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October 20, 20250 citationsOpen Access

On the Performance of Amplitude-Based Models for Low-Rank Matrix Recovery

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HGHuanmin GeZXZhiqiang Xu

Key Points

  • The rank-constrained model achieves a reconstruction error bound of approximately the noise level divided by the square root of the number of measurements.
  • Regardless of its simplicity, the low-rank phase retrieval model demonstrates effectiveness when the linear map follows a Gaussian distribution.
  • Introducing the Lasso model extends existing work on low-rank recovery, with theoretical guarantees for both constrained and unconstrained approaches.
  • This work establishes a new property for linear maps, enhancing theoretical foundations in both phase retrieval and low-rank matrix recovery.

Abstract

In this paper, we focus on low-rank phase retrieval, which aims to reconstruct a matrix X₀ R^n m with rank (X₀) r from noise-corrupted amplitude measurements y=|A (X₀) |+η, where A: R^n m R^p is a linear map and η Rᵖ is the noise vector. We first examine the rank-constrained nonlinear least-squares model X argminₗ ₑ^{₍ ₌, rank (X) r}\||A (X) |-y\|₂² to estimate X₀, and demonstrate that the reconstruction error satisfies \\|{X-X₀\|F, \|X+X₀\|F\} \|η\|₂p with high probability, provided A is a Gaussian measurement ensemble and p (m+n) r. We also prove that the error bound \|η\|₂p is tight up to a constant. Furthermore, we relax the rank constraint to a nuclear-norm constraint. Hence, we propose the Lasso model for low-rank phase retrieval, i. e. , the constrained nuclear-norm model and the unconstrained version. We also establish comparable theoretical guarantees for these models. To achieve this, we introduce a strong restricted isometry property (SRIP) for the linear map A, analogous to the strong RIP in phase retrieval. This work provides a unified treatment that extends existing results in both phase retrieval and low-rank matrix recovery from rank-one measurements.

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Cite This Study

Ge et al. (2025) studied this question.

synapsesocial.com/papers/68f5fcce8d54a28a75cf1cc6https://doi.org/10.48550/arxiv.2509.24699
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