(f\otimes A^{T}g) and that χ(I+R0χ)\chi(I+R_{0}\chi) is the same as its transpose, together with (I+R0χ)K2,airyχ=R0χ(I+R_{0}\chi)K_{2,airy}\chi=R_{0}\chi.

From this and (7.25), we obtain the following for ρ(ξ1,ξ2)\rho(\xi_{1},\xi_{2}) as in .

From (7.26) and ρ(ξ1,ξ2)=δ(ξ1−ξ2)+R0(ξ1,ξ2)χ\rho(\xi_{1},\xi_{2})=\delta(\xi_{1}-\xi_{2})+R_{0}(\xi_{1},\xi_{2})\chi, we obtain the following for ξ2∈(ζ,∞)\xi_{2}\in(\zeta,\infty).

We can now derive a system of ODEs satisfied by the functions in (7.17) and (7.18).

Let q±,jq_{\pm,j} and ϕj\phi_{j} be the values of Q±,jQ_{\pm,j} and Φj\Phi_{j} at ξ=ζ\xi=\zeta respectively and let the function Qj\mathcal{Q}_{j} be Qj=q+,j−q−,j\mathcal{Q}_{j}=q_{+,j}-q_{-,j}. Then functions u±,jku_{\pm,jk}, q±,jq_{\pm,j} and Qj\mathcal{Q}_{j} satisfy the following differential equations.

where W(f,g)W(f,g) is the Wronskian W(f,g)=fg′−gf′W(f,g)=fg^{\prime}-gf^{\prime}.

First by using (7.25) and (7.19), one can show as in , that, the derivatives of the u±,jku_{\pm,jk} are given by

where the prime denotes derivative of ζ\zeta. By eliminating u−,j1u_{-,j1} from the second equation, we obtain the differential equation for Qj\mathcal{Q}_{j} in (7.28). From (7.30), we see that u−,jku_{-,jk} are given by

Now by using the definition of Q+,jQ_{+,j}, we see that

This, together with (7.21), gives us the differential equation for q+,jq_{+,j}. ∎

This gives us the first set of differential equations. Let us now derive the second set of differential equations for the functions R±\mathcal{R}_{\pm} and Pj\mathcal{P}_{j}.

Let R0\mathcal{R}_{0} be R+−R−\mathcal{R}_{+}-\mathcal{R}_{-}. Then the functions R0\mathcal{R}_{0}, R+\mathcal{R}_{+}, P−,j\mathcal{P}_{-,j} and P0,j\mathcal{P}_{0,j} satisfy the following set of differential equations.

The proof is similar to (7.28). First, by (7.25), we can obtain the derivatives of Φk(ξ)\Phi_{k}(\xi) with respect to ζ\zeta.

From this, we obtain the derivatives of P±,0\mathcal{P}_{\pm,0}.

The differential equation for P±,0\mathcal{P}_{\pm,0} now follows from the fact that R0(ξ1,ξ2)R_{0}(\xi_{1},\xi_{2}) is symmetric with respect to the interchange of ξ1\xi_{1} and ξ2\xi_{2}.

From this and (7.21), we again have the following equations for R0\mathcal{R}_{0}.

The ODEs satisfied by the various functions can be further simplified. First, the function ϕ0=(I−K2,airyχ)Ai(ζ)\phi_{0}=(I-K_{2,airy}\chi)Ai(\zeta) is known to be the Hastings-McLeod solution of the Painlevé II equation (1.3) (See ).

The Wronskian of ϕ0/ψ\phi_{0}/\psi and ϕ1/ψ\phi_{1}/\psi can be written as

The function R0(ζ,ζ)R_{0}(\zeta,\zeta), again is known to be the logarithmic derivative of the Tracy-Widom distribution for the GUE . Therefore we have

To obtain ϕ1\phi_{1}, let us take the derivative of ϕ0\phi_{0} and use (7.26), then we have

As in the derivations of (7.29), we see that

Since (Φ0,Aiχ)=(Φ1,Aiχ)=0(\Phi_{0},Ai\chi)=(\Phi_{1},Ai\chi)=0 at ζ=∞\zeta=\infty, we obtain

To obtain ϕ2\phi_{2}, we use Ai′′(ξ)=ξAi(ξ)Ai^{\prime\prime}(\xi)=\xi Ai(\xi) to obtain

and let h⃗j\vec{h}_{j} be the vector h⃗j=(0,0,0,ϕjψ)T\vec{h}_{j}=\left(0,0,0,\frac{\phi_{j}}{\psi}\right)^{T} for j=0,1,2j=0,1,2 and h⃗j=0\vec{h}_{j}=0 for j=3j=3 and j=4j=4. Then the functions in (7.22) and (7.23) are given by

where v⃗j\vec{v}_{j} is the vector that satisfies the linear system of ODEs

These functions can also be characterized using the connection between Fredholm determinants and Riemann-Hilbert problems. We will outline this connection in Appendix B.

Appendix: A proof of the j.p.d.f. formula using Zonal polynomials

We present here a simpler algebraic proof of Theorem 2.1 using Zonal polynomials. Zonal polynomials are introduced by James and Hua independently. They are polynomials with matrix argument that depend on an index pp which is a partition of an integer kk. The real Zonal polynomials Zp(X)Z_{p}(X) take arguments in symmetric matrices and are homogenous polynomials in the eigenvalues of its matrix argument XX. We shall not go into the details of their definitions, but only state the important properties of these polynomials that is relevant to our proof. Readers who are interested can refer to the excellent references of , and .

Let pp be a partition of an integer kk and let l(p)l(p) be the length of the partition. We will use p⊢kp\vdash k to indicate that pp is a partition of kk. Let XX and YY be N×NN\times N symmetric matrices and xix_{i}, yiy_{i} their eigenvalues. Given a partition p=(p1,…,pl(p))p=(p_{1},\ldots,p_{l(p)}) of the integer kk, we will order the parts pip_{i} such that if i<ji<j, then pi>pjp_{i}>p_{j}. If we have 2 partitions pp and p′=(p1′,…,pl(p′)′)p^{\prime}=(p^{\prime}_{1},\ldots,p_{l(p^{\prime})}^{\prime}), then we say that p<p′p<p^{\prime} if there exists an index jj such that pi=pi′p_{i}=p_{i}^{\prime} for i<ji<j and pj<pj′p_{j}<p_{j}^{\prime}. Let the monomial xpx^{p} be x1p1…xpl(p)pl(p)x_{1}^{p_{1}}\ldots x_{p_{l(p)}}^{p_{l(p)}}, we say that xp′x^{p^{\prime}} is of a higher weight than xpx^{p} if p′>pp^{\prime}>p. Then the Zonal polynomial Zp(X)Z_{p}(X) is a homogenous polynomial of degree kk in the eigenvalues xjx_{j} with the highest weight term being xpx^{p}. It has the following properties.

These properties can be found in the references , and . Another important property is the following generating function formula for the Zonal polynomials, which can be found in and .

where dpd_{p} are constants. In particular, if (k)(k) is the partition of kk with length 1, that is, (k)=(k,0,…,0)(k)=(k,0,\ldots,0), then the constant d(k)d_{(k)} is given by

For the rank 1 spiked model, let us consider the case where all but one yjy_{j} is zero and denote the non-zero eigenvalue by yy. Then from the fact that the highest weight term in Zp(Y)Z_{p}(Y) is y1p1…ypl(p)pl(p)y_{1}^{p_{1}}\ldots y_{p_{l(p)}}^{p_{l(p)}}, we see that the only non-zero Zp(Y)Z_{p}(Y) is Z(k)(Y)Z_{(k)}(Y), which by the first equation in (A.1), is simply yky^{k}. Therefore the formulae in (A.1) and (A.2) are greatly simplified in this case.

By using the generating function formula, we see that Z(k)(IN)Z_{(k)}(I_{N}) is given by

By taking θ=12t\theta=\frac{1}{2t} in the second equation of (A.3), we see that

by taking residue at ∞\infty, which is the t−1t^{-1} coefficient in the following expansion

By taking y=τ2(1+τ)y=\frac{\tau}{2(1+\tau)}, this proves Theorem 2.1. There also exist complex and quarternionic Zonal polynomials Cp(X)C_{p}(X) and Qp(X)Q_{p}(X) which satisfy the followings instead.

Then by following the same argument as in the real case, we can write down the following integral formulae for rank one perturbations of the complex and quarternionic cases.

Appendix B: Connection to Riemann-Hilbert problem

Then the vectors FiF_{i} with entries FijF_{ij} in (7.6) are given by Y+(ξ)fijY_{+}(\xi)f_{ij}.

This Riemann-Hilbert problem can be connected to the Riemann-Hilbert problem of the Painlevé II equation. We will now outline this connection. For more details, please see . Let A(ξ)A(\xi) be the matrix in Lemma 6.19. Multiplying the solution YY of (A.1) by AA on the right and then deform the regions suitably will transform the Riemann-Hilbert problem (A.1) into the following Riemann-Hilbert problem.

where the contour Σ\Sigma is the union of

The contours in Σ\Sigma are all pointing towards ζ\zeta. The jump matrix JXJ_{X} is given by

Note the difference between our Riemann-Hilbert problem (A.2) and the one given in (2.11-15) of . In (A.2), as ξ→∞\xi\rightarrow\infty, the next to the leading order term is of order ξ−1\xi^{-1} smaller than the leading order term. This is due to the asymptotic behavior of the Airy functions in the matrix AA. As a result, our Riemann-Hilbert problem (A.2) will be uniquely solvable. This is important for us to keep track of the functions Φ0\Phi_{0} and Φ1\Phi_{1} that appears in the resolvent. In , it was shown that the Riemann-Hilbert problem (A.2) can be solved by using the monodromy problem associating with the Painlevé II equation. Let ΣΨ\Sigma_{\Psi} be the union of the contours

and let S±S_{\pm}, S1S_{1} and S2S_{2} be the regions

Then Ψ(ξ,v)\Psi(\xi,v) is the solution to the following monodromy problem of the Painlevé II equation.

where the contours are all pointing towards infinity. The matrix Ψ\Psi also satisfies the Lax equation for the Painlevé II equation.

where q(v)q(v) is related to the Hastings-McLeod solution of Painlevé II by (see (1.47) of )

By using the Lax equations (A.5) and the behavior of Ψ\Psi at ξ→∞\xi\rightarrow\infty, one can check that the next to the leading term Ψ∞\Psi_{\infty} in the expansion in (A.4) is given by

The authors in then showed that the solution to the Riemann-Hilbert problem (A.2) is given by

for some hh independent on ξ\xi. The function h(ζ)h(\zeta) is determined by making sure that the next to the leading order term in XX is of order indicated by (A.2). By using (A.7), one can check that the appropriate choice of hh in this case is given by h=−qh=-q. The properties of the Riemann-Hilbert problem in (A.4) is studied very thoroughly in , and these properties will hopefully be useful in the characterization of the functions in (7.22) and (7.23).

References