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PETER 2 N ∂θ T ∂ = with , 2 j 2 0 11 h rbblt est ucin(D)o h ntcircle unit the on (PDF) function density probability the , I + N U o oedtisadmotivations. and details more for ] 1 55,1A5 33E20. 15A15, 15B52, ≤ ( β 4 1. ⊗ N j Starting with (1.1) in the cases β = 1, 2 and 4, a different generalisation to regarding β as continuous is to consider a two-component interpolation between β =1 and 4. This is motivated by the fact that the logarithmic potential is the solution of the Poisson equation in two-dimensions, allowing the particles in the classical statistical mechanical interpretation of (1.1) to be thought of as charges. With the inverse temperature fixed to unity, the particles in (1.1) for β = 1 have charge +1, while those in (1.1) for β =4 have charge +2 — the pair potential between particles of charges q and q confined to the unit circle embedded in two-dimensions is q q log eiθ1 eiθ2 . 1 2 − 1 2 | − | A natural two-component generalisation is thus the PDF proportional to [15] N1 N2 eiθk eiθj eiφα eiφβ 4 eiθj eiφα 2, (1.3) | − | | − | | − | 1 2 j=1 α=1 1≤j N1 particles of charge +1 and N2 particles of charge +2. Since the charges are of the same sign, this two-component log-gas may also be referred to as a two-component plasma. It is immediate that when N2 =0 (resp. N1 =0), this model corresponds to (1.1) with β =1 (resp. β =4). It is furthermore the case that (1.3) corresponds to the ground state wave function of a two-component generalisation of the quantum many body Hamiltonian (1.2) [16]. Explicit evaluations of the partition function and the two-point charge–charge correlation func- tions corresponding to (1.3) were given in [15]. These explicit formulas allowed the free energy in the thermodynamic limit to be computed, as well as the evaluation of the bulk scaling limit of the two-point charge–charge correlation functions; see also [17]. Subsequently, it was found that the general (k1, k2)-point correlation function could be expressed as a quaternion determinant (or equivalently a Pfaffian) [18, Equation (6.168)]. Well established theory relating to the correlation functions for (1.1) with β = 1 and 4 [18, §6] (see also Section 1.2 below) implies that there is a family of skew orthogonal polynomials underpinning this result. Appreciating this point, the authors of [33] considered a variant of (1.3) on the real line specified by the Boltzmann factor N1 N2 α α β β 4 α β 2e−V (αj )−2V (βk) (1.4) | k − j | | k − j | | j − k| 1 2 j=1 1≤j 1.2. Skew orthogonal polynomials arising from log-gases. Since this paper is about the skew orthogonal polynomials arising from two-component log-gases (1.4), it is appropriate to first revise how skew orthogonal polynomials appear in the corresponding one-component cases N1 =0 and N2 = 0. In these cases, (1.4) is proportional to the eigenvalue PDF for invariant ensembles of real symmetric matrices (N2 = 0), and self dual Hermitian matrices (N1 = 0). With this interpretation, the skew orthogonal polynomials most simply occur as the averaged characteristic CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 3 polynomials [29, §5]. For β =1, the monic skew orthogonal polynomials p(1)(x) ∞ are given by { j }j=0 (up to a shift with arbitrary constant cn) p(1)(x)= det(x M) (1), p(1) (x)= (x + TrM + c ) det(x M) (1), (1.5) 2n h − i2n 2n+1 h n − i2n while for β =4, the monic skew orthogonal polynomials p(4)(x) ∞ are given by { j }j=0 p(4)(x)= det(x M) (4), p(4) (x)= (x + TrM + c ) det(x M) (4). (1.6) 2n h − in 2n+1 h n − in The label in these latter averages relates to the size of M regarded as having quaternion entries. In practice each quaternion is represented as a particular 2 2 complex matrix (see e.g. [18, §1.3.2]), × so the sizes are consistent with the β = 1 case. The quantities in these averages depend only on the eigenvalues of M. Consequently, they can each be written in terms of integrals over the corresponding eigenvalue PDFs. Thus, 2n (1) 1 −V (xl) p2n (x)= xk xj (x xl)e dxl, CN,1 In | − | − Z 1≤j 1.3. Main results. The family of skew orthogonal polynomials corresponding to the Boltzmann factor (1.4) is skew orthogonal with respect to a particular skew symmetric inner product , 1 2 , h· ·iX,V ,V which is a linear combination of the , 1 and , 2 . Since in [33] it has been shown that h· ·i1,V h· ·i4,V for the Gaussian weight, the skew orthogonal polynomials with , 1 2 can be written as a h· ·iX,V ,V linear combination of Hermite polynomials with coefficients expressed by Laguerre polynomials (the latter have argument in terms of the fugacity—below a grand canonical formalism will be introduced), we pose the question as to whether all of the classical skew orthogonal polynomials under , 1 2 can be related to classical orthogonal polynomials. An affirmative answer is h· ·iX,V ,V given in Proposition 2.6, showing that classical skew orthogonal polynomials under , 1 2 can h· ·iX,V ,V be constructed from the classical orthogonal polynomials due to the Pearson equation. There are four cases to consider: the Gaussian, Laguerre, Jacobi and (generalised) Cauchy weight. We show that the hypergeometric orthogonal polynomials in the Askey-scheme appear when expressing the coefficients of the linear combination, extending the result of the Gaussian case for which the coefficients are given by Laguerre polynomials (i.e. 1F1 hypergeometric function). In particular, special attention is paid to the so-called generalised Cauchy weight in the form (1 ix)c(1 + ix)c¯ − with x R and c C. The model with the generalised Cauchy weight on the real line can be ∈ ∈ transformed into a generalised two-component log-gases with Jacobi weight on the unit circle under a stereographic projection, and therefore relates to the original work [15]. 2. Skew orthogonal polynomials arising from a solvable mixed charge model In this section, we present the general formalism showing how skew orthogonal polynomials enter into the computation of the partition function for the mixed charge model (1.4). As has been pointed out above, the Gaussian weight case has previously been considered in [33]; our formalism works for general classical weights. 2.1. A solvable mixed charge model. Let us consider a statistical mechanical system of par- ticles corresponding to two-dimensional charges (logarithmic potential) confined to a line. Specif- ically, let there be L particles of charge +1 and M particles of charge +2, so that the total charge is L +2M = K. For convenience, we will assume that the total charge K = 2N is even, which implies L is even too. The configuration space ξ of this 1-dimensional system is a subspace of RL RM , defined as ξ = (ξ ; ξ ) = (α , , α ; β , ,β ), ξ RL, ξ RM , where α L × { 1 2 1 ··· L 1 ··· M 1 ∈ 2 ∈ } { i}i=1 and β M represent the locations of the charge +1 and +2 particles respectively. The particles { j}j=1 are each to subject to an external confining potential. The total energy of this model is given by E(ξ ; ξ )= log α α +4 log β β 1 2 | k − j | | k − j | 1≤j The partition function ZL,M of a fixed pair of species numbers (L,M) is specified by 1 −E(ξ1;ξ2) L M ZL,M = e dµ (α)dµ (β) L!M! RL RM Z × CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 5 with Boltzmann factor L M e−E(ξ1;ξ2) = α α β β 4 α β 2e−V1(αj )−2V2(βk) | k − j | | k − j | | j − k| 1≤j The second line in (2.1) follows from a confluent form of the Vandermonde determinant identity; see [15]. To most clearly exhibit solvable structures, we do not consider the partition function directly, but rather first form a particular grand canonical ensemble, obtained by simultaneously considering all systems with species numbers L and M such that L +2M = 2N. To distinguish the species number making up the grand canonical ensemble, we introduce a fugacity (generating function parameter) X in the specification of the corresponding grand canonical partition function, L L X −E(ξ1;ξ2) L M ZN (X)= X ZL,M = e dµ (α)dµ (β), L!M! RL×RM XhAi XhAi Z where here = (L,M) L +2M =2N,L,M Z . hAi { | ∈ ≥0} First we will demonstrate that the partition function ZN (X) has a Pfaffian representation. Proposition 2.1. The partition function ZN (X) can be written as a Pfaffian N 2N−1 ZN (X)=2 Pf(mi,j (X))i,j=0 , (2.2) where the moments mi,j (X) are defined as 2 X i j −V1(y)−V1(z) j i i+j−1 −2V2(y) mi,j (X)= y z sgn(z y)e dµ(y)dµ(z)+ − y e dµ(y). 2 R R − 2 R Z × Z (2.3) Proof. We begin by performing a Laplace expansion (see e.g. [38, §3.3]) of the confluent Vander- monde determinant in (2.1) to express the determinant as sums in terms of determinants of species α and β respectively, −E(ξ1;ξ2) σ(η) −V1(αj ) e = sgnσ det αj e · j, η = 1, ··· , L. σ X ′ ′ ′ ′ σ (η ) −V2(β ′ ) ′ ′ σ (η )−1 −V2(β ′ ) ′ j ′ j ′ det βj e , σ (η )βj e j = 1, ··· ,M, , × ′ ··· η = 1, , 2M where σ is injective map from 1, ,L 1, , 2N satisfying σ(1) < < σ(L) and the { ··· } 7→ { ··· } ··· image of σ′ is Im(σ′) = 1, , 2N Im(σ) satisfying σ′(1) < < σ′(2M). Moreover, the sum { ··· }\ ··· L σ represents the sum of all the possibilities of L integer partitions, contributing a factor C2N . Since the determinant has been expanded into terms involving species α and β independently, P we can similarly factor the integrations L L X −E(ξ1;ξ2) L M X σ(j) −V1(αj ) L e dµ (α)dµ (β)= sgnσ det αj e dµ (α) L!M! RL RM · L! RL × σ Z X Z 1 ′ ′ ′ ′ σ (j ) −V2(β j′ ) ′ ′ σ (j )−1 − V2(βj′ ) M det βj′ e , σ (j )βj′ e dµ (β). × M! RM Z 6 PETER J. FORRESTER AND SHI-HAO LI By making use of integration formulas due to de Bruijn [7] for both factors, the right hand side of the above equation is equal to 2 L 2M sgnσ Pf(X m˜ ) Pf(ˆm ′ ′ ) , · σ(i),σ(j) i,j=1 σ (i),σ (j) i,j=1 σ X where i−1 j−1 −V1(y)−V1(z) m˜ i,j = y z sgn(z y)e dµ(y)dµ(z), R R − Z × i+j−3 −2V2(y) mˆ i,j = (j i) y e dµ(y). − R Z We can now make use of [36, Lemma 4.2] to sum the Pfaffian according to 2 L 2M 2 2N sgnσ Pf(X m˜ ) Pf(ˆm ′ ′ ) = Pf(X m˜ +m ˆ ) . · σ(i),σ(j) i,j=1 σ (i),σ (j) i,j=1 i,j i,j i,j=1 σ XhAi X 2 By denoting 2mi+1,j+1(X)= X m˜ i,j +m ˆ i,j , we complete the proof. 2.2. Skew orthogonal polynomials arising from the solvable mixed charge model. In keeping with Proposition 2.1, we introduce the skew symmetric inner product , 1 2 : C[z] C[z] C h· ·iX,V ,V × → i j 2 i j i j (z , z ) m (X)= X z ,z 1 + z ,z 2 . 7→ i,j h i1,V h i4,V Here, with weight function V , V specified in (2.3), the skew inner products , with β =1, 2, 4 1 2 h· ·iβ are defined by 1 −V (y)−V (z) φ(z), ψ(z) 1, V = φ(y)ψ(z)sgn(z y)e dµ(y)dµ(z), h i 2 R R − Z × −2V (z) φ(z), ψ(z) 2, V = φ(z)ψ(z)e dµ(z), h i R Z 1 −2V (z) φ(z), ψ(z) 4, V = (φ(z)∂zψ(z) ∂zφ(z)ψ(z))e dµ(z). h i 2 R − Z Following the procedure of skew symmetric tri-diagonalisation [2, 20], we know that the skew 2N−1 −1 −⊤ symmetric moment matrix M := (mi,j (X))i,j=0 can be decomposed into M = S JS , where S is a lower triangular matrix with diagonals 1 and J is a block matrix of the form 0 u0 0 uN−1 τ2n+2 2n−1 J = diag , , , un = , τ2n = Pf(mi,j )i,j=0 (2.4) u 0 ··· u 0 τ2n ( − 0 ! − N−1 !) with τ = 1. Due to the decomposition, we can introduce a family of polynomials Q (z) 2N−1 0 { n }n=0 such that Q (z) = (Sχ(z)) , χ(z) = (z0,z1, ,z2N−1)⊤, n n+1 ··· where (Sχ(z))n+1 denotes the (n + 1)-th component of vector (Sχ(z)). These polynomials skew diagonalise , 1 2 . h· ·iX,V ,V Proposition 2.2. The family of polynomials Q (z) 2N−1 are skew orthogonal with respect to the { n }n=0 inner product , 1 2 . In other words, we have h· ·iX,V ,V Q2n(z),Q2m+1(z) X,V1,V2 = unδn,m, h i (2.5) Q (z),Q (z) 1 2 = Q (z),Q (z) 1 2 =0 h 2m 2n iX,V ,V h 2m+1 2n+1 iX,V ,V CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 7 for n, m =0, 1, ,N 1. ··· − Proof. By denoting Q(z) = (Q (z), ,Q (z))⊤ = Sχ(z), one can easily find 0 ··· 2N−1 ⊤ ⊤ ⊤ ⊤ Q(z),Q (z) 1 2 = S χ(z),χ (z) 1 2 S = SMS = J. h iX,V ,V h iX,V ,V Remark 2.3. Since the skew orthogonal relation (2.5) is equivalent to a linear system, one can obtain a Pfaffian form of the skew orthogonal polynomials following the procedure in [8, Section 2]. Since we mainly consider the relation between the skew orthogonal polynomials and orthogonal polynomials in this paper, we omit the Pfaffian forms here. The skew symmetric inner product defined in (2.3) is a linear combination of skew symmet- ric inner products induced by random matrices with orthogonal and symplectic invariance (i.e. β =1, 4 respectively). As is known from [1] , the skew orthogonal polynomials with β =1, 4 can be expressed as a linear combination of orthogonal polynomials in the classical cases (a precise meaning of ‘classical’ is given in the paragraph above Proposition 2.6). Therefore, we seek a rela- tionship between the skew orthogonal polynomials arising from (2.3) and orthogonal polynomials. Important for this purpose is the following proposition. Proposition 2.4. For specific coefficients ζ ∞ , if p (z) ∞ are monic polynomials satisfying { j }j=0 { j }j=0 (1) p (z),p (z) ζ p (z) 1 = hn δ , h 2m 2n+1 − n 2n−1 i1,V n,m p2m(z),p2n(z) 1,V1 = p2n+1(z) ζnp2n−1(z),p2m+1(z) ζmp2m−1(z) 1,V1 =0, h i h (4) − (4) − i (2.6) p2m(z),p2n+1(z) 4,V2 = h δn,m h δm−1,n, h i 2n − 2m−1 p (z),p (z) 2 = p (z),p (z) 2 =0, h 2m 2n i4,V h 2m+1 2n+1 i4,V then there exist a family of monic skew orthogonal polynomials Q (z) ∞ { j }j=0 m m 1 1 Q2m(z)= αkp2k(z),Q2m+1(z)= ξk(p2k+1(z) ζkp2k−1(z)), (2.7) αm ξm − Xk=0 Xk=0 2 skew orthogonal under the skew symmetric inner product , 1 2 = X , 1 + , 2 . h· ·iX,V ,V h· ·i1,V h· ·i4,V Moreover, the coefficients α ∞ and ξ ∞ satisfy the recurrence relations { j}j=0 { j }j=0 h(4) α X2h(1) + h(4) + ζ h(4) α + ζ h(4) α =0 (2.8a) 2j+1 j+1 − j 2j j 2j−1 j j 2j−2 j−1 ζ h(4)ξ X2h(1) + h(4) + ζ h(4) ξ + h(4) ξ =0 (2.8b) j+1 2j j+1 − j 2j j 2j−1 j 2j−1 j−1 with initial values α−1 = ξ−1 =0 and α0 = ξ0 =1. Proof. Since p (z), p (z) ζ p (z) ∞ form a basis of L2(dµ), we can write the monic { 2j 2j+1 − j 2j−1 }j=0 polynomials Q (z) ∞ as linear combinations of this basis { j }j=0 m m−1 Q (z)= α(m)p (z)+ β(m)(p (z) ζ p (z)), α(m) =1, (2.9a) 2m k 2k k 2k+1 − k 2k−1 m k=0 k=0 Xm X m Q (z)= ξ(m)(p (z) ζ p (z)) + η(m)p (z), ξ(m) =1. (2.9b) 2m+1 k 2k+1 − k 2k−1 k 2k m Xk=0 Xk=0 8 PETER J. FORRESTER AND SHI-HAO LI The skew orthogonal relations (2.5) can be written as 1 Q (z),p (z) ζ p (z) 1 2 =0, for j Q (z),p (z) 1 2 =0, for j m; (2.10b) h 2m 2j iX,V ,V ≤ Q (z),p (z) ζ p (z) 1 2 =0, for j Q (z),p (z) 1 2 =0, for j < m. (2.10d) h 2m+1 2j iX,V ,V From (2.9a) and (2.9b), the equation (2.10a) is equivalent to m (m) α p (z),p (z) ζ p (z) 1 2 =0, for j α−1 =0, α0 =1 (2.12) and m m−1 1 (m) Q2m(z)= αkp2k(z)+ βk (p2k+1(z) ζkp2k−1(z)). αm − Xk=0 Xk=0 Now substituting the above form of Q2m(z) into (2.10b), one can see m−1 β(m) p (z) ζ p (z),p (z) =0, k h 2k+1 − k 2k−1 2j iX,V Xk=0 which leads us to m−1 m−1 X2 β(m)h(1)δ β(m)(h(4)δ h(4) δ ) − k k k,j − k 2k k,j − 2j−1 j−1,k Xk=0 Xk=0 m−1 + β(m)ζ (h(4) δ h(4) δ )=0, for j m. k k 2k−2 k−1,j − 2j−1 k,j ≤ Xk=0 Taking j from m to 0 iteratively we find β(m) = = β(m) = 0. Therefore, from (2.10a) and m−1 ··· 0 (2.10b), we obtain m 1 Q2m(z)= αkp2k(z), αm kX=0 where α satisfy (2.8a) with initial values α =0 and α =1. { k} −1 0 1 For the third condition, the skew orthogonal relation only hold for j < m since we haven’t assume Q2m+1(z) is independent of Q2m(z) yet. CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 9 Now we turn to equations (2.10c) and (2.10d). First consider (2.10c). From (2.9a) and (2.9b), this is equivalent to m (m) η p (z),p (z) ζ p (z) 1 2 =0, for j < m. k h 2k 2j+1 − j 2j−1 iX,V ,V Xk=0 Again, by the use of conditions (2.6), one can show that this implies h(4) η(m) X2h(1) + h(4) + ζ h(4) η(m) + ζ h(4) η(m) =0, for j < m, 2j+1 j+1 − j 2j j 2j−1 j j 2j−2 j−1 demonstrating that η(m) admit the same recurrence relation with α(m) and therefore { j } { j } m Q (z)= ξ(m)(p (z) ζ p (z)) + c Q (z) 2m+1 k 2k+1 − k 2k−1 m 2m kX=0 with a constant cm. A basic property of skew orthogonal polynomials, is that the transformation Q (z) Q (z)+ c Q (z) does not change the skew orthogonality (this explains the 2m+1 7→ 2m+1 m 2m arbitrary constant cn in (1.5) and (1.6)), and therefore we are free to set cm =0, giving m Q (z)= ξ(m)(p (z) ζ p (z)). 2m+1 k 2k+1 − k 2k−1 kX=0 We now make use of (2.10d) by substituting this form to obtain m m m X2 ξ(m)h(1)δ ξ(m)(h(4)δ h(4) δ )+ ξ(m)ζ (h(4) δ h(4) δ )=0 − k k k,j − k 2k k,j − 2j−1 k,j−1 k k 2k−2 k−1,j − 2j−1 k,j Xk=0 Xk=0 Xk=0 (m) for j Corollary 2.5. We have j (4) −1 h2k−2 ξj = cj αj , where cj = ζk . (2.13) h(4) kY=1 2k−1 −1 ˆ Proof. Note that if we make the transformation of variables ξj = cj ξj , the recurrence relation (2.8b) reads (4) cj ˆ 2 (1) (4) (4) ˆ (4) cj ˆ ζj+1h2j ξj+1 X hj + h2j + ζj h2j−1 ξj + h2j−1 ξj−1 =0. cj+1 − cj−1 To be consistent with (2.8a), it is further required (4) cj (4) (4) cj (4) ζj+1h2j = h2j+1, h2j−1 = ζj h2j−2. cj+1 cj−1 Hence j (4) h2k−2 −1 cj = C ζk , and ξj = cj αj , h(4) kY=1 2k−1 for some constant C. By noting α0 = ξ0 =1, it follows that C =1, thus completing the proof. 10 PETER J. FORRESTER AND SHI-HAO LI The condition of proposition (2.4) is very general. Thus, starting with two arbitrary skew symmetric inner products , s1 and , s2 , if a family of (not necessarily orthogonal) polynomials ∞ h· ·i h· ·i pj(z) j=0 satisfy the condition (2.6), then we can define a new skew symmetric inner product { } 2 , = X , 1 + , 2 with corresponding skew orthogonal polynomials specified by (2.7), h· ·inew h· ·is h· ·is (2.8a) and (2.8b). The task then is to specify families of skew symmetric inner products and polynomials p (z) ∞ { j }j=0 satisfying (2.6). In fact we find that all of the classical monic orthogonal polynomials p (x) ∞ { j }j=0 with weight e−2V , characterised by the Pearson equation 2V ′(z)= g(z)/f(z) with deg g 1 and ≤ deg f 2, satisfy the condition (2.6) with ≤ 1 1 V = V + log f, V = V log f. (2.14) 1 2 2 − 2 It is remarkable that for the classical weights, the procedure to find the relations between β =1, 4 and β =2 is to construct a linear operator [1] f ′ g = f∂ + − A z 2 −1 such that φ, ψ 2,V = φ, ψ 1,V1 and φ, ψ 2,V = φ, ψ 4,V2 . In this case, the inner product h A i −h i h A i 2 −h 1 i , 1 2 can be constructed from the operator X + , but it needs more computations h· ·iX,V ,V A A which are not considered in this paper. Proposition 2.6. All classical orthogonal polynomials, in the sense of the requirement on the Pearson equation as specified above, satisfy (2.6), where the relations (2.14) are assumed. Proof. The proof of this claim is based on the Pearson equation. The first two relations have been demonstrated in [1]—the key idea is to use the Pearson pair (f,g) to find the skew orthogonal polynomials with β = 1; a detailed procedure can be found in the Appendix B. Moreover, the quantities ζ ∞ and h(1) ∞ are computed from the procedure. The last two relations can also { j }j=0 { j }j=0 be obtained from the Pearson pair. In [3], it has been demonstrated that the classical orthogonal polynomials p (z) ∞ which are characterised by the Pearson pair (f,g) must satisfy { n }n=0 ′ f(z)pn(z)= anpn+1(z)+ bnpn(z)+ cnpn−1(z), where a ∞ , b ∞ , c ∞ are three sequences independent of z. Therefore, one can obtain { n}n=0 { n}n=0 { n}n=0 p (z),p (z) 2 = p (z),p (z) 2 =0, h 2m 2n i4,V h 2m+1 2n+1 i4,V 1 ′ 1 ′ p (z),p (z) 2 = p (z),f(z)p (z) f(z)p (z),p (z) h 2m 2n+1 i4,V 2h 2m 2n+1 i2,V − 2h 2m 2n+1 i2,V 1 1 = (c h a h )δ (c h a h )δ , 2 2n+1 2n − 2n 2n+1 n,m − 2 2m 2m−1 − 2m−1 2m m,n+1 where h = p (z),p (z) . We complete the proof by defining h(4) = 1 (c h a h ). n h n n i2,V j 2 j+1 j − j j+1 In conclusion to this section, we demonstrate that the partition function ZN (X) in (2.2) can be calculated by use of the skew orthogonal polynomials constructed in Proposition 2.4, thus exhibiting the solvability of the model. To begin, note that N−1 N (2.2) N (2.4) N (2.5) N Z (X) = 2 τ = 2 u = 2 Q ,Q 1 2 . N 2N j h 2j 2j+1iX,V ,V j=0 j=1 Y Y CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 11 Substituting the skew orthogonal polynomials Q (z) ∞ in terms of orthogonal polynomials via { j }j=0 (2.7) shows N−1 N−1 j j N N 1 2 Q2j ,Q2j+1 X,V1,V2 =2 αk1 ξk2 p2k1 ,p2k2+1 ζk2 p2k2−1 X,V1,V2 . h i αj ξj h − i j=0 j=0 1 2 Y Y kX=0 kX=0 Making the use of (2.6), we see this is equal to j j j N−1 1 2N α ξ (X2h(1) + h(4) + ζ h(4) ) α ξ ζ h(4) α ξ h(4) . α ξ k k k 2k k 2k−1 − k−1 k k 2k−2 − k k−1 2k−1 j=0 j j ! Y Xk=0 Xk=1 Xk=1 By taking into account the recurrence relation (2.8a), we conclude N−1 N (4) ZN (X)=2 αN h2j+1. j=0 Y In the classical cases, h(4) ∞ are known normalisations, expressible in terms of quantities { j }j=0 relating to the corresponding orthogonal polynomials [1]. We will show below that in these cases αN , and thus the partition function, can be written in terms of hypergeometric orthogonal poly- nomials. Interestingly, this class of polynomials has appeared in a recent work in the moments of the spectral density for the classical weights with β =2 [10]. 3. The classical cases We know from Proposition 2.6 that the classical weights allow for a structured form of the skew orthogonal polynomials generated in terms of the classical orthogonal polynomials. Here we will show that the coefficients α ∞ and ξ ∞ can be expressed in terms of hypergeometric or- { j }j=0 { j }j=0 thogonal polynomials from the Askey-Wilson table. There are four classical weights: the Gaussian, Laguerre, Jacobi and generalised Cauchy. These will be considered in turn. 3.1. Gaussian case. The two-component plasma for mixed charges with Gaussian weight has already been considered in [33]. We restate the main results for the completeness of our work. It is a standard result that the monic Hermite polynomials p (z) ∞ satisfy the orthogonal relation { k }k=0 p (z),p (z) =2−k√πΓ(k + 1)δ , h k j i2,V k,j 2 where the weight function is given by e−2V (z) = e−z . From the weight function, we can compute the Pearson pair as (f,g)=(1, 2z), and therefore e−V1(z) = e−V2(z) = z2/2, meaning that the ex- ternal potentials of these two different particles are exactly the same. Moreover, from [1, Equation 3.2], we have −2n p ,p np 1 =2 √πΓ(2n + 1)δ , h 2m 2n+1 − 2n−1i1,V n,m and from the derivative formula ∂zpk(z)= kpk−1(z), one knows 1 1 p ,p 2 = (2n + 1) p ,p 2 (2m) p ,p 2 h 2m 2n+1i4,V 2 h 2m 2ni2,V − 2 h 2m−1 2n+1i2,V =2−2n−1√πΓ(2n + 2)δ 2−2m√πΓ(2m + 1)δ . n,m − m−1,n Therefore, the coefficients of the Hermite polynomials with regard to the relations (2.6) are (1) −2j (4) −j−1 ζj = j, hj =2 √πΓ(2j + 1), hj =2 √πΓ(j + 2). (3.1) 12 PETER J. FORRESTER AND SHI-HAO LI Substituting them into the recurrence relation (2.8a), one finds that the coefficients α satisfy { j } (2j + 2)(2j + 1)α 2(2X2 +4j + 1)α +4α =0, j+1 − j j−1 2j j! which, upon scaling αj =2 (2j)! αˆj , reduces to 1 1 (j +1)ˆα (X2 +2j + )ˆα + (j )ˆα =0. j+1 − 2 j − 2 j−1 This equation, in combination with the initial conditions (2.12), can be recognised as the three term recurrence satisfied by the Laguerre polynomials with parameter 1/2, and so αˆ = L−1/2( X2), − j j − where La (z) ∞ denotes the standard (not monic!) Laguerre polynomials with parameter a { n }n=0 through the orthogonal relation ∞ Γ(a + n + 1) La (z)La (z)zae−zdx = δ . n m Γ(n + 1) n,m Z0 Therefore, we can conclude that j! − 1 α =22j L 2 ( X2). j (2j)! j − With regard of the coefficients ξ ∞ , since { j }j=0 (4) −2j−1 −2j−2 (4) ζj+1h2j = (j + 1)2 √πΓ(2j +2)=2 √πΓ(2j +3)= h2j+1, one sees that α ∞ and ξ ∞ satisfy the same recurrence relation with same initial values. { j}j=0 { j}j=0 Therefore, j! − 1 α = ξ =22j L 2 ( X2), j j (2j!) j − as demonstrated in [33, Section 4]. 3.2. Laguerre case. The Laguerre case is to consider the weight function e−2V (z) = zae−z, supported on [0, ). The Pearson pair of the Laguerre weight is (f,g) = (z,z a), and therefore, ∞ − according to (2.14) the external potentials are e−V1(z) = z(a−1)/2e−z/2 and e−V2(z) = z(a+1)/2e−z/2. For the monic Laguerre polynomials 2 p(a)(z) ∞ , we have { k }k=0 p(a),p(a) = Γ(n + 1)Γ(n + a + 1)δ , h m n i2,V n,m d (3.2) p(a−1)(z)= p(a)(z)+ np(α) (z), p(a)(z)= np(a+1)(z). n n n−1 dx n n−1 From [1, Equation 3.6] or [30, Equation 4.31], one knows (a) (a) (a) p ,p 2n(2n + a)p 1 = 2Γ(2n + 1)Γ(2n + a + 1)δ . h 2m 2n+1 − 2n−1i1,V n,m Properties of the Laguerre polynomials (3.2) tell us (a) (a) 1 (a) (a+1) 1 (a+1) (a) p ,p 2 = (2n + 1) p ,p 2 (2m) p ,p 2 h 2m 2n+1i4,V 2 h 2m 2n+1 i2,V − 2 h 2m−1 2n i2,V 1 (a+1) (a+1) (a+1) 1 (a+1) (a+1) (a+1) = (2n + 1) p +2mp ,p 2 (2m) p ,p + (2n + 1)p 2 2 h 2m 2m−1 2n i2,V − 2 h 2m−1 2n+1 2n i2,V 1 1 = Γ(2n + 2)Γ(2n + a + 2)δ Γ(2m + 1)Γ(2m + a + 1)δ . 2 n,m − 2 m−1,n 2 (a) − k (a) The monic Laguerre polynomials are given in terms of the Laguerre polynomials by pk (z) = ( 1) k!Lk (z) CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 13 Therefore, the coefficients in (2.6) for the Laguerre case are 1 ζ =2j(2j + a), h(1) = 2Γ(2j + 1)Γ(2j + a + 1), h(4) = Γ(j + 2)Γ(j + a + 2). (3.3) j j j 2 Substituting in the recurrence relation (2.8a) shows (2j + 1)(2j + 2)(2j + a + 1)(2j + a + 2)αj+1 (4X2 + (2j + 1)(2j + a +1)+2j(2j + a))α + α =0. − j j−1 Scaling α = 1 αˆ gives that αˆ ∞ satisfy j (2j)! j { j }j=0 a a 1 1 a 1 a 1 (j + + 1)(j + + )ˆα X2 + (j + )(j + + )+ j(j + ) αˆ + j(j )ˆα =0. 2 2 2 j+1 − 2 2 2 2 j − 2 j−1 Together with the initial condition (2.12), we recognise this three term recurrence as that satisfied by a particular continuous dual Hahn polynomial [25, Section 1.3] a +1 1 αˆ = S˜ X2; , , 0 j j − 2 2 or hypergeometric function a+1 a+1 j, 2 X, 2 + X αˆj = 3F2 − a+2− a+1 1 . , ! 2 2 Hence, for the coefficients α ∞ we have { j }j=0 1 a +1 1 α = S˜ X2; , , 0 . j (2j)! j − 2 2 (4) (4) As for the Laguerre case we can check ζj+1h2j = h2j+1, and thus the recurrence relations of ξ ∞ are the same with α ∞ . Therefore, { j }j=0 { j}j=0 1 a +1 1 ξ = S˜ X2; , , 0 . j (2j)! j − 2 2 3.3. Jacobi case. The weight function in the Jacobi case is e−2V (z) = (1 z)a(1 + z)b supported − on the interval ( 1, 1). This is more general than the Gaussian and Laguerre weights, in the − sense that the latter can be obtained as limiting cases. For the Pearson pair, we have (f,g) = 1 z2, (a + b)z + (a b) , and therefore the external potentials are e−V1(z) = (1 z)(a−1)/2(1 + − − − z)(b−1)/2 and e−V2(z) = (1 z)(a+1)/2(1 + z)(b+1)/2. − The monic Jacobi polynomials p(a,b)(z) ∞ have the well known properties { k }k=0 (a,b) (a,b) (a,b) d (a,b) (a+1,b+1) pm ,pn 2,V = hn δn,m, pn (z)= npn−1 (z), h i dz (3.4) (a,b) (a+1,b+1) (a,b) (a+1,b+1) (a,b) (a+1,b+1) pn (z)= pn (z)+ µn pn−1 (z)+ ǫn pn−2 (z), where the coefficients are Γ(n + 1)Γ(n + a + 1)Γ(n + b + 1)Γ(n + a + b + 1) h(a,b) =2a+b+2n+1 , n Γ(2n + a + b + 1)Γ(2n + a + b + 2) 2n n + b +1 n + a µ(a,b) = + , (3.5) n (2n + a + b + 1) −2n + a + b +2 2n + a + b 4n(n 1)(n + a)(n + b) ǫ(a,b) = − . n −(2n + a + b + 1)(2n + a + b)2(2n + a + b 1) − 14 PETER J. FORRESTER AND SHI-HAO LI From [1, Equation 3.14], one knows (a,b) (a,b) (a,b) (a,b) (1) p ,p ζ p 1 = h δ h 2m 2n+1 − n 2n−1i1,V n n,m with 8n(2n + a)(2n + b)(2n + a + b) ζ(a,b) = , n (4n + a + b 1)(4n + a + b)(4n + a + b + 1)(4n + a + b + 2) − Γ(2n + 1)Γ(2n + a + 1)Γ(2n + b + 1)Γ(2n + a + b + 1) h(1) =2a+b+4n+2 . n Γ(4n + a + b + 1)Γ(4n + a + b + 3) Furthermore, from the properties (3.4), one can compute (a,b) (a,b) 1 (a,b) (a+1,b+1) 1 (a+1,b+1) (a,b) p ,p 2 = (2n + 1) p ,p 2 (2m) p ,p 2 h 2m 2n+1i4,V 2 h 2m 2n i2,V − 2 h 2m−1 2n+1i2,V 1 (a+1,b+1) (a,b) (a+1,b+1) (a,b) (a+1,b+1) (a+1,b+1) = (2n + 1) p + µ p + ǫ p ,p 2 2 h 2m 2m 2m−1 2m 2m−2 2n i2,V 1 (a+1,b+1) (a+1,b+1) (a,b) (a+1,b+1) (a,b) (a+1,b+1) (2m) p ,p + µ p + ǫ p 2 (3.6) − 2 h 2m−1 2n+1 2n+1 2n 2n+1 2n−1 i2,V 1 = (2n + 1)h(a+1,b+1) (2n)ǫ(a,b) h(a+1,b+1) δ 2 2n − 2n+1 2n−1 n,m 1 (2m)h(a+1,b+1) (2m 1)ǫ(a,b)h(a+1,b+1) δ , − 2 2m−1 − − 2m 2m−2 m−1,n (a,b) (a,b) where hn and ǫn are defined in (3.5). As a consequence, 8j(2j + a)(2j + b)(2j + a + b) ζ = , j (4j + a + b 1)(4j + a + b)(4j + a + b + 1)(4j + a + b + 2) − Γ(2j + 1)Γ(2j + a + 1)Γ(2j + b + 1)Γ(2j + a + b + 1) h(1) =2a+b+4j+2 , j Γ(4j + a + b + 1)Γ(4j + a + b + 3) Γ(j + 2)Γ(j + a + 2)Γ(j + b + 2)Γ(j + a + b + 2) h(4) =2a+b+2j+2 . j Γ(2j + a + b + 2)Γ(2j + a + b + 4) Substituting into the recurrence relation (2.8a), one finds that the coefficients α ∞ satisfy the { j }j=0 recurrence (2j + 1)(2j + a + 1)(2j + b + 1)(2j + a + b + 1) 2j(2j + a)(2j + b)(2j + a + b) X2 + + α (4j + a + b + 1)(4j + a + b + 3) (4j + a + b 1)(4j + a + b + 1) j − (2j + 1)2(2j + a + 1)2(2j + b + 1)2(2j + a + b + 1)2 1 =4 αj+1 + (4j + a + b 2)(4j + a + b)αj−1, (4j + a + b + 1)3(4j + a + b + 3)3 4 − where the Pochhammer symbol (a)k is defined by (a) =1, and (a) = a(a + 1) (a + k 1), k =1, 2, 3, . 0 k ··· − ··· Making the substitution (4j + a + b + 1)! α =2−2j αˆ j (2j)!(2j + b)! j gives the modified recurrence 2 1 a+1 b+1 a+b+1 a b a+b X (j + 2 )(j + 2 )(j + 2 )(j + 2 ) j(j + 2 )(j + 2 )(j + 2 ) + a+b+3 a+b+1 + a+b+1 a+b−1 αˆj 4 (2j + 2 )(2j + 2 ) (2j + 2 )(2j + 2 ) ! a+2 a+1 a+b+2 a+b+1 1 b b−1 (j + 2 )(j + 2 )(j + 2 )(j + 2 ) j(j 2 )(j + 2 )(j + 2 ) = a+b+3 a+b+1 αˆj+1 + − a+b+1 a+b−1 αˆj−1. (2j + 2 )(2j + 2 ) (2j + 2 )(2j + 2 ) CLASSICAL SKEW ORTHOGONAL POLYNOMIALS IN A TWO-COMPONENT LOG-GAS 15 This modified recurrence, together with the initial conditions (2.12), is recognised as being satisfied by a special case of the Wilson polynomials [25, Section 1.1], telling us that X2 a +1 b +1 1 αˆ = W˜ ; , , , 0 j j − 4 2 2 2 or in terms of a hypergeometric function a+b+1 a+1−X a+1+X j, j + 2 , 2 , 2 αˆj = 4F3 − a+1 a+2 a+b+2 1 . , , ! 2 2 2 Hence (4j + a + b + 1)! X2 a +1 b +1 1 α =2−2j W˜ ; , , , 0 . j (2j)!(2j + b)! j − 4 2 2 2 In contrast to the Gaussian and Laguerre cases, in the Jacobi case ζ h(4) = h(4) . This means j 2j 6 2j+1 the recurrence relation for ξ ∞ is different to that for α ∞ . However, one can make use of { j }j=0 { j }j=0 Corollary 2.5 to conclude that if we change ξˆ = c ξ , then ξˆ ∞ admits the same recurrence as j j j { j}j=0 α ∞ . In the Jacobi case, c can be computed via (2.13) and we find { j }j=0 j j (4) j h2k−2 4k + a + b 2 2+ a + b cj = ζk = − = . h(4) 4k + a + b +2 4j + a + b +2 kY=1 2k−1 kY=1 −1 Therefore, ξj = cj αj and (4j + a + b + 2)! X2 a +1 b +1 1 ξ =2−2j W˜ ; , , , 0 . j (2j)!(2j + b)!(2 + a + b) j − 4 2 2 2 3.4. Generalised Cauchy case. In this subsection, we consider the remaining of the classical weights on the line, namely the generalised Cauchy weight e−2V (z) = (1 iz)c(1 + iz)c¯ with z R, − ∈ c C. In the one-component case, this weight is in fact related to the circular Jacobi ensemble ∈ [21, 26], whose probability density function (PDF) is defined on [0, 2π)N . Thus if we consider the stereographic projection 1 ix eiθj = − j , 1+ ixj then we can transform the eigenvalue PDF on the unit circle N (1 eiθj )βa(1 e−iθj )βa¯ eiθk eiθj βdθ dθ − − | − | 1 ··· N j=1 Y 1≤j N (1 ix )c(1 + ix )c¯ x x βdx dx . − j j | k − j | 1 ··· N j=1 Y 1≤j
CLASSICAL SKEW ORTHOGONAL POLYNOMIALS in a TWO-COMPONENT LOG-GAS 3 Polynomials [29, §5]
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