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Private Low-Rank Approximation for Covariance Matrices, Dyson Brownian Motion, and Eigenvalue-Gap Bounds for Gaussian Perturbations

11 February 2025
Oren Mangoubi
Nisheeth K. Vishnoi
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Abstract

We consider the problem of approximating a d×dd \times dd×d covariance matrix MMM with a rank-kkk matrix under (ε,δ)(\varepsilon,\delta)(ε,δ)-differential privacy. We present and analyze a complex variant of the Gaussian mechanism and obtain upper bounds on the Frobenius norm of the difference between the matrix output by this mechanism and the best rank-kkk approximation to MMM. Our analysis provides improvements over previous bounds, particularly when the spectrum of MMM satisfies natural structural assumptions. The novel insight is to view the addition of Gaussian noise to a matrix as a continuous-time matrix Brownian motion. This viewpoint allows us to track the evolution of eigenvalues and eigenvectors of the matrix, which are governed by stochastic differential equations discovered by Dyson. These equations enable us to upper bound the Frobenius distance between the best rank-kkk approximation of MMM and that of a Gaussian perturbation of MMM as an integral that involves inverse eigenvalue gaps of the stochastically evolving matrix, as opposed to a sum of perturbation bounds obtained via Davis-Kahan-type theorems. Subsequently, again using the Dyson Brownian motion viewpoint, we show that the eigenvalues of the matrix MMM perturbed by Gaussian noise have large gaps with high probability. These results also contribute to the analysis of low-rank approximations under average-case perturbations, and to an understanding of eigenvalue gaps for random matrices, both of which may be of independent interest.

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@article{mangoubi2025_2502.07657,
  title={ Private Low-Rank Approximation for Covariance Matrices, Dyson Brownian Motion, and Eigenvalue-Gap Bounds for Gaussian Perturbations },
  author={ Oren Mangoubi and Nisheeth K. Vishnoi },
  journal={arXiv preprint arXiv:2502.07657},
  year={ 2025 }
}
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