New Restricted Isometry Property Analysis for $\ell_{1}$-$\alpha\ell_{2}$ Minimization

In this paper, we consider the <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{1}-\alpha\ell_{2}$</tex-math></inline-formula> minimization method for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha \in (0, 2]$</tex-math></inline-formula>. Specifically, we present sparse signal recovery conditions under two types of noise: <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{2}$</tex-math></inline-formula>-bounded noise (<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\|\mathbf{v}\|_{2}\leq\epsilon$</tex-math></inline-formula>) and <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{\infty}$</tex-math></inline-formula>-bounded noise (<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\|\mathbf{A}^{T}\mathbf{v}\|_{\infty}\leq\epsilon$</tex-math></inline-formula>). First, based on the RIP framework, we provide a new theoretical guarantee for the successful recovery of sparse signal in the presence of noise when <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(0,1]$</tex-math></inline-formula>, and show that our results are superior to existing ones. Second, we extend the range of <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha$</tex-math></inline-formula> to <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$(1,2]$</tex-math></inline-formula> and provide a new theoretical guarantee for sparse signal recovery under the RIP framework. Finally, numerical experiments demonstrate that the recovery success rate for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(1,2]$</tex-math></inline-formula> is higher than that for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(0,1]$</tex-math></inline-formula>.

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Publication Details

Journal
IEEE Transactions on Signal Processing
Published
2025-01-01
DOI
https://doi.org/10.1109/tsp.2025.3582921
Citations
2
Primary Topic
Approximation Theory and Sequence Spaces
Type
article
Field-Weighted Citation Impact
5.26
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article

New Restricted Isometry Property Analysis for $\ell_{1}$-$\alpha\ell_{2}$ Minimization

Haifeng Li, Jinming Wen, Liang‐Dong Guo
2 citations
IEEE Transactions on Signal Processing
Approximation Theory and Sequence Spaces
5.26
article

New Restricted Isometry Property Analysis for $\ell_{1}$-$\alpha\ell_{2}$ Minimization

Haifeng Li, Jinming Wen, Liang‐Dong Guo
article en
2 citations

Abstract

In this paper, we consider the <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{1}-\alpha\ell_{2}$</tex-math></inline-formula> minimization method for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha \in (0, 2]$</tex-math></inline-formula>. Specifically, we present sparse signal recovery conditions under two types of noise: <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{2}$</tex-math></inline-formula>-bounded noise (<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\|\mathbf{v}\|_{2}\leq\epsilon$</tex-math></inline-formula>) and <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\ell_{\infty}$</tex-math></inline-formula>-bounded noise (<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\|\mathbf{A}^{T}\mathbf{v}\|_{\infty}\leq\epsilon$</tex-math></inline-formula>). First, based on the RIP framework, we provide a new theoretical guarantee for the successful recovery of sparse signal in the presence of noise when <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(0,1]$</tex-math></inline-formula>, and show that our results are superior to existing ones. Second, we extend the range of <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha$</tex-math></inline-formula> to <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$(1,2]$</tex-math></inline-formula> and provide a new theoretical guarantee for sparse signal recovery under the RIP framework. Finally, numerical experiments demonstrate that the recovery success rate for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(1,2]$</tex-math></inline-formula> is higher than that for <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\alpha\in(0,1]$</tex-math></inline-formula>.

IEEE Transactions on Signal ProcessingVol. 73
Jilin University (CN), Jilin Medical University (CN), Henan Normal University (CN)
Openalex Percentile: Top 5%
Approximation Theory and Sequence Spaces
5.26
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