Linear Differential Equations for the Resolvents of the Classical Matrix Ensembles

preprint2020arXivOpen access

Abstract

The spectral density for random matrix ββ ensembles can be written in terms of the average of the absolute value of the characteristic polynomial raised to the power of ββ, which for even ββ is a polynomial of degree β(N−1)β(N-1). In the cases of the classical Gaussian, Laguerre, and Jacobi weights, we show that this polynomial, and moreover the spectral density itself, can be characterised as the solution of a linear differential equation of degree β+1β+1. This equation, and its companion for the resolvent, are given explicitly for β=2β=2 and 44 for all three classical cases, and also for β=6β=6 in the Gaussian case. Known dualities for the spectral moments relating ββ to 4/β4/β then imply corresponding differential equations in the case β=1β=1, and for the Gaussian ensemble, the case β=2/3β=2/3. We apply the differential equations to give a systematic derivation of recurrences satisfied by the spectral moments and by the coefficients of their 1/N1/N expansions, along with first-order differential equations for the coefficients of the 1/N1/N expansions of the corresponding resolvents. We also present the form of the differential equations when scaled at the hard or soft edges.

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