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首页> 外文期刊>Journal of Multivariate Analysis: An International Journal >Estimation of multivariate normal covariance and precision matrices in a star-shape model with missing data
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Estimation of multivariate normal covariance and precision matrices in a star-shape model with missing data

机译:缺少数据的星形模型中多元正态协方差和精度矩阵的估计

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摘要

In this paper, we study the problem of estimating the covariance matrix Sigma and the precision matrix Omega (the inverse of the covariance matrix) in a star-shape model with missing data. By considering a type of Cholesky decomposition of the precision matrix Omega = Psi'Psi, where Psi is a lower triangular matrix with positive diagonal elements, we get the MLEs of the covariance matrix and precision matrix and prove that both of them are biased. Based on the MLEs, unbiased estimators of the covariance matrix and precision matrix are obtained. A special group G, which is a subgroup of the group consisting all lower triangular matrices, is introduced. By choosing the left invariant Haar measure on g as a prior, we obtain the closed forms of the best equivariant estimates of Omega under any of the Stein loss, the entropy loss, and the symmetric loss. Consequently, the MLE of the precision matrix (covariance matrix) is inadmissible under any of the above three loss functions. Some simulation results are given for illustration. (C) 2005 Elsevier Inc. All rights reserved.
机译:在本文中,我们研究在缺少数据的星形模型中估计协方差矩阵Sigma和精度矩阵Omega(协方差矩阵的逆)的问题。通过考虑精度矩阵Omega = Psi'Psi的Cholesky分解,其中Psi是具有正对角线元素的下三角矩阵,我们得到协方差矩阵和精度矩阵的MLE并证明它们都存在偏差。基于MLE,获得协方差矩阵和精度矩阵的无偏估计量。引入了特殊的组G,它是由所有下三角矩阵组成的组的子组。通过选择g上的左不变Haar度量作为先验,我们得到在Stein损失,熵损失和对称损失中任何一个条件下Omega最佳等变估计的闭合形式。因此,在上述三个损失函数中的任何一个下,精度矩阵(协方差矩阵)的MLE都是不允许的。给出一些仿真结果用于说明。 (C)2005 Elsevier Inc.保留所有权利。

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