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J. Phys. A: Math. Theor. 40 No 36 (7 September 2007) F849-F855
doi:10.1088/1751-8113/40/36/F01
PII: S1751-8113(07)55391-6

FAST TRACK COMMUNICATION

A note on the Pfaffian integration theorem

Alexei Borodin1 and Eugene Kanzieper2

1 Department of Mathematics, California Institute of Technology, CA 91125, USA
2 Department of Applied Mathematics, H.I.T.–Holon Institute of Technology, Holon 58102, Israel

E-mail: borodin@caltech.edu and eugene.kanzieper@weizmann.ac.il

Received 18 July 2007, in final form 31 July 2007
Published 21 August 2007

Abstract. Two alternative, fairly compact proofs are presented of the Pfaffian integration theorem that surfaced in the recent studies of spectral properties of Ginibre's Orthogonal Ensemble. The first proof is based on a concept of the Fredholm Pfaffian; the second proof is purely linear algebraic.

PACS numbers: 02.10.Yn, 02.50.–r, 05.40.–a

1. Introduction

In the recent studies of spectral properties of Ginibre's orthogonal ensemble (Ginibre 1965) of real asymmetric random matricesNote1, the following theorem was presented by Kanzieper and Akemann (2005) and Akemann and Kanzieper (2007):

Pfaffian integration theorem. Let π(dz) be an arbitrary measure on z\in {\bb C} with finite moments. Define the function Q_n(z,w) = {\underline {\bm q}}(z) {{\bm \mu}} {\underline {\bm q}}^{\rm T}(w) in terms of the vector {\underline {\bm q}}(z) = (q_0(z), \ldots, q_{n-1}(z)) composed of arbitrary polynomials qj(z) of the jth order, and of an n × n antisymmetric matrix μ. Then

\fl
\frac 1{\ell!}\prod_{j=1}^\ell \int_{ {\bb C}} \pi({\rm d}z_j) {\rm pf } \left[
\begin{array}{@{}cc@{}}
Q_{n}(z_i, z_j) & Q_{n}(z_i, {\bar z}_j) \\ \ms
Q_{n}({\bar z}_i, z_j) & Q_{n}({\bar z}_i, {\bar z}_j)
\end{array}
\right]_{1\le i,j \le \ell} = e_\ell\left( \frac{1}{2} {\rm tr}( {{\bm \upsilon}}^1),\ldots,\frac{1}{2} {\rm tr} ({{\bm \upsilon}}^\ell) \right), \nonumber

where e(p1,  ..., p) are the elementary symmetric functionsNote2 written as polynomials of the power sums, and n × n matrix [b.upsi] is [b.upsi]  =  μ g with

{{\bm g}} = \int_{\bb C} \pi({\rm d}z) ({\underline {\bm q}}^{\rm T}(\bar z) {\underline {\bm q}}(z) - {\underline {\bm q}}^{\rm T}(z) {\underline {\bm q}}(\bar{z})). \nonumber

This theorem has been a key ingredient of the recent calculation (Kanzieper and Akemann 2005, Akemann and Kanzieper 2007) of the probability pn,k to find exactly k real eigenvalues in the spectra of n × n real asymmetric random matrices drawn from Ginibre's orthogonal ensemble. An earlier attempt to address the same problem is due to Edelman (1997).

Remark 1.1. The explicit form of e(p1,  ..., p) is well known (see, e.g., Macdonald 1998):

Equation (1.1)

The notation \blambda = \big(\ell_1^{\sigma_1},\ldots, \ell_g^{\sigma_g}\big) stands for the frequency representation of the partition [b.lambda] of the size |[b.lambda]|  =  ℓ. It implies that the part ℓj appears σj times so that ℓ  =  ∑gj = 1jσj, where g is the number of nonzero parts of the partition.

An immediate corollary of equation (1.1) is the identity

Equation (1.2)

Remark 1.2. The Pfaffian integration theorem can be viewed as a generalization of the Dyson integration theorem (Dyson 1970, Mahoux and Mehta 1991) for the case where the quaternion kernel {\bm {\cal Q}}_n(z,w) represented by the 2 × 2 matrixNote3

\Theta[{\bm {\cal Q}}_n(z,w)] = {\skew3\tilde{\bm J}}^{-1} \left(
\begin{array}{@{}cc@{}}
Q_{n}(z, w) & Q_{n}(z, {\bar w}) \\
Q_{n}({\bar z}, w) & Q_{n}({\bar z}, {\bar w})
\end{array}
\right) \nonumber

does not satisfy the projection property

\int_{{\bb C}} {\rm d}\pi(w) {\bm {\cal Q}}_n(z,w) {\bm {\cal Q}}_n(w,z^\prime) = {\bm {\cal Q}}_n(z,z^\prime). \nonumber

The original proof (Akemann and Kanzieper 2007) of the theorem involved an intricate topological interpretation of the ordered Pfaffian expansion combined with the term-by-term integration that spanned dozens of pages. In the present contribution, we provide two alternative, concise proofs of slight variations of the Pfaffian integration theorem. They are formulated in the form of the two theorems and represent the main result of our note.

Theorem 1. Let (X, m) be a measure space, and the vectors {{\underline{\bm \varphi}^+}}(x) and {{\underline{\bm \varphi}^-}}(x) be composed of measurable functions {{\underline{\bm \varphi}^\pm}}(x)=\big(\varphi^{\pm}_0(x), \ldots, \varphi^{\pm}_{n-1}(x)\big) from X to {\bb C} . Define the functions

\Phi_n^{\pm \pm}(x,y) = {{\underline{\bm \varphi}^\pm}}(x) {{\bm {\mu}}} {{\underline{\bm \varphi}}}^{\pm {\rm T}}(y), \nonumber

where μ is an n × n antisymmetric matrix. ThenNote4

Equation (1.3)

where the n × n matrix [b.upsi] is [b.upsi]  =  μ g with

Equation (1.4)

Theorem 2. In the notation of theorem 1, assume that the matrix μ is invertible (hence, n is even). Then

Equation (1.5)

Remark 1.3. The equivalence of theorems 1 and 2 is easily established. Indeed, multiplying both sides of equation (1.3) by τ and summing up over ℓ from 0 to ∞ with the help of equation (1.2), one finds that the right-hand side turns into

\exp\left(\frac{1}{2}\sum_{j=1}^\infty (-1)^{j-1} \tau^j\frac{{\rm tr} ({\bm \upsilon}^j)}{j} \right)=\sqrt{\det ({\bm I}+\tau{\bm \upsilon})}={\rm pf }{{\bm \mu}}\cdot{\rm pf }[ {{\bm \mu}}^{-1 {\rm T}}-\tau {\bm g}],

given that μ is invertible. This proves the equivalence for invertible (nondegenerate) μ. Theorem 1 with degenerate μ of even size follows by the limit transition, and decreasing the size n by 1 is achieved by setting varphi±n–1 ≡ 0 and nullifying the last, nth, row and column in the matrix μ.

2. Fredholm Pfaffian proof of theorem 1

For \ell \in {\bb Z}^+ , define the infinite sequence

Equation (2.1)

supplemented by σ0(n)  =  1, and consider the series

Equation (2.2)

By definition (equation (A.3)) introduced by Rains (2000), the function {\cal S}(\tau;n) is the Fredholm Pfaffian on the measure space (X, m)

Equation (2.3)

(See appendix for the matrix notation used.) Here, [b.Phi]n is the 2 × 2 matrix kernel

Equation (2.4)

that can also be written as

Equation (2.5)

where the vector {\underline {\bm \psi}}^{\pm}(x) is {\underline {\bm \psi}}^{\pm}(x) = {\underline {\bm \varphi}}^{\pm}(x) {\bm \mu}^{\rm T} .

The matrix I – τ J[b.Phi]n appearing under the sign of the Fredholm determinant can be represented as I  +  A B with

Equation (2.6)

Equation (2.7)

Following Tracy and Widom (1998), one observes the `needlessly fancy' general relation det[ I  +  A B]  =  det[ I  +  B A] that holds for arbitrary Hilbert–Schmidt operators A and B. They may act between different spaces as long as the products make sense. In the present context, det[ I  +  A B] is the Fredholm determinant detX[ I  +  A B] whilst the determinant det[ I  +  B A] is that of the n × n matrix

Equation (2.8)

where [b.upsi]  =  µ g with g defined by equation (1.4).

The above calculation allows us to write down the Fredholm Pfaffian {\cal S}(\tau;n) in the form

Equation (2.9)

Identity equation (1.2) concludes the proof.

3. Linear-algebraic proof of theorem 2

A linear-algebraic proof of theorem 2 is based on the works by Ishikawa and Wakayama (1995, 2000) and de Bruijn (1955) as formulated in sections 3.1 and 3.2. Section 3.3 contains a proof of theorem 2.

3.1.  Minor summation formulae and identities by Ishikawa and Wakayama

Let T be any M × N matrix, and let [m] denote the set {1, 2,  ..., m} for a positive integer m \in {\bb Z}^+ . For n-element subsets I  =  {i1 < ··· < in} ⊆ [M] and J  =  {j1 < ··· < jn} ⊆ [N] of row and column indices, let {\boldsymbol T}^I_J={\boldsymbol T}^{i_1\cdots i_n}_{j_1\cdots j_n} denote the submatrix of T obtained by picking up the rows and columns indexed by I and J. In this notation, the following three lemmas holdNote5.

Lemma 1 (Ishikawa and Wakayama 1995). Let MN and assume M is even. For any M × N matrix A and any N × N antisymmetric matrix B, one has

Equation (3.1)

Lemma 2 (Ishikawa and Wakayama 2000). Let A be an N × N invertible antisymmetric matrix. Then, for any I ⊆ [N], one has

Equation (3.2)

where \overline{I}\subseteq &N; stands for the complementary of I, and |I| denotes the sum of the elements of I, |I|  =  ∑i inI i.

Lemma 3 (Ishikawa and Wakayama 2000). Let A and B be N × N antisymmetric matrices. Then

Equation (3.3)

Here, lfloornrfloor denotes the integer part of n.

In what follows, we will need the following corollary.

Corollary 1. Let A and B be N × N antisymmetric matrices, and A is invertible. Then

Equation (3.4)

Proof. Using lemma 3 and lemma 2 (in this order), we write down

Equation (3.5)

This concludes the proof.        square

3.2.  de Bruijn integration formula

Lemma 4 (de Bruijn 1955). Let (X, m) be a measure space, and the vectors {{\underline{\bm \varphi}^+}}(x) and {{\underline{\bm \varphi}^-}}(x) be composed of measurable functions {{\underline{\bm \varphi}^\pm}}(x)= \big(\varphi^{\pm}_0(x), \ldots, \varphi^{\pm}_{2\ell-1}(x)\big) from X to {\bb C} . Then

\prod_{j=1}^\ell \int_X m({\rm d}x_j) \det \left[
\begin{array}{@{}c@{}}
\varphi_j^{+}(x_i) \\ \ms
\varphi_j^{-}(x_i)
\end{array}
\right]_{0 \le i \le 2\ell-1, 1\le j\le \ell} =\ell! {\rm pf}\left[{\boldsymbol g}^{\rm T}\right],

where the 2ℓ × 2ℓ matrix g isNote6

{{\bm g}} = \int_{X} m({\rm d}x) ({\underline {\bm \varphi}^{- {\rm T}}}(x) {\underline {\bm \varphi}^+}(x) - {\underline {\bm \varphi}}^{+ \rm T}(x) {\underline {\bm \varphi}}^{-}(x)). \nonumber

3.3.  Proof of theorem 2

In the notation of theorem 1, let us set A to be the 2ℓ × n matrix

Equation (3.6)

and identify B with the n × n matrix μ,

Equation (3.7)

Noting that

Equation (3.8)

we make use of the lhs of lemma 1, to write down the expansion

Equation (3.9)

Consequently, the lhs of equation (1.5) reduces to (note that n is even by the hypothesis)

Equation (3.10)

Here, we have used lemma 3. By corollary 1, the rhs of equation (3.10) is equivalent to

Equation (3.11)

This concludes the proof.

Acknowledgments

EK is grateful to G Akemann, a joint work with whom on the integrable structure of Ginibre's Orthogonal Ensemble has triggered this study. AB was partially supported by the NSF grants DMS-0402047 and DMS-0707163. EK acknowledges a partial support by the Israel Science Foundation through the grant no 286/04.

Appendix. The Fredholm Pfaffian

Let K(x, y) be a 2 × 2 matrix kernel

Equation (A.1)

which is antisymmetric under the change of its arguments, K(x, y)  =  – KT(y, x), and yet another 2 × 2 matrix kernel J(x, y) be

Equation (A.2)

(i)  

The Fredholm Pfaffian pfX[ J  +  K] on the measure space (X, m) is defined via the series (Rains 2000)

Equation (A.3)

(ii)  

A more familiar Fredholm determinant detX[I  +  K] of a scalar kernel K,

Equation (A.4)

appears to be a particular case of the Fredholm Pfaffian since

Equation (A.5)

Here, ε is any antisymmetric scalar kernel.

(iii)  

The connection between the Fredholm Pfaffian and Fredholm determinant is given by

Equation (A.6)

where I is the 2 × 2 matrix kernel

Equation (A.7)

References
[1] 
Akemann G and Kanzieper E 2007 Integrable structure of Ginibre's ensemble of real random matrices and a Pfaffian integration theorem Preprint math-ph/0703019  (J. Stat. Phys. submitted)
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[2] 
de Bruijn N G 1955 On some multiple integrals involving determinants J. Indian Math. Soc. 19 133 
[3] 
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Edelman A 1997 The probability that a random real Gaussian matrix has k real eigenvalues, related distributions, and the circular law J. Multivar. Anal. 60 203 
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Kanzieper E and Akemann G 2005 Statistics of real eigenvalues in Ginibre's ensemble of random real matrices Phys. Rev. Lett. 95 230201 
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Notes

Note1
 For a discussion of physical applications of Ginibre's random matrices, the reader is referred to the detailed paper by Akemann and Kanzieper (2007).
Note2
 Up to a factorial prefactor, the elementary symmetric functions e(p1,  ..., p) coincide with the zonal polynomials Z_{(1^\ell)}(p_1,\ldots, p_\ell)=\ell! e_\ell(p_1,\ldots, p_\ell) appearing in the original formulation of the theorem.
Note3
 See appendix for the notation.
Note4
 In what follows, we assume that our measures are such that all integrals are finite.
Note5
 Lemma 2 is a reformulation of theorem 3.1 by Ishikawa and Wakayama (2000).
Note6
 Compare to equation (1.4).



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