The Wishart distribution of dimension K is defined over K×K positive definite matrices. Its parameters are V, its scale matrix, and ν>K−1, its degrees of freedom.
WK(A∣V,ν)=|A|(ν−K−1)/2exp(−12Tr(V−1A))2νK/2|V|ν/2ΓK(ν2)lnWK(A∣V,ν)=ν−K−12lndetwhere \Gamma_K is the multivariate gamma function[wiki], \psi_K is the multivariate digamma function[wiki] and \psi_1 is the trigamma function[wiki].
This distribution has a mode only if \nu \geqslant K + 1:
Let (\mathbf{A}_n) a set of observed realisations from a Gamma distribution.
\hat{\mathbf{V}} \mid (\mathbf{A}_n), \nu | = \frac{1}{\nu}\overline{\mathbf{A}} |
\hat{\nu} \mid (\mathbf{A}_n) | solution of: K \ln \hat{\nu} - \psi_K\left(\frac{\hat{\nu}}{2}\right) = K \ln 2 + \ln\det\overline{\mathbf{A}} - \overline{\ln \det \mathbf{A}} |
\hat{\mathbf{V}} \mid (\mathbf{A}_n) | = \hat{\mathbf{V}} \mid (\mathbf{A}_n), \hat{\nu} |
where
There is no closed form solution for \hat{\nu}, but an approximate solution can be found by numerical optimisation.
I need to check my math for \nu
We list here the distributions that can be used as conjugate prior for the parameters of an univariate Normal distribution:
\mathbf{V} \mid \nu | Inverse-Wishart | \mathcal{W}^{-1} |
Update equations can be found in the Conjugate prior article.
The KL-divergence can be written as
where H is the cross-entropy. We have
Specialisation | |
Exponential | \mathrm{Exp}(\lambda) = \mathcal{W}\left(\frac{1}{2\lambda}, 2\right) |
Chi-squared | \chi^2(\nu) = \mathcal{G}\left(1, \nu\right) |
Gamma | \mathcal{G}(\alpha, \beta) = \mathcal{W}\left(\frac{1}{2\beta}, 2\alpha\right) |
Power | |
Inverse-Wishart | \mathbf{X} \sim \mathcal{W}(\mathbf{V}, \nu) \Rightarrow \mathbf{X}^{-1} \sim \mathcal{W}^{-1}\left(\mathbf{V}^{-1}, \nu\right) |
Another parameterisation, which may feel more natural when using the Wishart distribution as a prior for the precision matrix of a multivariate Gaussian distribution, uses the expected matrix instead of the scale matrix:
This distribution has a mode only if \nu \geqslant K + 1:
Let (\mathbf{A}_n) a set of observed realisations from a Gamma distribution.
\hat{\boldsymbol\Lambda} \mid (\mathbf{A}_n) | = \overline{\mathbf{A}} |
\hat{\nu} \mid (\mathbf{A}_n) | solution of: K \ln \hat{\nu} - \psi_K\left(\frac{\hat{\nu}}{2}\right) = K \ln 2 + \ln\det\overline{\mathbf{A}} - \overline{\ln \det \mathbf{A}} |
where
There is no closed form solution for \hat{\nu}, but an approximate solution can be found by numerical optimisation.
I need to check my math for \nu
The KL divergence becomes
Created by Yaël Balbastre on 10 April 2018. Last edited on 10 April 2018.