Circular Ensembles

In the theory of random matrices, the circular ensembles are measures on spaces of unitary matrices introduced by Freeman Dyson as modifications of the Gaussian matrix ensembles. The three main examples are the circular orthogonal ensemble (COE) on symmetric unitary matrices, the circular unitary ensemble (CUE) on unitary matrices, and the circular symplectic ensemble (CSE) on self dual unitary quaternionic matrices.

Probability distributions

The distribution of the unitary circular ensemble CUE(''n'') is the Haar measure on the unitary group ''U(n)''. If ''U'' is a random element of CUE(''n''), then ''U^TU'' is a random element of COE(''n''); if ''U'' is a random element of CUE(''2n''), then ''U^RU'' is a random element of CSE(''n''), where
:$U^R = \left( \begin 0 & -1 & & & & & \\ 1 & 0 & & & & & \\ & & 0 & -1 & & & \\ & & 1 & 0 & & & \\ & & & & \ddots & & \\ & & & & & 0& -1\\ & & & & & 1 & 0 \end \right) U^T \left( \begin 0 & 1 & & & & & \\ -1 & 0 & & & & & \\ & & 0 & 1 & & & \\ & & -1 & 0 & & & \\ & & & & \ddots & & \\ & & & & & 0& 1\\ & & & & & -1 & 0 \end \right)~.$

Each element of a circular ensemble is a unitary matrix, so it has eigenvalues on the unit circle: $\lambda_k=e^$ with $0 \leq \theta_k < 2\pi$ for ''k=1,2,... n'', where the $\theta_k$ are also known as eigenangles or eigenphases. In the CSE each of these ''n'' eigenvalues appears twice. The distributions have densities with respect to the eigenangles, given by
: $p(\theta_1, \cdots, \theta_n) = \frac \prod_ , e^ - e^, ^\beta~$
on $\R_^n$ (symmetrized version), where β=1 for COE, β=2 for CUE, and β=4 for CSE. The normalisation constant ''Z_n,β'' is given by
: $Z_ = (2\pi)^n \frac~,$
as can be verified via Selberg's integral formula, or Weyl's integral formula for compact Lie groups.

Generalizations

Generalizations of the circular ensemble restrict the matrix elements of ''U'' to real numbers o that ''U'' is in the orthogonal group ''O(n)''">orthogonal_group.html" ;"title="o that ''U'' is in the orthogonal group">o that ''U'' is in the orthogonal group ''O(n)''or to real quaternion numbers [so that ''U'' is in the symplectic group ''Sp(2n)''. The Haar measure on the orthogonal group produces the circular real ensemble (CRE) and the Haar measure on the symplectic group produces the circular quaternion ensemble (CQE).

The eigenvalues of orthogonal matrices come in complex conjugate pairs $e^$ and $e^$, possibly complemented by eigenvalues fixed at ''+1'' or ''-1''. For ''n=2m'' even and ''det U=1'', there are no fixed eigenvalues and the phases ''θ_k'' have probability distribution
: $p(\theta_1, \cdots, \theta_m) = C \prod_ (\cos\theta_k - \cos\theta_j)^2~,$
with ''C'' an unspecified normalization constant. For ''n=2m+1'' odd there is one fixed eigenvalue ''σ=det U'' equal to ±1. The phases have distribution
: $p(\theta_1, \cdots, \theta_m) = C \prod_(1-\sigma\cos\theta_i) \prod_ (\cos\theta_k - \cos\theta_j)^2~.$
For ''n=2m+2'' even and ''det U=-1'' there is a pair of eigenvalues fixed at ''+1'' and ''-1'', while the phases have distribution
: $p(\theta_1, \cdots, \theta_m) = C \prod_(1-\cos^2\theta_i) \prod_ (\cos\theta_k - \cos\theta_j)^2~.$
This is also the distribution of the eigenvalues of a matrix in ''Sp(2m)''.

These probability density functions are referred to as Jacobi distributions in the theory of random matrices, because correlation functions can be expressed in terms of Jacobi polynomials.

Calculations

Averages of products of matrix elements in the circular ensembles can be calculated using Weingarten functions. For large dimension of the matrix these calculations become impractical, and a numerical method is advantageous. There exist efficient algorithms to generate random matrices in the circular ensembles, for example by performing a QR decomposition on a Ginibre matrix.

References

Software Implementations

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External links

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*{{Citation , last1=Forrester , first1=Peter J. , title=Log-gases and random matrices , publisher=Princeton University Press , isbn=978-0-691-12829-0 , year=2010

Random matrices
Mathematical physics
Freeman Dyson