Lower bounds for the minimax risk using $f$-divergences and applications

Adityanand Guntuboyina

I Introduction

where the infimum is over all measurable functions θ^:X→A\hat{\theta}:{\mathcal{X}}\rightarrow{\mathcal{A}} and the expectation is taken under the assumption that XX is distributed according to PθP_{\theta}.

the infimum being over all estimators TT taking values in FF. The proof of this inequality relies on the triangle inequality satisfied by the metric ρ\rho and can be found, for example, in [1, Page 1570, Proof of Theorem 1] (Let us note, for the convenience of the reader, that the notation employed by Yang and Barron differs from ours in that they use dd for the metric ρ\rho, ϵn,d\epsilon_{n,d} for our η\eta and Nϵn,dN_{\epsilon_{n},d} for the finite set FF. Also the proof in involves a positive constant AA which can be taken to be 1 for our purposes. The constant AA arises because Yang and Barron do not require that dd is a metric but rather require it to satisfy a weaker local triangle inequality which involves the constant AA.)

The next step is to note that rr is bounded from below by Bayes risks. Let ww be a probability measure on FF. The Bayes risk rˉw\bar{r}_{w} corresponding to the prior ww is defined by

where wθ:=w{θ}w_{\theta}:=w\left\{\theta\right\} and the infimum is over all estimators TT taking values in FF. When ww is the discrete uniform probability measure on FF, we simply write rˉ\bar{r} for rˉw\bar{r}_{w}. The trivial inequality r≥rˉwr\geq\bar{r}_{w} implies that lower bounds for rˉw\bar{r}_{w} are automatically lower bounds for rr.

if PP is absolutely continuous with respect to QQ and ∞\infty otherwise.

Our proof of Theorem II.1 presented in section II is extremely simple. It just relies on the convexity of the function ff and the standard result that rˉw\bar{r}_{w} has the following exact expression:

where pθp_{\theta} denotes the density of PθP_{\theta} with respect to a common dominating measure μ\mu (for example, one can take μ:=∑θ∈FPθ\mu:=\sum_{\theta\in F}P_{\theta}).

We show that Fano’s inequality is a special case (see Example II.4) of Theorem II.1, obtained by taking f(x)=xlog⁡xf(x)=x\log x. Fano’s inequality is used extensively in the nonparametric statistics literature for obtaining minimax lower bounds, important works being . In the special case when FF has only two points, Theorem II.1 gives a sharp inequality relating the total variation distance between two probability measures to ff-divergences (see Corollary II.3). When f(x)=xlog⁡xf(x)=x\log x, Corollary II.3 implies an inequality due to Topsøe from which Pinsker’s inequality can be derived. Thus Theorem II.1 can be viewed as a generalization of both Fano’s inequality and Pinsker’s inequality.

The bound given by Theorem II.1 involves the quantity Jf:=inf⁡Q∑θ∈FDf(Pθ∣∣Q)/∣F∣J_{f}:=\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q)/|F|, where the infimum is over all probability measures QQ and ∣F∣|F| denotes the cardinality of the finite set FF. It is usually not possible to calculate JfJ_{f} exactly and in section III, we provide upper bounds for JfJ_{f}. The main result of this section, Theorem III.1, provides an upper bound for JfJ_{f} based on approximating the set of ∣F∣|F| probability measures {Pθ,θ∈F}\left\{P_{\theta},\theta\in F\right\} by a smaller set of probability measures. This result is motivated by and a generalization to ff-divergences of a result of Yang and Barron for the Kullback-Leibler divergence.

In section IV, we use the inequalities proved in sections II and III to obtain minimax lower bounds involving only global metric entropy attributes. Of all the lower bounds presented in this paper, Theorem IV.1, the main result of section IV, is the most application-ready method. In order to apply this in a particular situation, one only needs to determine suitable bounds on global covering and packing numbers of the parameter space Θ\Theta and the space of probability measures {Pθ,θ∈Θ}\left\{P_{\theta},\theta\in\Theta\right\} (see section V for an application).

Although the main results of sections II and III hold true for all ff-divergences, Theorem IV.1 is stated only for the Kullback-Leibler divergence, chi-squared divergence and the divergences based on f(x)=xl−1f(x)=x^{l}-1 for l>1l>1. The reason behind this is that Theorem IV.1 is intended for applications where it is usually the case that the underlying probability measures PθP_{\theta} are product measures and divergences such as the Kullback-Leibler divergence and chi-squared divergence can be computed for product probability measures.

The inequalities given by Theorem IV.1 for the chi-squared divergence and divergences based on f(x)=xl−1f(x)=x^{l}-1 for l>1l>1 are new while the inequality for the Kullback-Leibler divergence is due to Yang and Barron . There turn out to be qualitative differences between these inequalities in the case of estimation problems involving finite dimensional parameters where the inequality based on chi-squared divergence gives minimax lower bounds having the optimal rate while the one based on the Kullback-Leibler divergence only results in sub-optimal lower bounds. We shall explain this happening in section IV by means of elementary examples.

We shall present two applications of our bounds. In section V, we shall prove a new lower bound for the minimax risk in the problem of estimation/reconstruction of a dd-dimensional convex body from noisy measurements of its support function in nn directions. In section VI, we shall provide a different proof of a recent result by Cai, Zhang and Zhou on covariance matrix estimation.

We shall prove a lower bound for rˉw\bar{r}_{w} defined in (2) in terms of ff-divergences. We shall assume that the N:=∣F∣N:=|F| probability measures Pθ,θ∈FP_{\theta},\theta\in F are all dominated by a sigma finite measure μ\mu with densities pθ,θ∈Fp_{\theta},\theta\in F. In terms of these densities, rˉw\bar{r}_{w} has the exact expression given in (3). A trivial consequence of (3) that we shall often use in the sequel is that rˉ≤1−1/N\bar{r}\leq 1-1/N (recall that rˉ\bar{r} is rˉw\bar{r}_{w} in the case when ww is the uniform probability measure on FF).

where W:=∫XwT(x)dQ(x)W:=\int_{{\mathcal{X}}}w_{T(x)}dQ(x). In particular, taking ww to be the uniform probability measure, we get that

The proof of this theorem relies on a simple application of the convexity of ff and it is presented below.

We may assume that all the weights wθw_{\theta} are strictly positive and that the probability measure QQ has a density qq with respect to μ\mu. We start with a simple inequality for nonnegative numbers aθ,θ∈Fa_{\theta},\theta\in F with τ:=arg⁡max⁡θ∈F{wθaθ}\tau:=\arg\max_{\theta\in F}\left\{w_{\theta}a_{\theta}\right\}. We first write

and then use the convexity of ff to obtain that the quantity ∑θwθf(aθ)\sum_{\theta}w_{\theta}f(a_{\theta}) is bounded from below by

We now fix x∈Xx\in{\mathcal{X}} such that q(x)>0q(x)>0 and apply the inequality just derived to aθ:=pθ(x)/q(x)a_{\theta}:=p_{\theta}(x)/q(x). Note that in this case τ=T(x)\tau=T(x). We get that

Integrating inequality (6) with respect to the probability measure QQ, we get that the term ∑θ∈FwθDf(Pθ∣∣Q)\sum_{\theta\in F}w_{\theta}D_{f}(P_{\theta}||Q) is bounded from below by

Let Q′Q^{\prime} be the probability measure on X{\mathcal{X}} having the density q′(x):=wT(x)q(x)/Wq^{\prime}(x):=w_{T(x)}q(x)/W with respect to μ\mu. Clearly

which, by Jensen’s inequality, is larger than or equal to Wf((1−rˉw)/W)Wf((1-\bar{r}_{w})/W). It follows similarly that

This completes the proof of inequality (4). When ww is the uniform probability measure on the finite set FF, it is obvious that WW equals 1/N1/N and this leads to inequality (5). ∎

Let us denote the function of rˉ\bar{r} on the right hand side of (5) by gg:

Inequality (5) provides an implicit lower bound for rˉ\bar{r}. This is because rˉ∈[0,1−1/N]\bar{r}\in[0,1-1/N] and gg is non-increasing on [0,1−1/N][0,1-1/N] (as can be seen in the proof of the next corollary in the case when ff is differentiable; if ff is not differentiable, one needs to work with right and left derivatives which exist for convex functions).

The convexity of ff also implies trivially that gg is convex, which can be used to convert the implicit bound (5) into an explicit lower bound. This is the content of the following corollary. We assume differentiability for convenience; to avoid working with one-sided derivatives.

Suppose that f:[0,∞)f:[0,\infty) is a differentiable convex function and that gg is defined as in (7). Then, for every a∈[0,1−1/N]a\in[0,1-1/N], we have

where the infimum is over all probability measures QQ.

Fix a probability measure QQ. Inequality (5) says that ∑θ∈FDf(Pθ∣∣Q)≥g(rˉ)\sum_{\theta\in F}D_{f}(P_{\theta}||Q)\geq g(\bar{r}). The convexity of ff implies that gg is also convex and hence, for every a∈[0,1−1/N]a\in[0,1-1/N], we can write

Because gg is convex, we have g′(a)≤g′(1−1/N)=0g^{\prime}(a)\leq g^{\prime}(1-1/N)=0 for a≤1−1/Na\leq 1-1/N (this proves that gg is non-increasing on [0,1−1/N][0,1-1/N]). Therefore, by rearranging (9), we obtain (8). ∎

Let us now provide an intuitive understanding of inequality (5). When the probability measures Pθ,θ∈FP_{\theta},\theta\in F are tightly packed i.e., when they are close to one another, it is hard to distinguish between them (based on the observation XX) and hence, the testing Bayes risk rˉ\bar{r} will be large. On the other hand, when the probability measures are well spread out, it is easy to distiguish between them and therefore, rˉ\bar{r} will be small. Indeed, rˉ\bar{r} takes on its maximum value of 1−1/N1-1/N when the probability measures Pθ,θ∈FP_{\theta},\theta\in F are all equal to one another and it takes on its smallest value of 0 when max⁡pθ=∑pθ\max p_{\theta}=\sum p_{\theta} i.e., when Pθ,θ∈FP_{\theta},\theta\in F are all mutually singular.

Now, one way of measuring how packed/spread out the probability measures Pθ,θ∈FP_{\theta},\theta\in F are is to consider the quantity inf⁡Q∑θ∈FDf(Pθ∣∣Q)\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q), which is small when the probabilities are tightly packed and large when they are spread out. It is therefore reasonable to expect a connection between this quantity and rˉ\bar{r}. Inequality (5) makes this connection explicit and precise. The fact that the function gg in (7) is non-increasing means that when inf⁡Q∑θ∈FDf(Pθ∣∣Q)\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q) is small, the lower bound on rˉ\bar{r} implied by (5) is large and when inf⁡Q∑θ∈FDf(Pθ∣∣Q)\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q) is large, the lower bound on rˉ\bar{r} is small.

Theorem II.1 implies the following corollary which provides sharp inequalities between total variation distance and ff-divergences. The total variation distance between two probability measures is defined as half the L1L^{1} distance between their densities.

where the infimum is over all probability measures QQ. Moreover this inequality is sharp in the sense that for every V∈V\in, the infimum of the left hand side of (10) over all probability measures P1P_{1} and P2P_{2} with total variation distance VV equals the right hand side of (10).

In the setting of Theorem II.1, suppose that F={1,2}F=\left\{1,2\right\} and that the two probability measures are P1P_{1} and P2P_{2} with densities p1p_{1} and p2p_{2} respectively. Since 2max⁡(p1,p2)2\max(p_{1},p_{2}) equals p1+p2+∣p1−p2∣p_{1}+p_{2}+|p_{1}-p_{2}|, it follows that 2rˉ2\bar{r} equal 1−V1-V. Inequality (10) is then a direct consequence of inequality (5).

The following example shows that (10) is sharp. Fix V∈V\in. Consider the space X={1,2}{\mathcal{X}}=\left\{1,2\right\} and define the probabilities P1P_{1} and P2P_{2} by P1{1}=P2{2}=(1+V)/2P_{1}\left\{1\right\}=P_{2}\left\{2\right\}=(1+V)/2 and of course P1{2}=P2{1}=(1−V)/2P_{1}\left\{2\right\}=P_{2}\left\{1\right\}=(1-V)/2. Then the total variation distance between P1P_{1} and P2P_{2} equals VV. Also if we take QQ to be the uniform probability measure Q{1}=Q{2}=1/2Q\left\{1\right\}=Q\left\{2\right\}=1/2, then one sees that Df(P1∣∣Q)+Df(P2∣∣Q)D_{f}(P_{1}||Q)+D_{f}(P_{2}||Q) equals f(1+V)+f(1−V)f(1+V)+f(1-V) which is same as the right hand side in (10). ∎

What we have actually shown in the above proof is that inequality (10) is sharp for the space X={1,2}{\mathcal{X}}=\left\{1,2\right\}. However, the result holds in more general spaces as well. For example, if the space is such that there exist two disjoint nonempty subsets A1A_{1} and A2A_{2} and two probability measures ν1\nu_{1} and ν2\nu_{2} concentrated on A1A_{1} and A2A_{2} respectively, then we can define P1:=ν1(1+V)/2+ν2(1−V)/2P_{1}:=\nu_{1}(1+V)/2+\nu_{2}(1-V)/2 and P2:=ν1(1−V)/2+ν2(1+V)/2P_{2}:=\nu_{1}(1-V)/2+\nu_{2}(1+V)/2 so that V(P1,P2)=VV(P_{1},P_{2})=V and (10) becomes an equality (with Q=ν1/2+ν2/2Q=\nu_{1}/2+\nu_{2}/2).

There exist many inequalities in the literature relating the ff-divergence of two probability measures to their total variation distance. We refer the reader to for the sharpest results in this direction and for earlier references. Inequality (10), which is new, can be trivially converted into an inequality between Df(P1∣∣P2)D_{f}(P_{1}||P_{2}) and VV by taking Q=P2Q=P_{2}. The resulting inequality will not be sharp however and hence will be inferior to the inequalities in . As stated, inequality (10) is a sharp inequality relating not Df(P1∣∣P2)D_{f}(P_{1}||P_{2}) but a symmetrized form of ff-divergence between P1P_{1} and P2P_{2} to their total variation distance.

In the remainder of this section, we shall apply Theorem II.1 and Corollary II.3 to specific ff-divergences.

Let f(x):=xlog⁡xf(x):=x\log x. Then Df(P∣∣Q)D_{f}(P||Q) becomes the Kullback-Leibler divergence D(P∣∣Q)D(P||Q) between PP and QQ. The quantity ∑θ∈FD(Pθ∣∣Q)\sum_{\theta\in F}D(P_{\theta}||Q) is minimized when Q=Pˉ:=(∑θ∈FPθ)/NQ=\bar{P}:=(\sum_{\theta\in F}P_{\theta})/N. This is a consequence of the following identity which is sometimes referred to as the compensation identity, see for example [12, Page 1603]:

Using inequality (5) with Q=Pˉ=(∑θ∈FPθ)/NQ=\bar{P}=(\sum_{\theta\in F}P_{\theta})/N, we obtain

The quantity on the left hand side is known as the Jensen-Shannon divergence. It is also Shannon’s mutual information [16, Page 19] between the random parameter θ\theta distributed according to the uniform distribution on FF and the observation XX whose conditional distribution given θ\theta equals PθP_{\theta}. The above inequality is stronger than the version of Fano’s inequality commonly used in nonparametric statistics. It is implicit in [17, Proof of Theorem 1] and is explicitly stated in a slightly different form in [18, Theorem 3]. The proof in is based on the Fano’s inequality from information theory [16, Theorem 2.10.1]. To obtain the usual form of Fano’s inequality as used in statistics, we turn to inequality (8). For a0:=(N−1)/(2N−1)≤1−1/Na_{0}:=(N-1)/(2N-1)\leq 1-1/N and the function gg in (7), it can be checked that

and g′(a0)=−Nlog⁡Ng^{\prime}(a_{0})=-N\log N. Using inequality (8) with a=a0a=a_{0}, we get that

Since log⁡((2N−1)/N)≤log⁡2\log((2N-1)/N)\leq\log 2, we have obtained

which is the commonly used version of Fano’s inequality.

By taking f(x)=xlog⁡xf(x)=x\log x in Corollary II.3, we get that

This inequality relating the Jensen-Shannon divergence between two probability measures (also known as capacitory discrimination) to their total variation distance is due to Topsøe [12, Equation (24)]. Our proof is slightly simpler than Topsøe’s. Topsøe also explains how to use this inequality to deduce Pinsker’s inequality with sharp constant: D(P1∣∣P2)≥2V2D(P_{1}||P_{2})\geq 2V^{2}. Thus, Theorem II.1 can be considered as a generalization of both Fano’s inequality and Pinsker’s inequality to ff-divergences.

Let f(x)=x2−1f(x)=x^{2}-1. Then Df(P∣∣Q)D_{f}(P||Q) becomes the chi-squared divergence χ2(P∣∣Q):=∫p2/q−1\chi^{2}(P||Q):=\int p^{2}/q-1. The function gg can be easily seen to satisfy

Because rˉ≤1−1/N\bar{r}\leq 1-1/N, we can invert the inequality inf⁡Q∑θ∈Fχ2(Pθ∣∣Q)≥g(rˉ)\inf_{Q}\sum_{\theta\in F}\chi^{2}(P_{\theta}||Q)\geq g(\bar{r}) to obtain

Also it follows from Corollary II.3 that for every two probability measures P1P_{1} and P2P_{2},

The weaker inequality χ2(P1∣∣Pˉ)+χ2(P2∣∣Pˉ)≥2V2\chi^{2}(P_{1}||\bar{P})+\chi^{2}(P_{2}||\bar{P})\geq 2V^{2} can be found in [12, Equation (11)].

Let f(x)=1−xf(x)=1-\sqrt{x}. Then Df(P∣∣Q)=1−∫pqdμ=H2(P,Q)/2D_{f}(P||Q)=1-\int\sqrt{pq}d\mu=H^{2}(P,Q)/2, where H2(P,Q)=∫(p−q)2dμH^{2}(P,Q)=\int(\sqrt{p}-\sqrt{q})^{2}d\mu is the square of the Hellinger distance between PP and QQ. It can be shown, using the Cauchy-Schwarz inequality, that ∑θ∈FDf(Pθ∣∣Q)\sum_{\theta\in F}D_{f}(P_{\theta}||Q) is minimized when QQ has a density with respect to μ\mu that is proportional to (∑θ∈Fpθ)2(\sum_{\theta\in F}\sqrt{p_{\theta}})^{2}. Indeed if u:=∑θ∈Fpθu:=\sum_{\theta\in F}\sqrt{p_{\theta}}, then

by the Cauchy-Schwarz inequality with equality when qq is proportional to u2u^{2}. The inequality (5) can then be simplified to

We let h2:=∑θ,θ′H2(Pθ,Pθ′)/N2h^{2}:=\sum_{\theta,\theta^{\prime}}H^{2}(P_{\theta},P_{\theta^{\prime}})/N^{2} so that ∫u2dμ=N2(1−h2/2)\int u^{2}d\mu=N^{2}(1-h^{2}/2). As a consequence, we have ∫u2dμ≤N2\int u^{2}d\mu\leq N^{2}. Also note that ∫u2dμ≥∫(∑θpθ)dμ=N\int u^{2}d\mu\geq\int(\sum_{\theta}p_{\theta})d\mu=N. Therefore, the right hand side of the inequality (14) lies between 1 and N\sqrt{N}. On the other hand, it can be checked that, as a function of rˉ\bar{r}, the left hand side of (14) is strictly increasing from 11 at rˉ=0\bar{r}=0 to N\sqrt{N} at rˉ=1−1/N\bar{r}=1-1/N. It therefore follows that inequality (14) is equivalent to rˉ≥r˘\bar{r}\geq\breve{r} where r˘∈[0,1−1/N]\breve{r}\in[0,1-1/N] is the solution to the equation obtained by replacing the inequality in (14) with an equality.

This equation can be solved in the usual way by squaring etc., until we get a quadratic equation in rˉ\bar{r} which can be solved resulting in two solutions. One of the two solutions can be discarded by continuity considerations (the solution has to be continuous in ∫u2dμ/N\int u^{2}d\mu/N) and the fact that rˉ≤1−1/N\bar{r}\leq 1-1/N. The other solution equals r˘\breve{r} and is given by

In the case when N=2N=2 and F={1,2}F=\left\{1,2\right\}, it is clear that h2=(H2(P1,P2)+H2(P2,P1))/4=H2(P1,P2)/2h^{2}=(H^{2}(P_{1},P_{2})+H^{2}(P_{2},P_{1}))/4=H^{2}(P_{1},P_{2})/2. Also since 2rˉ2\bar{r} equals 1−V1-V, where VV denotes the total variation distance between P1P_{1} and P2P_{2}, the above inequality implies that for every pair of probability measures P1P_{1} and P2P_{2}, we have

This inequality is usually attributed to Le Cam .

Let f(x)=∣x−1∣/2f(x)=|x-1|/2. Then Df(P∣∣Q)D_{f}(P||Q) becomes the total variation distance between PP and QQ. The function gg satisfies

Since rˉ≤1−1/N\bar{r}\leq 1-1/N, we have N(1−rˉ)≥1N(1-\bar{r})\geq 1 and Nrˉ/(N−1)≤1N\bar{r}/(N-1)\leq 1 so that the above expression for g(rˉ)g(\bar{r}) simplifies to N−1−NrˉN-1-N\bar{r}. Inequality (5), therefore, results in

where VθV_{\theta} denotes the total variation distance between PθP_{\theta} and QQ.

Let f(x)=xl−1f(x)=x^{l}-1 where l>1l>1. The case l=2l=2 has already been considered in Example II.5. The function gg has the expression

It therefore follows that inf⁡Q∑θ∈FDf(Pθ∣∣Q)≥g(rˉ)≥Nl(1−rˉ)l−N\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q)\geq g(\bar{r})\geq N^{l}(1-\bar{r})^{l}-N which results in the inequality

When l=2l=2, inequality (15) results in a bound that is weaker than inequality (12) although for large NN, the two bounds are almost the same.

Let f(x)=−log⁡xf(x)=-\log x so that Df(P∣∣Q)=D(Q∣∣P)D_{f}(P||Q)=D(Q||P). Then from Corollary II.3, we get that for every two probability measures P1P_{1} and P2P_{2},

Unlike Example II.4, it is not true that D(Q∣∣P1)+D(Q∣∣P2)D(Q||P_{1})+D(Q||P_{2}) is minimized when Q=PˉQ=\bar{P}. This is easy to see because D(Pˉ,P1)+D(Pˉ,P2)D(\bar{P},P_{1})+D(\bar{P},P_{2}) is finite only when P1<<P2P_{1}<<P_{2} and P2<<P1P_{2}<<P_{1}. By taking Q=P1Q=P_{1} and Q=P2Q=P_{2}, we get that

The above inequality, which is clearly weaker than inequality (16), can also be found in [20, Proof of Lemma 2.6].

In order to apply the minimax lower bounds of the previous section in practical situations, we must be able to bound the quantity Jf:=inf⁡Q∑θ∈FDf(Pθ∣∣Q)/NJ_{f}:=\inf_{Q}\sum_{\theta\in F}D_{f}(P_{\theta}||Q)/N from above. We shall provide such bounds in this section. It should be noted that for some functions ff, it may be possible to calculate JfJ_{f} directly. For example, the quantity inf⁡Q∑θ∈FH2(Pθ,Q)\inf_{Q}\sum_{\theta\in F}H^{2}(P_{\theta},Q) can be written in terms of pairwise Hellinger distances (Example II.6) and may be calculated exactly for certain probability measures PθP_{\theta}. This is not the case for most functions ff however.

The following is a simple upper bound for JfJ_{f} which, in the case when f(x)=xlog⁡xf(x)=x\log x or Kullback-Leibler divergence, has been frequently used in the literature (see for example and ).

We observed in section II that JfJ_{f} measures the spread of the probability measures Pθ,θ∈FP_{\theta},\theta\in F i.e., how tightly packed/spread out they are. It should be clear that the simple bound max⁡θ,θ′Df(Pθ∣∣Pθ′)\max_{\theta,\theta^{\prime}}D_{f}(P_{\theta}||P_{\theta^{\prime}}) does not adequately describe this aspect of Pθ,θ∈FP_{\theta},\theta\in F and it is therefore desirable to look for alternative upper bounds for JfJ_{f} that capture the notion of spread in a better way.

In the case of the Kullback-Leibler divergence, Yang and Barron [1, Page 1571] provided such an upper bound for JfJ_{f}. They showed that for any finite set {Qα:α∈G}\left\{Q_{\alpha}:\alpha\in G\right\} of probability measures,

Let us now take a closer look at this beautiful inequality of Yang and Barron . The ∣G∣|G| probability measures Qα,α∈GQ_{\alpha},\alpha\in G can be viewed as an approximation of the NN probability measures Pθ,θ∈FP_{\theta},\theta\in F. The term max⁡θmin⁡αD(Pθ∣∣Qα)\max_{\theta}\min_{\alpha}D(P_{\theta}||Q_{\alpha}) then denotes the approximation error, measured via the Kullback-Leibler divergence. The right hand side of inequality (17) can therefore be made small if it is possible to choose not too many probability measures QαQ_{\alpha} which well approximate the given set of probability measures PθP_{\theta}.

It should be clear how the upper bound (17) measures the spread of the probability measures Pθ,θ∈FP_{\theta},\theta\in F. If the probabilities are tightly packed, it is possible to approximate them well with a smaller set of probabilities and then the bound will be small. On the other hand, if Pθ,θ∈FP_{\theta},\theta\in F are well spread out, we need more probability measures for approximation and consequently the bound will be large.

Another important aspect of inequality (17) is that it can be used to obtain lower bounds for RR depending only on global metric entropy properties of the parameter space Θ\Theta and the space of probability measures {Pθ,θ∈Θ}\left\{P_{\theta},\theta\in\Theta\right\} (see section IV). On the other hand, the evaluation of inequalities resulting from the use of Jf≤max⁡θ,θ′D(Pθ∣∣Pθ′)J_{f}\leq\max_{\theta,\theta^{\prime}}D(P_{\theta}||P_{\theta^{\prime}}) requires knowledge of both metric entropy and the existence of certain special localized subsets. We refer the reader to for a detailed discussion of these issues.

The goal of this section is to generalize inequality (17) to ff-divergences. The main result is given below. In section IV, we shall use this theorem along with the results of the previous section to come up with minimax lower bounds involving global entropy properties.

Let Qˉ:=∑α∈GQα/M\bar{Q}:=\sum_{\alpha\in G}Q_{\alpha}/M and qˉ:=∑α∈Gqα/M\bar{q}:=\sum_{\alpha\in G}q_{\alpha}/M. Clearly for each θ∈F\theta\in F, we have

The convexity of ff implies that the map y↦y[f(a/y)−f(0)]y\mapsto y[f(a/y)-f(0)] is non-increasing for every nonnegative aa. Using this and the fact that qˉ≥qj(θ)/M\bar{q}\geq q_{j(\theta)}/M, we get that for every θ∈F\theta\in F,

Inequality (18) now follows as a consequence of the inequality Jf≤∑θ∈FDf(Pθ∣∣Qˉ)/NJ_{f}\leq\sum_{\theta\in F}D_{f}(P_{\theta}||\bar{Q})/N. ∎

In the following examples, we shall demonstrate that Theorem III.1 is indeed a generalization of the bound (17) to ff-divergences. We shall also see that Theorem III.1 results in inequalities that have the same qualitative structure as (17), at least for the convex functions ff of interest such as xl−1,l>1x^{l}-1,l>1 and (x−1)2(\sqrt{x}-1)^{2}.

Let f(x)=xlog⁡xf(x)=x\log x. In this case, JfJ_{f} equals ∑θ∈FD(Pθ∣∣Pˉ)/N\sum_{\theta\in F}D(P_{\theta}||\bar{P})/N and invoking inequality (18), we get that

Inequality (17) now follows if we choose j(θ):=arg⁡min⁡α∈GD(Pθ∣∣Qα)j(\theta):=\arg\min_{\alpha\in G}D(P_{\theta}||Q_{\alpha}). Hence Theorem III.1 is indeed a generalization of (17).

Let f(x)=xl−1f(x)=x^{l}-1 for l>1l>1. Applying inequality (18), we get that

By choosing j(θ)=arg⁡min⁡α∈GDf(Pθ∣∣Qα)j(\theta)=\arg\min_{\alpha\in G}D_{f}(P_{\theta}||Q_{\alpha}), we get that

In particular, in the case of the chi-squared divergence i.e., when l=2l=2, the quantity Jf=inf⁡Q∑θ∈Fχ2(Pθ∣∣Q)/NJ_{f}=\inf_{Q}\sum_{\theta\in F}\chi^{2}(P_{\theta}||Q)/N is bounded from above by

Just like (17), each of the above two inequalities is also a function of the number of probability measures QαQ_{\alpha} and the approximation error which is now measured in terms of the chi-squared divergence.

Let f(x)=(x−1)2f(x)=(\sqrt{x}-1)^{2} so that Df(P∣∣Q)=H2(P,Q)D_{f}(P||Q)=H^{2}(P,Q), the square of the Hellinger distance between PP and QQ. Using inequality (18), we get that

If we now choose j(θ):=arg⁡min⁡α∈GH2(Pθ,Qα)j(\theta):=\arg\min_{\alpha\in G}H^{2}(P_{\theta},Q_{\alpha}), then we get

Notice, once again, the trade-off between MM and the approximation error which is measured in terms of the Hellinger distance.

IV Bounds involving global entropy

In this section, we shall apply the results of the previous two sections to obtain lower bounds for the minimax risk RR depending only on global metric entropy properties of the parameter space. The theorem is stated below, but we shall need to establish some notation first.

For η>0\eta>0, let N(η)≥1N(\eta)\geq 1 be a real number for which there exists a finite subset F⊆ΘF\subseteq\Theta with cardinality ≥N(η)\geq N(\eta) satisfying ρ(θ,θ′)≥η\rho(\theta,\theta^{\prime})\geq\eta whenever θ,θ′∈F\theta,\theta^{\prime}\in F and θ≠θ′\theta\neq\theta^{\prime}. In other words, N(η)N(\eta) is a lower bound on the η\eta-packing number of the metric space (Θ,ρ)(\Theta,\rho).

We note here that the probability measures Qα,α∈GQ_{\alpha},\alpha\in G in the definition of Mf(ϵ,S)M_{f}(\epsilon,S) do not need to be included in the set {Pθ,θ∈Θ}\left\{P_{\theta},\theta\in\Theta\right\} and the set GG just denotes the index set and need not have any relation to SS or Θ\Theta.

We now fix ϵ>0\epsilon>0 and use the definition of MC(ϵ,F)M_{C}(\epsilon,F) to get a finite set GG with cardinality ≤MC(ϵ,F)\leq M_{C}(\epsilon,F) and probability measures Qα,α∈GQ_{\alpha},\alpha\in G such that sup⁡θ∈Smin⁡α∈Gχ2(Pθ∣∣Qα)≤ϵ2\sup_{\theta\in S}\min_{\alpha\in G}\chi^{2}(P_{\theta}||Q_{\alpha})\leq\epsilon^{2}. We then use inequality (20) to get that

The proof is complete by the trivial observation MC(ϵ,F)≤MC(ϵ,Θ)M_{C}(\epsilon,F)\leq M_{C}(\epsilon,\Theta). ∎

The inequality (21) is due to Yang and Barron [1, Proof of Theorem 1]. In their paper, Yang and Barron mainly considered the problem of estimation from nn independent and identically distributed observations. However their method results in inequality (21) which applies to every estimation problem. Inequalities (22) and (23) are new.

Note that the lower bounds for RR given in Theorem IV.1 all depend only on the quantities N(η)N(\eta) and Mf(ϵ,Θ)M_{f}(\epsilon,\Theta), which describe packing/covering properties of the entire parameter space Θ\Theta. Consequently, these inequalities only involve global metric entropy properties. This is made possible by the use of inequalities in Theorem III.1. In applications of Fano’s inequality (11) with the standard bound Jf≤max⁡θ,θ′∈FD(Pθ∣∣Pθ′)J_{f}\leq\max_{\theta,\theta^{\prime}\in F}D(P_{\theta}||P_{\theta^{\prime}}) as well as in the application of other popular methods for obtaining minimax lower bounds like Le Cam’s method or Assouad’s lemma, one needs to construct the finite subset FF of the parameter space in a very special way: the parameter values in FF should be reasonably separated in the metric ρ\rho and also, the probability measures Pθ,θ∈FP_{\theta},\theta\in F should be close in some probability metric. In contrast, the application of Theorem IV.1 does not require the construction of such a special subset FF.

Yang and Barron have successfully applied inequality (21) to achieve minimax lower bounds of the optimal rate for many nonparametric density estimation and regression problems where N(η)N(\eta) and MKL(ϵ,Θ)M_{KL}(\epsilon,\Theta) can be deduced from standard results in approximation theory for function classes. We refer the reader to for examples. In some of these examples, inequality (22) can also be applied to get optimal lower bounds. In section V, we shall employ inequality (22) to obtain a new minimax lower bound in the problem of reconstructing convex bodies from noisy support function measurements.

But prior to that, let us assess the performance of inequality (22) in certain standard parametric estimation problems. In these problems, an interesting contrast arises between the two minimax lower bounds (21) and (22): the inequality (21) only results in a sub-optimal lower bound on the minimax risk (this observation, due to Yang and Barron [1, Page 1574], is also explained in Example IV.2 below) while (22) produces rate-optimal lower bounds.

Our intention here is to demonstrate, with the help of the subsequent three examples, that inequality (22) works even for finite dimensional parametric estimation problems, a scenario in which it is already known [1, Page 1574] that inequality (21) fails. Of course, obtaining optimal minimax rates in such problems is facile in most situations. For example, a two-points argument based on Hellinger distance gives the optimal rate, as is widely recognized since Le Cam . But the point here is that even in finite dimensional situations, global metric entropy features are adequate for obtaining rate-optimal minimax lower bounds. This is contrary to the usual claim that in order to establish rate-optimal lower bounds in parametric settings, one needs more information than global entropy characteristics [1, Page 1574].

Suppose that mθm_{\theta} equals the normal distribution with mean θ\theta and variance 1. It can be readily verified that, for θ,θ′∈Θ\theta,\theta^{\prime}\in\Theta, one has

It follows directly that D(Pθ∣∣Pθ′)≤ϵ2D(P_{\theta}||P_{\theta^{\prime}})\leq\epsilon^{2} if and only if ∣θ−θ′∣≤2ϵ/n|\theta-\theta^{\prime}|\leq\sqrt{2}\epsilon/\sqrt{n} and χ2(Pθ∣∣Pθ′)≤ϵ2\chi^{2}(P_{\theta}||P_{\theta^{\prime}})\leq\epsilon^{2} if and only if ∣θ−θ′∣≤log⁡(1+ϵ2)/n|\theta-\theta^{\prime}|\leq\sqrt{\log(1+\epsilon^{2})}/\sqrt{n}. As a result, we can take

for ϵ≤ϵ0\epsilon\leq\epsilon_{0}. Now, inequality (21) says that the minimax risk RnR_{n} satisfies

The function ϵ↦ϵ2−log⁡ϵ\epsilon\mapsto\epsilon^{2}-\log\epsilon is minimized on [0,ϵ0][0,\epsilon_{0}] at, say, ϵ=ϵ1\epsilon=\epsilon_{1} and we then get

where c3c_{3} is a function of c2c_{2} and ϵ1\epsilon_{1}. We now note that when η=c/n\eta=c/\sqrt{n} for a constant cc, the quantity inside the parantheses on the right hand side of (25) converges to 0 as nn goes to ∞\infty. This means that inequality (21) only gives lower bounds of inferior order for RnR_{n}, the optimal order being, of course, 1/n1/n.

On the other hand, we shall show below that inequality (22) gives Rn≥c/nR_{n}\geq c/n for a positive constant cc. Indeed, inequality (22) says that

Taking ϵ=ϵ0\epsilon=\epsilon_{0} and η=c3/n\eta=c_{3}/\sqrt{n}, we get

where c4c_{4} depends only on c1,c2c_{1},c_{2} and ϵ0\epsilon_{0}. Hence by choosing c3c_{3} small, we get that Rn≥c/nR_{n}\geq c/n for all large nn.

Suppose that Θ\Theta is a compact interval of the positive real line that is bounded away from zero and suppose that mθm_{\theta} denotes the uniform distribution on [0,θ][0,\theta]. It is then elementary to check that the chi-squared divergence between PθP_{\theta} and Pθ′P_{\theta^{\prime}} equals (θ′/θ)n−1(\theta^{\prime}/\theta)^{n}-1 if θ≤θ′\theta\leq\theta^{\prime} and ∞\infty otherwise. It follows accordingly that χ2(Pθ∣∣Pθ′)≤ϵ2\chi^{2}(P_{\theta}||P_{\theta^{\prime}})\leq\epsilon^{2} provided

Because the parameter space is a compact interval bounded away from zero, in order to ensure (27), it is enough to require that 0≤θ′−θ≤c2log⁡(1+ϵ2)/n0\leq\theta^{\prime}-\theta\leq c_{2}\log(1+\epsilon^{2})/n. Therefore, we can take

for ϵ≤ϵ0\epsilon\leq\epsilon_{0}. Inequality (22) now implies that

Taking ϵ=ϵ0\epsilon=\epsilon_{0} and η=c4/n\eta=c_{4}/n, we get that

where c5c_{5} depends only on c1,c3c_{1},c_{3} and ϵ0\epsilon_{0}. Hence by choosing c4c_{4} sufficiently small, we get that Rn≥c/n2R_{n}\geq c/n^{2} for all large nn. This is the optimal minimax rate for this problem as can be seen by estimating θ\theta by the maximum of the observations.

Suppose that mθm_{\theta} denotes the uniform distribution on the interval [θ,θ+1][\theta,\theta+1]. We shall argue that MC(ϵ,Θ)M_{C}(\epsilon,\Theta) can be chosen to be

for a positive constant c2c_{2} at least for large nn. To see this, let us define ϵ′\epsilon^{\prime} so that 2ϵ′:=(1+ϵ2)1/n−12\epsilon^{\prime}:=(1+\epsilon^{2})^{1/n}-1 and let GG denote an ϵ′\epsilon^{\prime}-grid of points in the interval Θ\Theta; GG would contain at most c2/ϵ′c_{2}/\epsilon^{\prime} points when ϵ≤ϵ0\epsilon\leq\epsilon_{0}. For a point α\alpha in the grid, let QαQ_{\alpha} denote the nn-fold product of the uniform distribution on the interval [α,α+1+2ϵ′][\alpha,\alpha+1+2\epsilon^{\prime}]. Now, for a fixed θ∈Θ\theta\in\Theta, let α\alpha denote the point in the grid such that α≤θ≤α+ϵ′\alpha\leq\theta\leq\alpha+\epsilon^{\prime}. It can then be checked that the chi-squared divergence between PθP_{\theta} and QαQ_{\alpha} is equal to (1+2ϵ′)n−1=ϵ2(1+2\epsilon^{\prime})^{n}-1=\epsilon^{2}. Hence MC(ϵ,Θ)M_{C}(\epsilon,\Theta) can be taken to be the number of probability measures QαQ_{\alpha}, which is the same as the number of points in GG. We thus have (28). It can be checked by elementary calculus (Taylor expansion, for example) that the inequality

holds for ϵ≤2\epsilon\leq\sqrt{2} (in fact for all ϵ\epsilon, but for ϵ>2\epsilon>\sqrt{2}, the right hand side above may be negative). Therefore for ϵ≤min⁡(ϵ0,2)\epsilon\leq\min(\epsilon_{0},\sqrt{2}), we get that

From inequality (22), we get that for every η≤η0\eta\leq\eta_{0} and ϵ≤min⁡(ϵ0,2)\epsilon\leq\min(\epsilon_{0},\sqrt{2}),

If we now take ϵ=min⁡(ϵ0,1)\epsilon=\min(\epsilon_{0},1) and η=c3/n\eta=c_{3}/n, we see that the quantity inside the parantheses converges to 1−c3c41-\sqrt{c_{3}}c_{4} where c4c_{4} depends only on c1,c2c_{1},c_{2} and ϵ0\epsilon_{0}. Therefore by choosing c3c_{3} sufficiently small, we get that Rn≥c/n2R_{n}\geq c/n^{2}. This is the optimal minimax rate for this problem as can be seen by estimating θ\theta by the minimum of the observations.

The fact that inequality (22) produced optimal lower bounds for the minimax risk in each of the above three examples is reassuring but not really exciting because, as we mentioned before, there are other simpler methods of obtaining such bounds in these examples. We presented them as simple toy examples to evaluate the performance of (22), to present a difference between (21) and (22) (which provides a justification for using divergences other than the Kullback-Leibler divergence for lower bounds) and also to stress the fact that global packing and covering characteristics are enough to obtain optimal minimax lower bounds. In order to convince the reader of the effectiveness of (22) in more involved situations, we now apply it to obtain the optimal minimax rate in a dd-dimensional normal mean estimation problem. We are grateful to an anonymous referee for communicating this example to us. Another non-trivial application of (22) is presented in the next section.

We shall use inequality (22) to show that the minimax risk RR for this problem is larger than or equal to a constant multiple of dσ2d\sigma^{2} when Γ≥σd\Gamma\geq\sigma\sqrt{d}. We begin by arguing that we can take

whenever σlog⁡(1+ϵ2)≤Γ\sigma\sqrt{\log(1+\epsilon^{2})}\leq\Gamma.

For N(η)N(\eta), we first note that the η\eta-packing number of the metric space (Θ,ρ)(\Theta,\rho) is bounded from below by its η\eta-covering number. Now, for any η\eta-covering set, the space Θ\Theta is contained in the union of the balls of radius η\eta with centers in the covering set and hence the volume of Θ\Theta must be smaller than the sum of the volumes of these balls. Therefore, the number of points in the η\eta-covering set must be at least (Γ/η)d(\Gamma/\eta)^{d}. Since this is true for every η\eta-covering set, it follows that the η\eta-covering number and hence the η\eta-packing number is not smaller than (Γ/η)d(\Gamma/\eta)^{d}.

For MC(ϵ,Θ)M_{C}(\epsilon,\Theta), we first observe that for θ,θ′∈Θ\theta,\theta^{\prime}\in\Theta, the chi-squared divergence between PθP_{\theta} and Pθ′P_{\theta^{\prime}} can be easily computed (because they are normal distributions with the same covariance matrix) to be χ2(Pθ∣∣Pθ′)=exp⁡(ρ2(θ,θ′)/σ2)−1\chi^{2}(P_{\theta}||P_{\theta^{\prime}})=\exp\left(\rho^{2}(\theta,\theta^{\prime})/\sigma^{2}\right)-1. Therefore χ2(Pθ∣∣Pθ′)≤ϵ2\chi^{2}(P_{\theta}||P_{\theta^{\prime}})\leq\epsilon^{2} if and only if ρ(θ,θ′)≤ϵ′:=σlog⁡(1+ϵ2)\rho(\theta,\theta^{\prime})\leq\epsilon^{\prime}:=\sigma\sqrt{\log(1+\epsilon^{2})}. As a result, MC(ϵ,Θ)M_{C}(\epsilon,\Theta) can be taken to be any upper bound on the ϵ′\epsilon^{\prime}-covering number of (Θ,ρ)(\Theta,\rho). The ϵ′\epsilon^{\prime}-covering number, as noted previously, is bounded from above by the ϵ′\epsilon^{\prime}-packing number. Now, for any ϵ′\epsilon^{\prime}-packing set, the balls of radius ϵ′/2\epsilon^{\prime}/2 with centers in the packing set are all disjoint and their union is contained in the ball of radius Γ+(ϵ′/2)\Gamma+(\epsilon^{\prime}/2) centered at the origin. Consequently, the sum of the volumes of these balls is smaller than the volume of the ball of radius Γ+(ϵ′/2)\Gamma+(\epsilon^{\prime}/2) centered at the origin. Therefore, the number of points in the ϵ′\epsilon^{\prime}-packing set is at most (1+(2Γ/ϵ′))d≤(3Γ/ϵ′)d(1+(2\Gamma/\epsilon^{\prime}))^{d}\leq(3\Gamma/\epsilon^{\prime})^{d} provided ϵ′≤Γ\epsilon^{\prime}\leq\Gamma. Since this is true for every ϵ′\epsilon^{\prime}-packing set, it follows that the ϵ′\epsilon^{\prime}-packing number and hence the ϵ′\epsilon^{\prime}-covering number is not larger than (3Γ/ϵ′)d(3\Gamma/\epsilon^{\prime})^{d}.

We can thus apply inequality (22) with (29) to get that, for every η>0\eta>0 and ϵ>0\epsilon>0 such that σlog⁡(1+ϵ2)≤Γ\sigma\sqrt{\log(1+\epsilon^{2})}\leq\Gamma, we have

Now by elementary calculus, it can be checked that the function ϵ↦1+ϵ2/(log⁡(1+ϵ2))d/4\epsilon\mapsto\sqrt{1+\epsilon^{2}}/(\log(1+\epsilon^{2}))^{d/4} is minimized (subject to σlog⁡(1+ϵ2)≤Γ\sigma\sqrt{\log(1+\epsilon^{2})}\leq\Gamma) when 1+ϵ2=ed/21+\epsilon^{2}=e^{d/2}. We then get that

We now take η=c1σd\eta=c_{1}\sigma\sqrt{d} and since Γ≥σd\Gamma\geq\sigma\sqrt{d}, we obtain

V Reconstruction of convex bodies from noisy support function measurements

Let {ui,i≥1}\left\{u_{i},i\geq 1\right\} be a sequence of dd-dimensional unit vectors. Gardner, Kiderlen and Milanfar (see their paper for earlier references) considered the problem of reconstructing an unknown convex body KK from noisy measurements of hKh_{K} in the directions u1,…,unu_{1},\dots,u_{n}. More precisely, their problem was to estimate KK from observations Y1,…,YnY_{1},\dots,Y_{n} drawn according to the model Yi=hK(ui)+ξi,i=1,…,nY_{i}=h_{K}(u_{i})+\xi_{i},i=1,\dots,n where ξ1,…,ξn\xi_{1},\dots,\xi_{n} are independent and identically distributed mean zero gaussian random variables. They constructed a convex body (estimator) K^n=K^n(Y1,…,Yn)\hat{K}_{n}=\hat{K}_{n}(Y_{1},\dots,Y_{n}) having the property that, for nice sequences {ui,i≥1}\left\{u_{i},i\geq 1\right\}, the L2L^{2} norm ∣∣hK−hK^n∣∣2||h_{K}-h_{\hat{K}_{n}}||_{2} (see (30) below) converges to zero at the rate n−2/(d+3)n^{-2/(d+3)} for dimensions d=2,3,4d=2,3,4 and at a slower rate for dimensions d≥5d\geq 5 (see [25, Theorem 6.2]).

We shall show here that in the same setting, it is impossible in the minimax sense to construct estimators for KK converging at a rate faster than n−2/(d+3)n^{-2/(d+3)}. This implies that the least squares estimator in is rate optimal for dimensions d=2,3,4d=2,3,4. We shall need some notation to describe our result.

An estimator for hKh_{K} is allowed to be a bounded function on Sd−1S^{d-1} that depends on the data Y1,…,YnY_{1},\dots,Y_{n}. The loss functions that we shall use are the LpL^{p} norms for p∈[1,∞]p\in[1,\infty] defined by

for p∈[1,∞)p\in[1,\infty) and ∣∣hK−h^∣∣∞:=sup⁡u∈Sd−1∣hK(u)−h^(u)∣||h_{K}-\hat{h}||_{\infty}:=\sup_{u\in S^{d-1}}|h_{K}(u)-\hat{h}(u)|. For convex bodies KK and LL and p∈[1,∞]p\in[1,\infty], we shall also write δp(K,L)\delta_{p}(K,L) for ∣∣hK−hL∣∣p||h_{K}-h_{L}||_{p} and refer to δp\delta_{p} as the LpL^{p} distance between KK and LL.

We shall consider the minimax risk of the problem of estimating hKh_{K} from Y1,…,YnY_{1},\dots,Y_{n} when KK is assumed to belong to Kd(Γ){\mathcal{K}}^{d}(\Gamma) i.e., we are interested in the quantity

The following is the main theorem of this section.

Fix p∈[1,∞)p\in[1,\infty) and Γ>0\Gamma>0. Suppose the errors ξ1,…,ξn\xi_{1},\dots,\xi_{n} are independent normal random variables with mean zero and variance σ2\sigma^{2}. Then the minimax risk rn(p,Γ)r_{n}(p,\Gamma) satisfies

for a constant cc that is independent of nn.

In the case when p=2p=2, Gardner, Kiderlen and Milanfar showed that the least squares estimator converges at the rate given by the right hand side of (31) for dimensions d=2,3,4d=2,3,4. Thus, at least for p=2p=2, the lower bound given by (31) is optimal for dimensions d=2,3,4d=2,3,4.

In order to apply inequality (22), we need to determine N(η)N(\eta) and MC(ϵ,Θ)M_{C}(\epsilon,\Theta). The quantity N(η)N(\eta) is a lower bound on the η\eta-packing number of the set Kd(Γ){\mathcal{K}}^{d}(\Gamma) under the LpL^{p} norm. When p=∞p=\infty, Bronshtein [26, Theorem 4 and Remark 1] proved that there exist positive constants c′c^{\prime} and η0\eta_{0} depending only on dd such that exp⁡(c′(η/Γ)(1−d)/2)\exp\left(c^{\prime}(\eta/\Gamma)^{(1-d)/2}\right) is a lower bound for the η\eta-packing number of Θ\Theta for η≤η0\eta\leq\eta_{0}. It is a standard fact that p=∞p=\infty corresponds to the Hausdorff metric on Kd(Γ){\mathcal{K}}^{d}(\Gamma).

It turns out that Bronshtein’s result is actually true for every p∈[1,∞]p\in[1,\infty] and not just for p=∞p=\infty. However, to the best of our knowledge, this has not been proved anywhere in the literature. By modifying Bronshtein’s proof appropriately and using the Varshamov-Gilbert lemma (see for example [27, Lemma 4.7]), we provide, in Theorem VII.1, a proof of this fact. Therefore from Theorem VII.1, we can take

where c′c^{\prime} and η0\eta_{0} are constants depending only on dd and pp.

Now let us turn to MC(ϵ,Θ)M_{C}(\epsilon,\Theta). For f,g∈Θf,g\in\Theta, PfP_{f} and PgP_{g} are normal distributions with the same covariance matrix and hence the chi-squared divergence between PfP_{f} and PgP_{g} can be seen to be

where ϵ′:=σlog⁡(1+ϵ2)/n\epsilon^{\prime}:=\sigma\sqrt{\log(1+\epsilon^{2})}/\sqrt{n}. Let Wϵ′W_{\epsilon^{\prime}} be the smallest WW for which there exist sets K1,…,KWK_{1},\dots,K_{W} in Kd(Γ){\mathcal{K}}^{d}(\Gamma) having the property that for every set K∈Kd(Γ)K\in{\mathcal{K}}^{d}(\Gamma), there exists a KjK_{j} such that the Hausdorff distance between KK and KjK_{j} is less than or equal to ϵ′\epsilon^{\prime}. It must be clear from (33) that MC(ϵ,Θ)M_{C}(\epsilon,\Theta) can be taken to be a number larger than Wϵ′W_{\epsilon^{\prime}}. Bronshtein [26, Theorem 3 and Remark 1] showed that there exist positive constants c′′c^{\prime\prime} and ϵ0\epsilon_{0} depending only on dd such that

Hence for all ϵ\epsilon such that log⁡(1+ϵ2)≤nϵ02/σ2\log(1+\epsilon^{2})\leq n\epsilon_{0}^{2}/\sigma^{2}, we can take

We are now ready to prove inequality (31). We shall define two quantities

where c=c(d,p)c=c(d,p) will be specified shortly. Also let ϵ(n)\epsilon(n) be such that log⁡(1+ϵ2(n))=u2(n)\log(1+\epsilon^{2}(n))=u^{2}(n). Clearly as n→∞n\rightarrow\infty, we have η(n)→0\eta(n)\rightarrow 0, u(n)→∞u(n)\rightarrow\infty and u(n)/n→0u(n)/\sqrt{n}\rightarrow 0. As a result η(n)≤η0\eta(n)\leq\eta_{0} and u2(n)≤nϵ02/σ2u^{2}(n)\leq n\epsilon_{0}^{2}/\sigma^{2} for large nn and therefore from (32) and (34), we get that

for all large nn. If we now choose cc so that c(d−1)/2=c′/(2+2c′′)c^{(d-1)/2}=c^{\prime}/(2+2c^{\prime\prime}), we get that

Now observe that as n→∞n\rightarrow\infty, the quantity η(n)\eta(n) goes to 0 and hence N(η(n))N(\eta(n)) goes to ∞\infty. Further, as we have already noted, u(n)u(n) goes to ∞\infty. It follows hence that rn(p,Γ)≥η(n)/4r_{n}(p,\Gamma)\geq\eta(n)/4 for all large nn. By choosing cc even smaller, we can make inequality (31) true for all nn.

VI A covariance matrix estimation example

In the previous section, we have used the global minimax lower bound (22). However, in some situations, the global entropy numbers might be difficult to bound. In such cases, inequalities (21) and (22) are, of course, not applicable and we are unaware of the use of inequality (17) in conjuction with Fano’s inequality (11) in the literature. The standard examples use (11) with the bound Jf≤min⁡θ,θ′∈FD(Pθ∣∣Pθ′)J_{f}\leq\min_{\theta,\theta^{\prime}\in F}D(P_{\theta}||P_{\theta^{\prime}}) while the examples in all deal with the case when global entropies are available. In this section, we shall demonstrate how a recent minimax lower bound due to Cai, Zhang and Zhou can also be proved using inequalities (11) and (17).

Cai, Zhang and Zhou considered nn independent p×1p\times 1 random vectors X1,…,XnX_{1},\dots,X_{n} distributed according to Np(0,Σ)N_{p}(0,\Sigma). Suppose that the entries of the p×pp\times p covariance matrix Σ=(σij)\Sigma=(\sigma_{ij}) decay at a certain rate as we move away from the diagonal. Specifically, let us suppose that for a fixed positive constant α>0\alpha>0, the entries σij\sigma_{ij} of Σ\Sigma satisfy the inequality σij≤∣i−j∣−α−1\sigma_{ij}\leq|i-j|^{-\alpha-1} for i≠ji\neq j. Cai, Zhang and Zhou showed that when pp is large compared to nn, it is impossible to estimate Σ\Sigma from X1,…,XnX_{1},\dots,X_{n} in the spectral norm at a rate faster than n−α/(2α+1)n^{-\alpha/(2\alpha+1)}. More precisely, they showed that when p≥Cn1/(2α+1)p\geq Cn^{1/(2\alpha+1)},

where cc and CC denote positive constants depending only on α\alpha. Here Θ\Theta denotes the collection of all covariance matrices Σ=(σij)\Sigma=(\sigma_{ij}) satisfying σij≤∣i−j∣−α−1\sigma_{ij}\leq|i-j|^{-\alpha-1} for i≠ji\neq j and the norm ∣∣.∣∣||.|| is the spectral norm (largest eigenvalue).

Cai, Zhang and Zhou used Assouad’s lemma for the proof of the inequality (35). We shall use inequalities (11) and (17). Moreover, the choice of the finite subset FF that we use is different from the one used in [13, Equation (17)]. This makes our approach different from the general method, due to Yu , of replacing Assouad’s lemma by Fano’s inequality.

Throughout, Δ\Delta denotes a constant that depends on α\alpha alone. The value of the constant might vary from place to place.

Consider the matrix A=(aij)A=(a_{ij}) with aij=1a_{ij}=1 for i=ji=j and aij=1/(Δ∣i−j∣α+1)a_{ij}=1/(\Delta|i-j|^{\alpha+1}) for i≠ji\neq j. For Δ\Delta sufficiently large (depending on α\alpha alone), AA is positive definite and belongs to Θ\Theta. Let us fix a positive integer k≤p/2k\leq p/2 and partition AA as

where A12(τ)A_{12}(\tau) is the k×(p−k)k\times(p-k) matrix obtained by premultiplying A12A_{12} with the k×kk\times k diagonal matrix with diagonal entries τ1,…,τk\tau_{1},\dots,\tau_{k}. Clearly, A(τ)∈ΘA(\tau)\in\Theta for all τ∈{0,1}k\tau\in\left\{0,1\right\}^{k}. We shall need the following two lemmas in order to prove inequality (35).

For τ,τ′∈{0,1}k,τ≠τ′\tau,\tau^{\prime}\in\left\{0,1\right\}^{k},\tau\neq\tau^{\prime}, we have

where Υ(τ,τ′):=∑r=1k{τr≠τr′}\Upsilon(\tau,\tau^{\prime}):=\sum_{r=1}^{k}\left\{\tau_{r}\neq\tau^{\prime}_{r}\right\} denotes the Hamming distance between τ\tau and τ′\tau^{\prime}.

Fix τ,τ′∈{0,1}k\tau,\tau^{\prime}\in\left\{0,1\right\}^{k} with τ≠τ′\tau\neq\tau^{\prime}. Let vv denote the p×1p\times 1 vector (0k,1k,0p−2k)T\left(0_{k},1_{k},0_{p-2k}\right)^{T}, where 0k0_{k} denotes the k×1k\times 1 vector of zeros etc. Clearly ∣∣v∣∣2=k||v||^{2}=k and (A(τ)−A(τ′))v(A(\tau)-A(\tau^{\prime}))v will be a vector of the form (u,0)T(u,0)^{T} for some k×1k\times 1 vector u=(u1,…,uk)Tu=(u_{1},\dots,u_{k})^{T}. Moreover ur=∑s=1k(τr−τr′)ar,k+su_{r}=\sum_{s=1}^{k}(\tau_{r}-\tau_{r}^{\prime})a_{r,k+s} and hence

The proof is complete because ∣∣v∣∣2=k||v||^{2}=k. ∎

Let 1≤m<k,τ∈{0,1}k1\leq m<k,\tau\in\left\{0,1\right\}^{k} and τ′:=(0,…,0,τm,…,τk)\tau^{\prime}:=(0,\dots,0,\tau_{m},\dots,\tau_{k}). Then

The key is to note that one has the inequality D(N(0,A(τ))∣∣N(0,A(τ′)))≤Δ∣∣A(τ)−A(τ′)∣∣F2D\left(N(0,A(\tau))||N(0,A(\tau^{\prime}))\right)\leq\Delta||A(\tau)-A(\tau^{\prime})||^{2}_{F}, where ∣∣A∣∣F:=(∑i,jaij2)1/2||A||_{F}:=\left(\sum_{i,j}a_{ij}^{2}\right)^{1/2} denotes the Frobenius norm. The proof of this assertion can be found in [13, Proof of Lemma 6]. We can now bound

The Varshamov-Gilbert lemma (see for example [27, Lemma 4.7]) asserts the existence of a subset WW of {0,1}k\left\{0,1\right\}^{k} with ∣W∣≥exp⁡(k/8)|W|\geq\exp(k/8) such that Υ(τ,τ′)≥k/4\Upsilon(\tau,\tau^{\prime})\geq k/4 for all τ,τ′∈W\tau,\tau^{\prime}\in W with τ≠τ′\tau\neq\tau^{\prime}. Let F:={A(τ):τ∈W}F:=\left\{A(\tau):\tau\in W\right\}. From inequality (11) and Lemma VI.1, we get that

where PAP_{A} denotes the nn-fold product of the N(0,A)N(0,A) probability measure and Pˉ:=∑A∈FPA/∣W∣\bar{P}:=\sum_{A\in F}P_{A}/|W|. Now for 1≤m<k1\leq m<k and for t∈{0,1}k−m+1t\in\left\{0,1\right\}^{k-m+1}, let QtQ_{t} denote the nn-fold product of the N(0,A(0,…,0,t1,…,tk−m+1))N(0,A(0,\dots,0,t_{1},\dots,t_{k-m+1})) probability measure. Applying inequality (17), we get the quantity ∑A∈FD(PA∣∣Pˉ)/∣W∣\sum_{A\in F}D(P_{A}||\bar{P})/|W| is bounded from above by

Note that the above lower bound for Rn(α)R_{n}(\alpha) depends on kk and mm, which are constrained to satisfy 2k≤p2k\leq p and 1≤m<k1\leq m<k. To get the best lower bound, we need to optimize the right hand side of the above inequality over kk and mm. It should be obvious that in order to prove (35), it is enough to take k−m=n1/(2α+1)k-m=n^{1/(2\alpha+1)} and k=4Δn1/(2α+1)k=4\Delta n^{1/(2\alpha+1)}. The condition 2k≤p2k\leq p will be satisfied if p≥Cn1/(2α+1)p\geq Cn^{1/(2\alpha+1)} for a large enough CC. It is elementary to check that with these choices of kk and mm, inequality (35) is established.

VII A Packing Number Lower Bound

In this section, we shall prove that for every p∈[1,∞]p\in[1,\infty] the η\eta-packing number N(η;p,Γ)N(\eta;p,\Gamma) of Kd(Γ){\mathcal{K}}^{d}(\Gamma) under the LpL^{p} metric is at least exp⁡(c(η/Γ)(1−d)/2)\exp\left(c(\eta/\Gamma)^{(1-d)/2}\right) for a positive cc and sufficiently small η\eta. This means that there exist at least exp⁡(c(η/Γ)(1−d)/2)\exp\left(c(\eta/\Gamma)^{(1-d)/2}\right) sets in Kd(Γ){\mathcal{K}}^{d}(\Gamma) separated by at least η\eta in the LpL^{p} metric. This result was needed in the proof of Theorem V.1. Bronshtein [26, Theorem 4 and Remark 1] proved this for p=∞p=\infty (the case of the Hausdorff metric).

Fix p∈[1,∞]p\in[1,\infty]. There exist positive constants η0\eta_{0} and CC depending only on dd and pp such that for every η≤η0\eta\leq\eta_{0}, we have

Observe that by scaling, it is enough to prove for the case Γ=1\Gamma=1. We loosely follow Bronshtein [26, Proof of Theorem 4]. Fix ϵ∈(0,1)\epsilon\in(0,1). For each point x∈Sd−1x\in S^{d-1}, let SxS_{x} denote the supporting hyperplane to the unit ball BB at xx and let HxH_{x} be the hyperplane intersecting the sphere that is parallel to SxS_{x} and at a distance of ϵ\epsilon from SxS_{x}. Let Hx+H_{x}^{+} and Hx−H_{x}^{-} denote the two halfspaces bounded by HxH_{x} where we assume that Hx+H_{x}^{+} contains the origin. Let Tx:=Sd−1∩Hx−T_{x}:=S^{d-1}\cap H_{x}^{-} and Ax:=B∩HxA_{x}:=B\cap H_{x}, where BB stands for the unit ball. It can be checked that the (Euclidean) distance between xx and every point in TxT_{x} (and AxA_{x}) is less than or equal to 2ϵ\sqrt{2}\sqrt{\epsilon}. It follows that if the distance between two points xx and yy in Sd−1S^{d-1} is strictly larger than 22ϵ2\sqrt{2}\sqrt{\epsilon}, then the sets TxT_{x} and TyT_{y} are disjoint.

By standard results (see for example [26, Proof of Theorem 4] where it is referred to as Mikhlin’s result), there exist positive constants C1C_{1}, depending only on dd, and ϵ0\epsilon_{0} such that for every ϵ≤ϵ0\epsilon\leq\epsilon_{0}, there exist N≥C1(ϵ)1−dN\geq C_{1}(\sqrt{\epsilon})^{1-d} points x1,…,xNx_{1},\dots,x_{N} in Sd−1S^{d-1} such that the Euclidean distance between xix_{i} and xjx_{j} is strictly larger than 22ϵ2\sqrt{2}\sqrt{\epsilon} whenever i≠ji\neq j. From now on, we assume that ϵ≤ϵ0\epsilon\leq\epsilon_{0}. We then consider a mapping Φ:{0,1}N→Kd(1)\Phi:\left\{0,1\right\}^{N}\rightarrow{\mathcal{K}}^{d}(1), which is defined, for τ=(τ1,…,τN)∈{0,1}N\tau=(\tau_{1},\dots,\tau_{N})\in\left\{0,1\right\}^{N}, by

It must be clear that the Hausdorff distance between Φ(τ)\Phi(\tau) and Φ(τ′)\Phi(\tau^{\prime}) is not less than ϵ\epsilon (in fact, it is exactly equal to ϵ\epsilon) if τ≠τ′\tau\neq\tau^{\prime}. Thus, {Φ(τ):τ∈{0,1}N}\left\{\Phi(\tau):\tau\in\left\{0,1\right\}^{N}\right\} is an ϵ\epsilon-packing set for Kd(1){\mathcal{K}}^{d}(1) under the Hausdorff metric. However, it is not an ϵ\epsilon-packing set under the LpL^{p} metric. Indeed, the LpL^{p} distance between Φ(τ)\Phi(\tau) and Φ(τ′)\Phi(\tau^{\prime}) is not necessarily larger than ϵ\epsilon for all pairs (τ,τ′),τ≠τ′(\tau,\tau^{\prime}),\tau\neq\tau^{\prime}. The LpL^{p} distance between Φ(τ)\Phi(\tau) and Φ(τ′)\Phi(\tau^{\prime}) depends on the Hamming distance Υ(τ,τ′)=∑i{τi≠τi′}\Upsilon(\tau,\tau^{\prime})=\sum_{i}\left\{\tau_{i}\neq\tau_{i}^{\prime}\right\} between τ\tau and τ′\tau^{\prime}. We make the claim that

where C2C_{2} depends only on dd and pp. The claim will be proved later. Assuming it is true, we recall the Varshamov-Gilbert lemma from the previous section to assert the existence of a subset WW of {0,1}N\left\{0,1\right\}^{N} with ∣W∣≥exp⁡(N/8)|W|\geq\exp(N/8) such that Υ(τ,τ′)≥N/4\Upsilon(\tau,\tau^{\prime})\geq N/4 for all τ,τ′∈W\tau,\tau^{\prime}\in W with τ≠τ′\tau\neq\tau^{\prime}. Because N≥C1(ϵ)1−dN\geq C_{1}(\sqrt{\epsilon})^{1-d}, we get from (39) that for all τ,τ′∈W\tau,\tau^{\prime}\in W with τ≠τ′\tau\neq\tau^{\prime}, we have

Taking η:=C3ϵ\eta:=C_{3}\epsilon, we have obtained, for each η≤η0:=C3ϵ0\eta\leq\eta_{0}:=C_{3}\epsilon_{0}, an η\eta-packing subset of Kd(1){\mathcal{K}}^{d}(1) with size MM, where

The constant C4C_{4} only depends on dd and pp thereby proving (38).

It remains to prove the claim (39). Fix a point x∈Sd−1x\in S^{d-1} and ϵ∈(0,1)\epsilon\in(0,1). We first observe that it is enough to prove that

for a constant C5C_{5} depending on just dd and pp, where AxA_{x} and TxT_{x} are as defined in the beginning of the proof. This is because of the fact that for every τ,τ′∈W\tau,\tau^{\prime}\in W with τ≠τ′\tau\neq\tau^{\prime}, we can write

where I:={1≤i≤N:τi≠τi′}I:=\left\{1\leq i\leq N:\tau_{i}\neq\tau_{i}^{\prime}\right\}. The equality (41) is a consequence of the fact that the points x1,…,xNx_{1},\dots,x_{N} are chosen so that Tx1,…,TxNT_{x_{1}},\dots,T_{x_{N}} are disjoint.

We shall now prove the inequality (40) which will complete the proof. Let u0u_{0} denote the point in AxA_{x} that is closest to the origin. Also let u1u_{1} be a point in Ax∩Sd−1A_{x}\cap S^{d-1}. Let α\alpha denote the angle between u0u_{0} and u1u_{1}. Clearly, α\alpha does not depend on the choice of u1u_{1} and cos⁡α=1−ϵ\cos\alpha=1-\epsilon. Now let uu be a fixed unit vector and let θ\theta be the angle between the vectors uu and u0u_{0}. By elementary geometry, we deduce that

Because the difference of support functions only depends on the angle θ\theta, we can write, for a constant C6C_{6} depending only on dd, that

Now suppose β\beta is such that cos⁡(α−β)=1−ϵ/2\cos(\alpha-\beta)=1-\epsilon/2. Then from above, we get that

We shall show that sin⁡β≥(ϵ)/(22)\sin\beta\geq\left(\sqrt{\epsilon}\right)/(2\sqrt{2}) which will prove (40). Recall that cos⁡α=1−ϵ\cos\alpha=1-\epsilon. Thus

which when rearranged gives sin⁡β≥(ϵ)/(22)\sin\beta\geq\left(\sqrt{\epsilon}\right)/(2\sqrt{2}). The proof is complete. ∎

VIII Conclusion

By a simple application of convexity, we proved an inequality relating the minimax risk in multiple hypothesis testing problems to ff-divergences of the probability measures involved. This inequality is an extension of Fano’s inequality. As another corollary, we obtained a sharp inequality between total variation distance and ff-divergences. We also indicated how to control the quantity JfJ_{f} which appears in our lower bounds. This leads to important global lower bounds for the minimax risk. Two applications of our bounds are presented. In the first application, we used the bound (22) to prove a new lower bound (which turns to be rate-optimal) for the minimax risk of estimating a convex body from noisy measurements of the support function in nn directions. In the second application, we employed inequalities (11) and (17) to give a different proof of a recent lower bound for covariance matrix estimation due to Cai, Zhang and Zhou .

Acknowledgment

The author is indebted to David Pollard for his insight and also for numerous stimulating discussions which led to many of the ideas in this paper; to Andrew Barron for his constant encouragement and willingness to discuss his own work on minimax bounds. Thanks are also due to Aditya Mahajan for pointing out to the author that inequality (5) has the extension (4) for the case of non-uniform priors ww; to an anonymous referee for helpful comments, for pointing out an error and for Example IV.5; to Richard Gardner for comments that greatly improved the quality of the paper and to Alexander Gushchin for informing the author about his paper and for sending him a scanned copy of it.

References