Abstract:
We obtain order estimates for the Kolmogorov widths of periodic Sobolev classes defined by constraints on the Lpj-norm of the rjth derivative with respect to the jth variable for 1⩽j⩽d.
Bibliography: 31 titles.
We study the Kolmogorov widths of the periodic Sobolev class on the d-dimensional torus Td defined by the constraints
‖
on the partial derivatives. This class of functions is an example of the intersection of several Sobolev classes defined by constraints on one of the partial derivatives (see [1]–[3]). Functional classes of this kind on \mathbb R^d were studied in [4], § 6. Sufficient conditions for an embedding of such a class in the Lorentz space were obtained; the particular case p_1=\dots=p_d was considered earlier in [5]. Anisotropic Sobolev classes on a domain \Omega \subset \mathbb R^d defined by constraints on \biggl\| \dfrac{\partial^{r_j}}{\partial x^{r_j}_j}f\biggr\|_{L_{p_j}(\Omega)} (j=1,\dots,d) and the norm of the function f in the space L_{p_0} with a special weight were studied in [6], where it was assumed that
Embedding theorems in the weighted space L_q were obtained, and some (not order-sharp in general) estimates for the Kolmogorov widths were put forward. Here we consider nonweighted periodic classes, where condition (1.2) is not assumed, and the width estimates we obtain are order sharp.
The class of functions with constraints of the form (1.1) is an example of an anisotropic Sobolev class. Anisotropic function classes of another type (defined by constraints on derivatives in a mixed norm) were studied in [1] and [7]–[11].
Definition 1. Let X be a normed linear space, and let M\subset X and n\in \mathbb Z_+. Then the Kolmogorov n-width of M in X is defined by
here \mathcal L_n(X) is the class of all subspaces in X of dimension \leqslant n.
Widths of finite-dimensional balls were estimated in [12]–[17]. For a historical account of this problem, see also [18]–[20].
The papers [2], [3] and [21]–[24] were concerned with the problem of estimates for widths of a periodic Sobolev class on \mathbb{T}^d:=[0,2\pi]^d defined by a constraint on the L_p-norm of one or several (fractional) partial derivatives, and also for widths of the intersection of some periodic Sobolev classes on \mathbb{T}^1; see also [25] and [20]. The result of [3] on widths of an intersection of one-dimensional Sobolev classes was extended in [26] to the case of ‘small smoothness’ for q>2, with the exception of some ‘limiting’ cases.
Recall the definition of the Weyl derivative of a periodic function (see, for example, [18], Ch. 2, § 2). For d\in \mathbb N, d\geqslant 2, let \mathbb{T}^d=[0,2\pi]^d. We denote the space of distributions on \mathbb{T}^d by \mathcal S'(\mathbb{T}^d) (the corresponding space of test functions consists of infinitely smooth periodic functions). To each distribution f\in \mathcal S'(\mathbb{T}^d) there corresponds its Fourier series expansion f=\sum_{\overline{k}\in \mathbb Z^d} c_{\overline{k}}(f) e^{i(\overline{k},\cdot)} with convergence in the topology of \mathcal S'(\mathbb{T}^d); here and in what follows (\cdot,\cdot) is the standard inner product on \mathbb R^d. We set
Let r_j>0, 1\leqslant j\leqslant d. The Weyl derivative of order r_j with respect to x_j of a distribution f\in \mathring{\mathcal S}'(\mathbb{T}^d) is defined by
In the present paper we consider the order estimate problem for the Kolmogorov width of the class W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) in the space L_q(\mathbb{T}^d).
Given \overline{a}=(a_1,\dots,a_d) \in \mathbb R^d, the harmonic mean of a_1,\dots,a_d is defined by
For \overline{a}=(a_1,\dots,a_d)\in \mathbb R^d and \overline{b}=(b_1,\dots,b_d)\in \mathbb R^d we set \overline{a}\circ\overline{b}=(a_1b_1,\dots,a_db_d).
From Theorem 1 in [1] it follows that the set W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) is bounded in L_q(\mathbb{T}^d) if and only if
The above embedding is compact if this inequality is strict (see Theorem 5 in [1]).
Let us formulate some theorems on estimates for widths.
First we consider the case involving some additional constraints on the parameters. Then estimates of widths are explicitly found (except in the case where certain ‘limiting’ relations hold between the parameters).
Let us introduce some notation for order equalities and inequalities. Let X and Y be sets, and let f_1,f_2\colon X\times Y\to \mathbb{R}_+. We write f_1(x,y)\underset{y}{\lesssim} f_2(x,y) (or f_2(x,y)\underset{y}{\gtrsim} f_1(x,y) if for each y\in Y there exists c(y)>0 such that f_1(x,y)\leqslant c(y)f_2(x,y) for all x\in X; f_1(x,y)\underset{y}{\asymp} f_2(x,y) if f_1(x,y) \underset{y}{\lesssim} f_2(x,y) and f_2(x,y)\underset{y}{\lesssim} f_1(x,y).
Theorem 1. Let d\in \mathbb N, d\geqslant 2, 1<q<\infty, 1<p_j<\infty and r_j>0, j=1,\dots,d, and let \frac{\langle \overline{r}\rangle}{d}+\frac 1q-\frac{\langle \overline{r}\rangle}{\langle \overline{p}\circ\overline{r}\rangle} > 0. Assume that
3. Let 2<q<\infty. Assume that there exists i\in \{1,\dots,d\} such that p_i<q. Also set \theta_1=\frac{\langle \overline{r}\rangle}{d}, \theta_2=\frac{\langle \overline{r}\rangle}{d}+\frac 12-\frac{\langle \overline{r}\rangle}{\langle \overline{p}\circ\overline{r}\rangle} and \theta_3=\frac q2\bigl( \frac{\langle \overline{r}\rangle}{d}+\frac 1q-\frac{\langle \overline{r}\rangle}{\langle \overline{p}\circ \overline{r}\rangle}\bigr).
\begin{equation*}
d_n(W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d),L_q(\mathbb{T}^d)) \underset{\overline{r}, \overline{p}, q, d}{\asymp} n^{-\theta_{j_*}}.
\end{equation*}
\notag
Remark 1. We will also show that in the case where p_j\geqslant q for 1\leqslant j\leqslant d the assertion of the theorem also holds without condition (1.3).
Now we consider the general case where (1.3) is not assumed to hold.
In what follows we set \max \varnothing:=-\infty.
Theorem 2. Let d\in \mathbb N, d\geqslant 2, 1<q<\infty, 1<p_j<\infty and r_j>0, j=1, \dots,d, and let \frac{\langle \overline{r}\rangle}{d}+\frac 1q-\frac{\langle \overline{r}\rangle}{\langle \overline{p}\circ\overline{r}\rangle} > 0.
Now consider the case where condition (1.3) is not satisfied.
Theorem 3. Let d\in \mathbb N, d\geqslant 2, r_k>0 and 1<p_k\leqslant q<\infty for k=1,\dots,d, and assume that there exists j\in \{1,\dots,d\} such that
Then W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) is not compactly embedded in L_q(\mathbb{T}^d).
For d=2, if condition (1.3) is not met, then the orders of widths can be calculated explicitly. Assume without loss of generality that p_1>p_2. Then r_2\leqslant \frac{1}{p_2} -\frac{1}{p_1}. By Remark 1 and Theorem 3 it suffices to consider the case where p_2<q<p_1.
Theorem 4. Let 1<p_2<q<p_1<\infty, r_1>0 and r_2>0. Assume that
1. Let 1<q\leqslant 2. Let \lambda\in (0,1) be defined by \frac 1q=\frac{1-\lambda}{p_1}+ \frac{\lambda}{p_2}. Assume that \frac{\langle \overline{r}\rangle}{2} \ne \lambda r_2. Then
2. Let 2<q<\infty. Let \lambda\in (0,1) be defined by \frac 1q= \frac{1-\lambda}{p_1}+\frac{\lambda}{p_2}, and let \widehat s be defined by \widehat s\bigl(1-\frac{r_2(1-2/q)}{1/p_2-1/p_1}\bigr)=1.
and \mathcal T_{\overline{m}}=\operatorname{span} \{e^{i(\overline{k},\, \cdot)}\}_{\overline{k}\in \square_{\overline{m}}}. Given f(\cdot)=\sum_{\overline{k}\in \mathring{\mathbb Z}^d} c_{\overline{k}}(f)e^{i(\overline{k},\, \cdot)}, we define
Theorem 5 (Littlewood–Paley theorem; see [27], § 1.5.2; [18], Ch. 2, § 2.3, Theorem 15; [7], Ch. III, § 15.2; and [8]). Let 1<q<\infty. Then f\in L_q(\mathbb{T}^d) if and only if Pf\in L_q(\mathbb{T}^d); in addition,
Theorem 6 (see [20], Theorem 3.3.1, and [18], Ch. 2, § 2.3, Theorem 18 for r_j\geqslant 0). Let 1<p_j<\infty and r_j\in \mathbb R. Then for f\in \mathcal T_{\overline{m}},
For arbitrary r_j\in \mathbb R, this result is a consequence of Marcinkiewicz’s multiplier theorem (see [27], § 1.5.3, and [7], Ch. III, § 15.3).
Theorem 7 (see [3], Theorem B, and [28], vol. 2, Ch. X, Theorem 7.5). There exists an isomorphism A\colon \mathcal T_{\overline{m}} \to \mathbb R^{2^m} such that for all q\in (1,\infty) and f\in \mathcal T_{\overline{m}},
We denote the space \mathbb{R}^N equipped with this norm by l_q^N, and B_q^N is the unit ball in l_q^N.
The widths d_n(B_p^N,l_q^N) were estimated by Pietsch, Stesin, Kashin, Gluskin and Garnaev (see [12]–[17]). In what follows we present results on width estimates in a number of cases considered below.
Theorem 8 ([16]). Let 1\leqslant p\leqslant q<\infty and 0\leqslant n\leqslant N/2.
1. Let 1\leqslant q\leqslant 2. Then d_n(B_p^N,l_q^N) \asymp 1.
2. Let 2<q<\infty and \omega_{pq}=\min \bigl\{1,\frac{1/p-1/q}{1/2-1/q}\bigr\}. Then
Order estimates for Kolmogorov widths of intersections of N-dimensional balls were obtained in [2] for N=2n and in [29] for N\geqslant 2n. In [29] an order estimate was written down explicitly under the additional assumption that none of these balls contains another. In [26], Proposition 1, an estimate for the intersection of a finite number of balls was given in a general case. Let us formulate this result.
Theorem 10 (see [26], Proposition 1). Let A be a nonempty finite set, let 1\leqslant p_\alpha\leqslant \infty and \nu_\alpha>0, \alpha \in A, let
The original formulation of Proposition 1 in [26] involved nonstrict inequalities in place of the strict ones p_\alpha> q, p_\beta< q, p_\alpha> 2 and p_\beta< 2 in (2.5) and (2.6); the resulting estimate remains the same.
For k\in \{1,\dots,N\} let the sets V_k\subset \mathbb R^N be defined by
where \widehat{x}_j=1 for 1\leqslant j\leqslant k, \widehat{x}_j=0 for k+1\leqslant j\leqslant N and S_N is the permutation group on N elements. Note that V_1 =B_1^N and V_N=B_\infty^N.
For 2\leqslant q<\infty lower estimates for d_n(V_k,l_q^N) were obtained by Gluskin [15].
Theorem 11 ([15]). Let 2\leqslant q<\infty and 1\leqslant k\leqslant N. Then
The following result was obtained by Gluskin [30] (with a constant depending on q in the order inequality) and by Malykhin and Ryutin [31] (with a constant independent of q). It was noted in [30], p. 39, that the equality d_n(V_k,l_1^N)=\min\{k,N-n\} is due to Galeev.
Theorem 12 (see [30] and [31]). Let 1\leqslant q\leqslant 2, n\leqslant N/2. Then
Proof. In view of (3.1) it suffices to prove the lower estimates for the widths d_n(M_0,l_q^N).
In part 1 we use the embedding \nu_{\alpha_*} B^N_1 \subset M_0 and Theorem 8, and in part 2, the embedding \nu_{\alpha_*} N^{-1/p_{\alpha_*}} B^N_{\infty} \subset M_0 and Theorem 9.
In part 3 let the number l be defined by {\nu_{\alpha_*}}/{\nu_{\beta_*}}= l^{1/p_{\alpha_*}-1/p_{\beta_*}}; we also set k=\lceil l\rceil. From (3.3) it follows that 1\leqslant l\leqslant N, and so 1\leqslant k\leqslant N. We claim that \nu_{\alpha_*} ^{1-\lambda_{\alpha_*,\beta_*}}\nu_{\beta_*}^{\lambda_{\alpha_*,\beta_*}} k^{-1/q}V_k \subset 2M_0. Now the lower estimate for d_n(M_0,l_q^N) is secured by (2.8). It suffices to verify that for each \gamma\in A
that is, \nu_{\alpha_*} l^{1/p_\gamma-1/p_{\alpha_*}} \leqslant \nu_\gamma (see (2.3) and the definition of l). The last inequality follows from (3.2) by the same argument as in [29], p. 6.
Lemma 2. Let 2< q<\infty and p_\alpha\notin \{2,q\} for each \alpha\in A, let N^{2/q}\leqslant n \leqslant N/2, and let the set M_0 be defined by (2.2).
1. Let p_{\alpha_*} < 2 and \nu_{\alpha_*} \leqslant \nu_\beta for each \beta \in A. Then
Proof. By (3.5) it suffices to prove the lower estimate.
In part 1 we use the embedding \nu_{\alpha_*}B_1^N \subset M_0 and Theorem 8, and in part 2 we employ the embedding \nu_{\alpha_*}N^{-1/p_{\alpha_*}}B_\infty^N \subset M_0 and Theorem 9.
In this case we have 1\leqslant l\leqslant N, 1\leqslant k\leqslant N and n \leqslant N^{2/q} k^{1-2/q}. We claim that \nu_{\alpha_*}k^{-1/p_{\alpha_*}}V_k \,{\subset}\, 2M_0. As a result, estimate (3.7) follows from (2.7). The claim follows from the inequality \nu_{\alpha_*} l^{1/p_\beta-1/p_{\alpha_*}} \leqslant \nu_\beta for \beta\in A, which is in turn secured by (3.6).
In part 4 we set k=\lceil l\rceil. From (3.8) we obtain
\begin{equation*}
(n^{1/2}N^{-1/q})^{\frac{1}{1/2-1/q}}\leqslant l\leqslant N.
\end{equation*}
\notag
Hence 1\!\leqslant\! k\leqslant\! N and n \!\leqslant\! N^{2/q} k^{1-2/q}. Now we show that \nu_{\alpha_*}^{1-\lambda_{\alpha_*,\beta_*}} \nu_{\beta_*}^{\lambda_{\alpha_*,\beta_*}} k^{-1/q}V_k\! \subset 2M_0 and use (2.7). To do this, it suffices to verify that (3.4) holds for each \gamma\in A; in view of (2.3) and (3.11) this is equivalent to the inequality \nu_{\alpha_*} l^{1/p_\gamma-1/p_{\alpha_*}} \leqslant \nu_\gamma. It follows from (3.2) by the same argument as in [29], pp. 11–12.
In part 5 we set k=\lfloor l\rfloor. From (3.10) we obtain
Hence 1\!\leqslant\! k\!\leqslant\! N and n \!\geqslant\! N^{2/q} k^{1-2/q}. Now we show that \nu_{\alpha_*}^{1-\widetilde\lambda_{\alpha_*,\beta_*}} \nu_{\beta_*}^{\widetilde\lambda_{\alpha_*,\beta_*}} k^{-1/2}V_k \!\subset\! 2M_0 and use (2.7). To do this it suffices to verify that for each \gamma\in A,
in view of (2.4) and (3.11) this is equivalent to the inequality \nu_{\alpha_*} l^{1/p_\gamma-1/p_{\alpha_*}} \leqslant \nu_\gamma. It is secured by (3.9), where we proceed as in [29], pp. 12–13.
The following two results will be used to reduce the problem of estimates for widths of W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) to estimates for widths of finite-dimensional balls. Recall that for \overline{m}\in \mathbb N^d the number m was defined in (2.1).
Let the function h and the set D be defined by (1.6) and (1.7) (for q\leqslant 2 and q>2 alike).
Lemma 5. Let (\alpha_1^*,\dots,\alpha_d^*) be a minimum point of the function h on the set D, and let h(\alpha_1^*,\dots,\alpha_d^*)>0. Let the numbers C_{\overline{m}} be defined by (4.3). Then for each N\in \mathbb N,
where t=t_1+\dots+t_d. We also set \alpha_j={t_j}/{t}, 1\leqslant j\leqslant d. Comparing (4.7) and the function h, we have \varphi(t_1,\dots,t_d)=t \cdot h(\alpha_1,\dots,\alpha_d), (\alpha_1,\dots,\alpha_d)\in D. Setting E_t=\{(t_1,\dots, t_{d-1})\colon t_1+\dots+t_{d-1}\leqslant t,\, t_j\geqslant 0,\, 1\leqslant j\leqslant d-1\} we find that
If h has a unique minimum point on D, then (N\alpha_1^*,\dots,N\alpha_d^*) is a unique minimum point of the function \varphi on G_N:=\{(t_1,\dots,t_d)\colon t_1+\cdots+t_d\geqslant N, t_j\geqslant 0, 1\leqslant j\leqslant d\}. By (4.7) there exists b=b(\overline{p},q,\overline{r},d)> 0 such that
the second equality is secured by (4.4) and (4.5).
The lemma is proved.
Lemma 7. Assume that \min_D h>0, and let k_{\overline{m}}\in \mathbb Z_+, \overline{m}\in \mathbb N^d, be such that \sum_{\overline{m}\in \mathbb N^d}k_{\overline{m}}\leqslant Cn for some constant C\in \mathbb N. Then
Proof. We have \min_{D}h>0, and so it follows from (4.8) that the partial sums S_Nf:=\sum_{m\leqslant N} \delta_{\overline{m}}f form a Cauchy sequence in L_q(\mathbb{T}^d). On the other hand S_Nf\underset{N\to \infty}{\to} f in \mathcal S'(\mathbb{T}^d). Hence f\in L_q(\mathbb{T}^d) and S_Nf\underset{N\to \infty}{\to} f in L_q(\mathbb{T}^d), which implies that
Proof of Theorem 2. First we prove the upper estimate under the assumption that \min_{D}h>0. Then we prove the lower estimate, and obtain in passing that if \min_{D}h\leqslant 0, then W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) is not compact in L_q(\mathbb{T}^d). Hence, under the assumptions of Theorem 2 the inequality \min_{D}h>0 holds automatically, since the embedding is compact because
We set q_*=\min\{q,2\}. Let \overline{m}_*=(m_1^*,\dots,m_d^*)\in \mathbb R_+^d, 2^{m_*}\in [n,n^{q_*/2}] and \varepsilon>0 (\overline{m}_* and \varepsilon will be chosen below depending on \overline{p}, q, \overline{r} and d). We also set
Setting c_*\!=\!\min_{\widetilde D_{q/2}}\widetilde h and \log x\! :=\!\log_2 x, and using (4.3) and (4.8) for N\!=\!\lfloor\frac q2 \log n\rfloor, we have
which gives (4.14). If c_*=\widetilde h(\widehat \alpha_1, \dots,\widehat \alpha_d,\widehat s), then the function \widetilde h has a unique minimum point on \widetilde D_{q/2}; by Lemma 6, the function h has a unique minimum point on D. Applying (4.9), we arrive at (4.14) again.
Let us now estimate S_{2,\varepsilon}. First consider the case \varepsilon=0. We have
\begin{equation}
\psi_n(t_1,\dots,t_d,t)=\widetilde h \biggl(\frac{t_1}{\log n},\dots,\frac{t_d}{\log n}, \frac{t}{\log n}\biggr)\cdot\log n.
\end{equation}
\tag{4.16}
The function \widetilde h has a unique minimum point on the set \widetilde D, and so the function f_n(t_1, \dots,t_d):=\psi_n(t_1,\dots,t_d,t_1+\dots+t_d) also has a unique minimum point on G_n, and this point has the form (\widehat \alpha_1,\dots,\widehat \alpha_d)\log n. In addition, if \widehat s=\widehat \alpha_1+\dots+\widehat \alpha_d>1, then (\widehat \alpha_1,\dots,\widehat \alpha_d)\log n is the unique minimum point of the function f_n on the set
(the greatest possible \varepsilon for which (4.19) holds depends on \overline{p}, q, \overline{r} and d).
Let us use Theorems 8–10 and (4.13). We have 2^{m_*}\in [n,n^{q/2}], and so for sufficiently small \varepsilon>0 and for n\cdot 2^{-\varepsilon|\overline{m}-\overline{m}_*|}\leqslant 2^m \leqslant n^{q/2} we have k_n \asymp {n\cdot 2^{-\varepsilon|\overline{m}-\overline{m}_*|}}. Hence for some b=b(\overline{p},\overline{r},q,d)>0,
for small \varepsilon >0. Now from (4.14) we have the required upper estimate for the width.
We prove the lower estimate. Again, we consider the more involved case {q>2}. Let \overline{m} \in \mathbb N^d, 2n\leqslant 2^m \leqslant n^{q/2}, and let \alpha_j=m_j/\log n for 1\leqslant j\leqslant d and {s=\alpha_1+\dots+\alpha_d}. From Lemma 3 and Theorems 8–10 we obtain
Let \overline{m}_*\in G_n be defined by (4.17), and let \overline{m}\in G_n be a nearest point to \overline{m}_* (with respect to the Euclidean norm) with positive integer coordinates such that m\geqslant \log(2n). Then
from which the required lower estimate for the width follows.
If \min_D h\leqslant 0, then \min_{\widetilde D} \widetilde h\leqslant\min_{\widetilde D_{q/2}} \widetilde h\leqslant 0 (see Lemma 6), so that by (4.20) and (4.21) we have
By Theorem 2 it suffices to find a minimum point of the function h on D for {q\leqslant 2} and of the function \widetilde h on \widetilde D for q>2.
Consider the more involved case q>2 (the argument for q\leqslant 2 is similar and uses Lemma 1).
First we prove the theorem under the additional assumption that p_i\notin \{2,q\}, 1\leqslant i\leqslant d. We have I=I', J=J' and K=K'.
As above, let the numbers \lambda_{i,j} and \mu_{i,j} be defined by (1.9).
Lemma 8. Let p_i\notin \{2,q\} and \alpha_i\geqslant 0(1\leqslant i\leqslant d), let \alpha_1+\dots+\alpha_d=s, and assume that 1\leqslant s\leqslant q/2.
1. Let j\in I. Then \widetilde h(\alpha_1,\dots,\alpha_d,s)=r_j\alpha_j if and only if \alpha_jr_j-\alpha_ir_i\geqslant 0, 1\leqslant i\leqslant d.
Proof.Necessity. Part 1 holds because we have \alpha_jr_j\geqslant \alpha_ir_i for i\in I and r_j\alpha_j \geqslant (1- \lambda_{j,i})r_j\alpha_j+ \lambda_{j,i}r_i\alpha_i for i\in J\cup K. For part 2 we invoke the inequalities
The analysis of part 5 is similar to that of part 4.
Sufficiency. Consider part 1 (the other assertions of the theorem are dealt with similarly). Let \alpha_1^*+\dots+\alpha_d^*=s^*\in [1,q/2], \alpha_j^*\geqslant 0 (1\leqslant j\leqslant d), and let r_j\alpha_j^*\geqslant r_i\alpha_i^* for all i=1,\dots,d, but \widetilde h(\alpha_1^*,\dots, \alpha_d^*,s^*) > r_j\alpha_j^*. There exist c>0 and an open subset U of the set
such that for each (\alpha_1,\dots, \alpha_d,s)\in U,
\begin{equation}
\widetilde h(\alpha_1,\dots,\alpha_d,s)-r_j\alpha_j \geqslant c.
\end{equation}
\tag{5.1}
For sufficiently large n\in \mathbb N there exists (\alpha_1,\dots,\alpha_d,s)\in U such that m_k:=\alpha_k\log n \in \mathbb N (1\leqslant k\leqslant d) and m\geqslant \log(2n) (recall that m:=m_1+\dots+m_d). Hence
\begin{equation}
\alpha^3_j=\frac{q}{2}\alpha_j^2\quad\text{and} \quad \alpha^4_j=\frac{q}{2}\alpha_1^j, \qquad 1\leqslant j\leqslant d.
\end{equation}
\tag{5.4}
Note that by (1.3) we have \alpha^k_j>0 for 1\leqslant k\leqslant 4 and 1\leqslant j\leqslant d.
We claim that the minimum of the function \widetilde h on \widetilde D can only be attained at \xi_1, \xi_2 or \xi_3. We will also evaluate \widetilde h at these points.
We need the following notation. Let \widehat l_{m,t}, 1\leqslant m,t\leqslant 4, m\ne t, be the line segments between \xi_m and \xi_t. For 1\leqslant k\leqslant d we define line segments l_k, \widetilde l_k and \widehat l_k as follows: l_k is defined by
Note that \xi_1\in l_k, \xi_2\in \widehat l_k and \xi_3\in \widetilde l_k are endpoints of the corresponding segments; in addition, the systems of equalities and inequalities (5.5)–(5.7) have the same matrix. Hence the segments l_k, \widetilde l_k and \widehat l_k have the form
The set \widetilde D is partitioned into polytopes on which \widetilde h is an affine function. For such a polytope we now find the set of its vertices with positive \alpha_j; we will also indicate the set of edges outgoing of these vertices.
Let V be such a polytope.
1. Let V=\{(\alpha_1,\dots,\alpha_d,s)\in \widetilde D\colon \widetilde h(\alpha_1,\dots, \alpha_d,s)=r_j\alpha_j\}, where j\in I. We use part 1 of Lemma 8. At vertices of V with positive coordinates we have r_1\alpha_1=\dots= r_d\alpha_d, where \alpha_1+\dots+\alpha_d=s=1 or \alpha_1+\dots+\alpha_d=s=q/2. These equalities define the points \xi_1 and \xi_4. The edges going out of \xi_1 are given by
For s=1 we have the point \xi_1, and for s=q/2 we have \xi_3.
An edge going out of \xi_1 is either l_k (k=1,\dots,d, k\ne j; see (5.5) and part 2 of Lemma 8), or the line segment \widehat l_{1,3} between \xi_1 and \xi_3. By (5.14), for {s=1} we have \widetilde h(\alpha_1,\dots, \alpha_d,1)=r_j\alpha_j, and so from (5.10) and (5.11) we find that {\widetilde h(\xi_1)<\widetilde h(\xi_{1,k})}, k\ne j. Hence if \widetilde h(\xi_1)\leqslant \widetilde h(\xi_3), then \xi_1 is a minimum point of \widetilde h on V and {\widetilde h (\xi_1)={\langle \overline{r}\rangle}/{d}}.
An edge going out of the point \xi_3 is either \widehat l_{1,3}, or the segment \widetilde l_k (k=1,\dots,d, k\ne j; see (5.7)). Let \xi_{3,k}\ne \xi_3 be an endpoint of \widetilde l_k. From (5.8), (5.10), (5.11) and (5.14) we obtain
For s=1 we have the point \xi_2, and for s=q/2 we have \xi_3.
An edge going out of \xi_3 is either \widetilde l_k (k\ne j; see (5.7) and part 3 of Lemma 8), or the segment \widehat l_{2,3}. An edge going out of \xi_2 is either \widehat l_{2,3}, or a segment \widehat l_k (k\ne j; see (5.6)).
Let \xi_{2,k}\ne \xi_2 be an endpoint of the edge \widehat l_k and \xi_{3,k}\ne \xi_3 be an endpoint of \widetilde l_k. From (5.8), (5.10), (5.11) and (5.17) we obtain \widetilde h(\xi_2)< \widetilde h(\xi_{2,k}) and \widetilde h(\xi_3)< \widetilde h(\xi_{3,k}).
For s=1 this is the equality \alpha_ir_i-\alpha_jr_j=0, and so we obtain the point \xi_1 again. For s=q/2 we have \alpha_ir_i-\alpha_jr_j=\frac q2 (1/p_i-1/p_j); now from (5.20) and (5.21) we obtain
An edge going out of \xi_1 is either l_k (k\ne i, j), \widehat l_{1,3}, or \widehat l_{1,4}. On the edges l_k and \widehat l_{1,4} we have r_i\alpha_i=r_j\alpha_j, and the function \widetilde h coincides with \alpha_ir_i. Now from (5.10) and (5.11) we obtain \widetilde h(\xi_1)< \widetilde h(\xi_4) and \widetilde h(\xi_1)< \widetilde h(\xi_{1,k}), k\ne i,j. Hence if \widetilde h(\xi_1)\leqslant \widetilde h(\xi_3), then \min_{V} \widetilde h=\widetilde h(\xi_1)={\langle \overline{r} \rangle}/{d}.
An edge going out of \xi_3 is either \widetilde l_k (k\ne i, j), \widehat l_{1,3}, or \widehat l_{3,4}. On the edges \widetilde l_k we have r_i\alpha_i-{q}/(2p_i)=r_j\alpha_j-q/(2p_j), and so on \widetilde l_k the function \widetilde h is
Hence by (5.8), (5.10) and (5.11)\widetilde h(\xi_3)<\widetilde h(\xi_{3,k}) for k\ne i,j. So if \widetilde h(\xi_3)\leqslant \widetilde h(\xi_1), then by the inequality \widetilde h(\xi_1) < \widetilde h(\xi_4) we have
(recall the notation in the statement of Theorem 1); by the assumptions of the theorem there exists j_*\in \{1,2,3\} such that \theta_{j_*}=\min_{j\ne j_*} \theta_j, and therefore the minimum in (5.23) is attained at a unique point.
So the set \widetilde D falls into closed polytopes V^{(k)}, 1\leqslant k\leqslant k_0, where each V^{(k)} is defined by the assumptions of cases 1–5 above.
Now consider the general case where it is possible that p_i\in \{2, q\}. We define \overline{p}^N=(p_1^N,\dots,p_d^N) as follows. If p_j\notin \{2,q\}, then we set p_j^N=p_j. If p_j=q, then we set p_j^N=q+1/N, and if p_j=2, then p_j^N=2 \pm 1/N (the sign is the same for all j; the sign is negative for K=\{1,\dots,d\}, otherwise we take the positive sign). For large N we have p_j^N\notin \{2, q\}, 1\leqslant j\leqslant d. Let the function \widetilde h^N be defined like \widetilde h, but with p_j replaced by p_j^N. Then \widetilde h^N converges uniformly to \widetilde h on \widetilde D. If \overline{p} satisfies condition (1.3), then \overline{p}^N for large N also does.
Let \xi_t (1\leqslant t\leqslant 4) be given by (5.2)–(5.4). We define a set T\subset \{1,2,3\} as follows: if I=\{1,\dots,d\}, then T=\{1\}; if I \ne \{1,\dots,d\} and I\cup J=\{1,\dots,d\}\ne K, then T=\{1,3\}; if K= \{1,\dots,d\}, then T=\{2,3\}; otherwise, T=\{1,2,3\}. Note that all points \xi_t, t\in T, are distinct.
We claim that \min_{\widetilde D} \widetilde h=\min_{t\in T} \widetilde h(\xi_t). Indeed, let \xi_t^N and T_N be defined similarly to \xi_t and T with \overline{p} replaced by \overline{p}^N. Then \xi_t^N\underset{N\to \infty}{\to} \xi_t, and for large N we have T_N=T (we consider only such N in what follows). By the above \min_{\widetilde D} \widetilde h^N=\min_{t\in T}\widetilde h^N(\xi_t^N). There exist t_*\in T and a subsequence \{N_m\}_{m\in \mathbb N} such that \min_{t\in T}\widetilde h^{N_m}(\xi_t^{N_m})=\widetilde h^{N_m}(\xi_{t_*}^{N_m}). The functions \widetilde h^N converge uniformly to \widetilde h on \widetilde D and \xi_t^N\underset{N\to \infty}{\to} \xi_t, and thus \min_{\widetilde D} \widetilde h=\widetilde h(\xi_{t_*}). The explicit form of \widetilde h(\xi_{t_*}) also follows from the formulae for \widetilde h^{N_m}(\xi_{t_*}^{N_m}); see (5.13), (5.16), (5.18), (5.22), and (5.23).
Let us now show that \xi_{t_*} is a unique minimum point of \widetilde h. It suffices to verify that there exists a positive constant c=c(\overline{p},q,\overline{r},d) such that for large m\in \mathbb N,
(here |\cdot| is the Euclidean norm on \mathbb R^{d+1}). Letting m\to \infty, this establishes the inequality \widetilde h(\xi)-\widetilde h(\xi_{t_*})\geqslant c|\xi-\xi_{t_*}|, \xi\in \widetilde D.
Let us prove (5.24). Again, we consider the polytope V=V(m) containing the vertex \xi_{t_*}^{N_m}; the function \widetilde h^{N_m} is affine on this polytope (see the above analysis of cases 1–5). It suffices to show that (5.24) holds for points \xi on each edge going out of the vertex \xi_{t_*}^{N_m}. Indeed, by the assumptions of the theorem \widetilde h(\xi_{t_*}) < \widetilde h(\xi_t), t\in T\setminus \{t_*\}. Hence, since \widetilde h^N converges uniformly to \widetilde h on \widetilde D and \xi_t^N converges to \xi_t, for large m we have
Hence (5.24) holds on the edge between \xi_{t_*}^{N_m} and \xi^{N_m}_t, t\in T \setminus \{t_*\}. There can also be an edge from \xi_{t_*}^{N_m} connecting it with \xi_4^{N_m} (in this case \xi_1^{N_m} \in V; see the analysis of cases 1 and 4); we also have
Hence (5.24) also holds on this edge. Note also that the edge from \xi^{N_m}_{t_*} can coincide with l_k^m, \widetilde l_k^m or \widehat l_k^m (these line segments are given by formulae similar to (5.5), (5.7) and (5.6), with \overline{p} replaced by \overline{p}^{N_m}). In the analysis of these cases it was shown that the function \widetilde h^{N_m} has the form \alpha_jr_j+\mathrm{const} on l_k^m, \widetilde l_k^m and \widehat l_k^m, and s\in \{1, q/2\} on these edges. In view of (5.8), (5.10) and (5.11) we see that (5.24) holds on the edges l_k^m, \widetilde l_k^m and \widehat l_k^m going out of \xi^{N_m}_{t_*}.
First we show that if \frac{\langle \overline{r}\rangle}{d}+\frac 1q-\frac{\langle \overline{r}\rangle}{\langle \overline{r}\circ \overline{p}\rangle}\leqslant 0, then W^{\overline{r}}_{\overline{p}}(\mathbb{T}^d) is not compact in L_q(\mathbb{T}^d). We use induction on d. For d=1 this result is known.
For the step of induction from d-1 to d we assume that
We set \overline{r}_j=(r_1,\dots,r_{j-1},r_{j+1},\dots,r_d) and \overline{p}_j=(p_1, \dots,p_{j-1},p_{j+1},\dots,p_d). Condition (6.1) is equivalent to the inequality
and W^{\overline{r}_j}_{\overline{p}_j}(\mathbb{T}^{d-1}) is not compactly embedded in L_q(\mathbb{T}^{d-1}) by the induction assumption. Hence W^{\overline{r}}_{\overline{p}}(\mathbb{T}^{d}) is not compactly embedded in L_q(\mathbb{T}^{d}).
Let p_j>q. Setting \overline{p}^*=(p_1,\dots,p_{j-1},q,p_{j+1},\dots,p_d) we have
(the right-hand side is a bounded set in L_q(\mathbb{T}^{d})). This contradiction shows that the case p_j>q is impossible.
Proof of Theorem 3. Let j\in \{1,\dots,d\} satisfy (6.1) (which is equivalent to (6.2)). By the assumptions of the theorem p_j\leqslant q. Hence (6.3) holds. By the above W^{\overline{r}_j}_{\overline{p}_j}(\mathbb{T}^{d-1}) is not compactly embedded in L_q(\mathbb{T}^{d-1}); hence W^{\overline{r}}_{\overline{p}}(\mathbb{T}^{d}) is not compactly embedded in L_q(\mathbb{T}^{d}).
The theorem is proved.
Proof of Theorem 4. We apply Theorem 2 and write out the function h for q\leqslant 2 and \widetilde h for q>2.
(the case h(\alpha_1,\alpha_2)=r_2\alpha_2+1/q-1/p_2 > (1-\lambda)r_1\alpha_1+\lambda r_2\alpha_2 is possible only for r_2\alpha_2> r_1\alpha_1+1/p_2-1/p_1, which contradicts (1.10)). We have {\langle \overline{r}\rangle}/{2}\ne \lambda r_2, and so the function h attains its minimum either at
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Citation:
A. A. Vasil'eva, “Kolmogorov widths of a Sobolev class with constraints on derivatives in different metrics”, Sb. Math., 215:11 (2024), 1468–1498
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\paper Kolmogorov widths of a~Sobolev class with constraints on derivatives in different metrics
\jour Sb. Math.
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\issue 11
\pages 1468--1498
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