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Distributed Noise-Shaping Quantization: I. Beta Duals of Finite Frames and Near-Optimal Quantization of Random Measurements

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Abstract

This paper introduces a new algorithm for the so-called “analysis problem” in quantization of finite frame representations that provides a near-optimal solution in the case of random measurements. The main contributions include the development of a general quantization framework called distributed noise shaping and, in particular, beta duals of frames, as well as the performance analysis of beta duals in both deterministic and probabilistic settings. It is shown that for random frames, using beta duals results in near-optimally accurate reconstructions with respect to both the frame redundancy and the number of levels at which the frame coefficients are quantized. More specifically, for any frame E of m vectors in \(\mathbb {R}^k\) except possibly from a subset of Gaussian measure exponentially small in m and for any number \(L \ge 2\) of quantization levels per measurement to be used to encode the unit ball in \(\mathbb {R}^k\), there is an algorithmic quantization scheme and a dual frame together that guarantee a reconstruction error of at most \(\sqrt{k}L^{-(1-\eta )m/k}\), where \(\eta \) can be arbitrarily small for sufficiently large problems. Additional features of the proposed algorithm include low computational cost and parallel implementability.

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Notes

  1. As is common, our convention for \(\varepsilon \)-nets is synonymous to \(\varepsilon \)-coverings: \(\mathcal N\) is an \(\varepsilon \)-net for \(\mathscr {X}\) if for all \(x \in \mathscr {X}\) there exists \(y \in \mathcal {N}\) with \(\Vert x-y\Vert _2\le \varepsilon \).

  2. Similar exponential error bounds that have been obtained previously in the case of conventional sigma-delta modulation or for other quantization schemes are not compatible with the results of this paper: The results of [17] and [11] are for a fixed frame-like system, but using a different norm in infinite dimensions, and the dependence on L is unavailable. The results in [12], obtained in yet another functional setting for sigma-delta modulation, come close to being optimal; however, these results were obtained under modeling assumptions on the quantization noise and circuit stability. The exponential near-entropic error decay in the bitrate obtained in [19] combine sigma-delta modulation with further (lossy) bit encoding. Finally, the exponential error decay reported in [1] is obtained with adaptive hyperplane partitions and does not correspond to linear reconstruction.

  3. The following example shows that the minimum value can be strictly smaller: let \(H = \left[ \begin{matrix}1&{}\quad 0\\ -1&{}\quad 1\end{matrix}\right] \), \(E =\left[ \begin{matrix}1\\ 1\end{matrix}\right] \) for which \(\sqrt{m}/\sigma _{\mathrm{min}}(H^{-1}E) = \sqrt{2/5}\). Meanwhile, \(V = \left[ \begin{matrix}1&\quad 1 \end{matrix}\right] \) yields \(\sqrt{p}\Vert VH\Vert _{\infty \rightarrow \infty }/\sigma _{\mathrm{min}}(VE) = 1/2\).

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Acknowledgments

The authors would like thank Thao Nguyen, Rayan Saab and Özgür Yılmaz for the useful conversations on the topic of this paper and the anonymous referees for the valuable comments and the references they have brought to our attention.

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Correspondence to C. Sinan Güntürk.

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Communicated by Joel A. Tropp.

A Appendix

A Appendix

Lemma A.1

Let \(\xi \sim \mathcal {N}(0,I_l)\). For any \(0 < \varepsilon \le 1\), we have

$$\begin{aligned} \mathbb {P}\left( \Vert \xi \Vert _2 \le \varepsilon \sqrt{l} \right) \le \varepsilon ^{l} \mathrm{e}^{(1-\varepsilon ^2)l/2}. \end{aligned}$$

Proof

For any \(t \ge 0\), we have

$$\begin{aligned} \mathbb {P}\left( \Vert \xi \Vert ^2_2 \le \varepsilon ^2 l \right)\le & {} \int _{\mathbb {R}^l} \hbox {e}^{(\varepsilon ^2 l - \Vert x\Vert _2^2)t/2} \frac{\hbox {e}^{-\Vert x\Vert _2^2/2}}{(2\pi )^{l/2}} \,\mathrm {d}x \\= & {} \hbox {e}^{\varepsilon ^2 t l/2} \int _{\mathbb {R}^l} \frac{\hbox {e}^{-(1+t)\Vert x\Vert _2^2/2}}{(2\pi )^{l/2}} \,\mathrm {d}x = \left( \frac{\hbox {e}^{\varepsilon ^2 t}}{1+t} \right) ^{l/2}. \end{aligned}$$

Choosing \(t = \varepsilon ^{-2}-1\) yields the desired bound. \(\square \)

Proof of Theorem 4.3

For an arbitrary \(\tau > 1\), let \(\mathcal {E}_1\) be the event \(\{ \Vert \Omega \Vert _{2\rightarrow 2} \le 2\tau \sqrt{l}\}\). Proposition 4.1 with \(m=l\), \(E=\Omega \), \(t=2(\tau -1)\sqrt{l}\) implies

$$\begin{aligned} \mathbb {P}(\mathcal {E}_1^c) \le \hbox {e}^{-2(\tau -1)^2 l}. \end{aligned}$$

Next, consider a \(\rho \)-net Q of the unit sphere of \(\mathbb {R}^k\) with \(|Q| \le 2k(1+2/\rho )^{k-1}\) (see [27, Proposition 2.1]), where we set \(\rho = \varepsilon /(4\tau )\). Let \(\mathcal {E}_2\) be the event \(\{ \Vert \Omega z\Vert _2 \ge \varepsilon \sqrt{l},\ \forall z \in Q\}\). For each fixed \(z\in \mathbb {R}^k\) with unit norm, \(\Omega z\) has entries that are i.i.d. \(\mathcal {N}(0,1)\). By Lemma A.1, we have

$$\begin{aligned} \mathbb {P}(\mathcal {E}_2^c) \le |Q| \varepsilon ^{l} \hbox {e}^{(1-\varepsilon ^2)l/2} \le 2k(\varepsilon + 8 \tau )^{k-1} \varepsilon ^{l-k+1} \hbox {e}^{(1-\varepsilon ^2)l/2}. \end{aligned}$$

Suppose the event \(\mathcal {E}_1 \cap \mathcal {E}_2\) occurs. For any unit norm \(x \in \mathbb {R}^k\), there exists a \(z \in Q\) such that \(\Vert x-z\Vert _2 \le \rho \). Then \(\Vert \Omega (x-z)\Vert _2 \le 2\tau \rho \sqrt{l} = \varepsilon \sqrt{l}/2\) and \(\Vert \Omega z\Vert _2 \ge \varepsilon \sqrt{l}\), so that

$$\begin{aligned} \Vert \Omega x\Vert _2 \ge \Vert \Omega z\Vert _2 - \Vert \Omega (x-z)\Vert _2 \ge \varepsilon \sqrt{l}/2, \end{aligned}$$

hence \(\sigma _{\mathrm{min}}(\Omega ) \ge \varepsilon \sqrt{l}/2\). It follows that \(\mathcal {F}:=\left\{ \sigma _{\mathrm{min}}(\Omega ) \le \varepsilon \sqrt{l}/2 \right\} \subset \mathcal {E}_1^c \cup \mathcal {E}_2^c\), and therefore

$$\begin{aligned} \mathbb {P}\left( \mathcal {F}\right) \le \hbox {e}^{-2(\tau -1)^2 l} + 2k(\varepsilon + 8 \tau )^{k-1} \varepsilon ^{l-k+1} \hbox {e}^{l/2}. \end{aligned}$$

We still have the freedom to choose \(\tau > 1\) as a function of \(\varepsilon \), l, and k. For simplicity, we choose \(\tau = 1+\sqrt{\log \varepsilon ^{-1}}\), so that \(\hbox {e}^{-2(\tau -1)^2 l} = \varepsilon ^{2l}\). Noting that \(1 + k(1+8\tau )^{k-1} < (2+8\tau )^k\), we obtain

$$\begin{aligned} \mathbb {P}\left( \mathcal {F}\right)< \varepsilon ^{l-k+1} \left( 1 + 2k(1 + 8\tau )^{k-1} \hbox {e}^{l/2}\right) < 2 \left( 10+8\sqrt{\log \varepsilon ^{-1}}\right) ^k \hbox {e}^{l/2} \varepsilon ^{l-k+1}. \end{aligned}$$

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Chou, E., Güntürk, C.S. Distributed Noise-Shaping Quantization: I. Beta Duals of Finite Frames and Near-Optimal Quantization of Random Measurements. Constr Approx 44, 1–22 (2016). https://doi.org/10.1007/s00365-016-9344-4

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