Abstract
This paper deals with the approximation of functions by the classical Bernstein polynomials in terms of the Ditzian–Totik modulus of smoothness. Asymptotic and non-asymptotic results are respectively stated for continuous and twice continuously differentiable functions. By using a probabilistic approach, known results are either completed or strengthened.
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1 Introduction and Statements of the Main Results
Let \({\mathbb {N}}\) be the set of positive integers and \({\mathbb {N}}_0={\mathbb {N}}\cup \{0\}\). As usual, C[0, 1] denotes the space of all real continuous functions defined on [0, 1], and \(C^m[0,1]\), \(m\in {\mathbb {N}}_0\), denotes the subspace of all m-times continuously differentiable functions, with the obvious understanding that \(C^0[0,1]=C[0,1]\). For \(m\in {\mathbb {N}}\), we denote by \({\mathscr {C}}^m[0,1]\supset C^m[0,1]\) the set of functions \(f\in C^{m-1}[0,1]\) such that \(f^{(m-1)}\) is absolutely continuous, i. e.,
for some bounded measurable function g, which can be denoted by \(g=f^{(m)}\).
The indicator function of a set A is denoted by \(1_A\), and \({\mathbb {E}}\) stands for mathematical expectation.
Let \(f\in C[0,1]\). The sup-norm of f is simply denoted by \(\Vert f\Vert \), although, more generally, we use the notation \(\Vert f\Vert _A=\sup \{|f(x)|:x\in A\}\), \(A\subseteq [0,1]\).
The second order central difference of f is defined by
whenever \(x\pm h\in [0,1]\). The Ditzian–Totik modulus of smoothness of f with weight function \(\varphi (x)=\sqrt{x(1-x)}\) is defined by
The classical first order modulus of continuity is simply denoted by \(\omega (f;\delta )\).
In this paper, we will make use of the following important inequality proved by Bustamante [2]:
Finally, the nth Bernstein polynomial of f is defined as
We have the probabilistic representation
where \(S_n(x)\) is a random variable having the binomial law with parameters n and x, that is to say,
Throughout this paper, whenever we write f, n, x, and y, we are assuming that \(f\in C[0,1]\), \(n\in {\mathbb {N}}\), and \(x,y\in [0,1]\).
Following the works by Ditzian and Ivanov [4] and Totik [9], the rates of uniform convergence for the Bernstein polynomials are characterized by
for some absolute constants \(K_1\) and \(K_2\). Whereas no specific values for \(K_1\) have been provided yet, different authors completed statement (4) by showing specific values for the constant \(K_2\). In this regard, Adell and Sangüesa [1] gave \(K_2=4\), Gavrea et al. [5] and Bustamante [2] provided \(K_2=3\), and finally, Păltănea [7] proved the validity of \(K_2=2.5\), this being the best result up to date and up to our knowledge.
This notwithstanding, if additional smoothness conditions on f are added, then the second inequality in (4) may be valid for values of \(K_2\) smaller than 2.5. In this respect, Bustamante and Quesada [3] and Păltănea [8] obtained the following asymptotic result
provided that f is not an affine function.
The contribution of this paper is twofold. In first place, we strength statement (5) by giving a non-asymptotic version of it. In fact, we prove the following result.
Theorem 1
If \(f\in C^2[0,1]\), then
As a consequence, statement (5) holds true.
In second place, we complete statement (4) in the following asymptotic form.
Theorem 2
Let \((\tau _n)_{n\ge 1}\) be a sequence of positive real numbers such that
If \(f\in C[0,1]\) is not an affine function, then
Moreover, we have in (4),
This result is based upon Theorem 3 in Sect. 3, which gives estimates of the form
for some explicit constants \(K_2(n,x)\) depending on n and x.
The paper is organized as follows. The proof of Theorem 1 is given in Sect. 2. We show Theorem 2 in Sect. 3 with the aid of two kinds of auxiliary results. On the one hand, we define certain smooth approximants \(Q_h^af\) of the function \(f\in C[0,1]\), by antisymmetrizing in an appropriate way the classical Steklov means of f. On the other hand, we estimate the tail probabilities and the truncated variance of the random variable \(S_n(x)\) appearing in the probabilistic representation of \(B_nf\) given in (2).
2 Proof of Theorem 1
2.1 Preliminaries
The Taylor’s formula of order \(m\in {\mathbb {N}}\) for \(f\in {\mathscr {C}}^m[0,1]\), with remainder in integral form can be written as
where \(\beta _m\) is a random variable with the beta density \(\rho _m(\theta )=m(1-\theta )^{m-1}\), \(0\le \theta \le 1\).
Lemma 1
If \(f\in C^2[0,1]\) and \(\delta \ge 0\), then
Proof
Let \(h\ge 0\) with \(x\pm h\in [0,1]\). Using (9) with \(m=2\), we get
as well as
Adding these two identities, we obtain
Replacing in (10) h by \(h\varphi (x)\) and applying the reverse triangular inequality, we have
thus completing the proof. \(\square \)
Gonska et al. [6] showed that
2.2 Proof of Theorem 1
Statement (6) is an inmediate consequence of (11), Lemma 1 with \(\delta =1/\sqrt{n}\), and the reverse and direct triangular inequalities. On the other hand, we have from Lemma 1
since \(f\in C^2[0,1]\). Thus, statement (5) readily follows from (6), and completes the proof.
3 Proof of Theorem 2
3.1 Auxiliary Results
Let \(0<h\le 1/3\). We consider the Steklov means of f defined as
where
In probabilistic terms, the Steklov means of f can be written as follows. Let \(V_1\) and \(V_2\) be independent identically distributed random variables having the uniform distribution on \([-1,1]\) and set \(V=(V_1+V_2)/2\). Since \(\rho (v)\) is the probability density of V, we can write
Lemma 2
Let \(0<h\le 1/3\) and let \(P_hf(y)\) be as in (12). Then,
-
(a)
$$\begin{aligned} \left| P_hf(y)-f(y)\right| \le \frac{1}{2}\omega _2^{\varphi }\left( f;\frac{h}{\varphi (y)}\right) . \end{aligned}$$
-
(b)
$$\begin{aligned} \left| (P_hf)''(y)\right| \le \frac{1}{h^2}\omega _2^{\varphi }\left( f;\frac{h}{\varphi (y)}\right) . \end{aligned}$$
Proof
Since V takes values in \([-1,1]\) and is symmetric (i. e., V and \(-V\) have the same law), we see that
thus showing (a). On the other hand, it can be checked that
where \(f_{(2)}\) is a second antiderivative of f. This readily implies part (b) and completes the proof. \(\square \)
We will make use of the approximant \(P_hf\), whose domain is the interval \([h,1-h]\), to define a further one whose domain is the whole interval [0, 1], keeping at the same time analogous properties to those given in Lemma 2. To this end, we assume that
and take
It turns out that
Now, we define the approximant \(Q_h^af(y)\) by antisymmetrizing \(P_hf(y)\) around the axes \(y=ax\) and \(y=1-ax\) as follows
The fact that \(Q_h^af\) is well defined readily follows from (13) and (14). Also, note that \(Q_h^af\) is twice differentiable except at the points ax and \(1-ax\). In these two points, \(Q_h^af\) only has sided second derivatives. This implies that \(Q_h^af\in {\mathscr {C}}^2[0,1]\).
Lemma 3
Let \(R_a=[ax,1-ax]\). Under assumptions (13) and (14), we have
-
(a)
If \(y\in R_a\), then
$$\begin{aligned} \left| Q_h^af(y)-f(y)\right| \le \frac{1}{2}\omega _2^{\varphi }\left( f;\frac{1}{\sqrt{n}}\right) ,\quad \left| (Q_h^af)''(y)\right| \le \frac{1}{h^2}\omega _2^{\varphi }\left( f;\frac{1}{\sqrt{n}}\right) . \end{aligned}$$ -
(b)
If \(y\notin R_a\), then
$$\begin{aligned} \left| Q_h^af(y)-f(y)\right| \le \left( \frac{7}{2}+\frac{3\sqrt{anx}}{(1-a)^{3/2}}\right) \omega _2^{\varphi }\left( f;\frac{h}{\varphi (h)}\right) , \end{aligned}$$and
$$\begin{aligned} \left| (Q_h^af)''(y)\right| \le \frac{1}{h^2}\omega _2^{\varphi }\left( f;\frac{h}{\varphi (h)}\right) . \end{aligned}$$
Proof
(a) If \(y\in R_a\), then
Thus, the first inequality in part (a) follows from Lemma 2(a) and definition (16), whereas the second one follows from Lemma 2(b).
(b) Suppose that \(y\in [0,ax)\). By (16), we can write
Since \(h\le ax\le 2ax-y\le 1-h\), we see that
We therefore have from Lemma 2(a)
Applying (1) with \(\lambda =ax\varphi (h)/(h\varphi (ax))\) and \(\delta =h/\varphi (h)\), we obtain
as follows from (14) and some simple computations. Hence, the first inequality follows from (20) and (21).
On the other hand, we have from (16), (19), and Lemma 2(b)
If \(y\in (1-ax,1]\), the proof es similar. \(\square \)
The following estimates concerning the random variable \(S_n(x)/n\) will be needed.
Lemma 4
In the setting of Lemma 3, denote by \(r=1-a\). Then,
-
(a)
$$\begin{aligned} P\left( \frac{S_n(x)}{n}\notin R_a\right) \le e^{-nxr^2/2}+3e^{-nxr^2/(2e)}=:\epsilon _n(x). \end{aligned}$$
-
(b)
$$\begin{aligned}&\frac{1}{h^2}{\mathbb {E}}\left( \frac{S_n(x)}{n}-x\right) ^2 1_{\left\{ \frac{S_n(x)}{n}\notin R_a\right\} } \\&\quad \le \frac{nx}{a(1-ax)}\left( e^{-nxr^2/2}+6e^{-(n-2)xr^2/(2e)}\right) =:\delta _n(x). \end{aligned}$$
Proof
(a) As follows from (3), we have
Let \(\theta \ge 0\). By (22) and Chebyshev’s inequality, we have
where we have used the inequalities
Choosing \(\theta =r\) in (23) (the value minimizing the exponent), we get
On the other hand, we claim that
Indeed, let \(0\le \theta \le 1\). Using the inequalities
we have, as in the proof of (24),
since \(x\le 1/2\). Thus, claim (25) follows by choosing \(\theta =r/e\) in (26). Hence, part (a) follows from (24) and (25).
(b) From (24), we see that
On the other hand, since \(1-ax\ge 1/2\), we have
We therefore have
since \(n\ge 3\). Observe that
as follows from assumptions (13) and (14). By (25), the right-hand side in (28) can be bounded above by
This, together with (27) and (28), shows part (b) and completes the proof.
\(\square \)
We are in a position to give the following local estimate.
Theorem 3
In the setting of Lemma 4, we have
where
Proof
We use the notation \(Qf(y)=Q_h^af(y)\) and write
By Lemma 3(a), we have
By (2) and Lemma 3(a) and (b), we see that
Finally, denote by \(\xi _n(x)=x+(S_n(x)/n-x)\beta _2\). Applying (9) with \(m=2\) and Lemma 3, we get
where we have used (14), the inequality \(1/\sqrt{n}\le h/\varphi (h)\), and the well known fact that
The result follows from (30)–(33) and Lemma 4. \(\square \)
3.2 Proof of Theorem 2
Since the random variables \(S_n(x)\) and \(n-S_n(1-x)\) have the same law, we have
On the other hand, if \(g(y)=f(1-y)\), we obviously have
Thus, without loss of generality, we can assume that \(0<x\le 1/2\).
In the setting of Lemma 4, we claim that
Actually, choose \(\lambda =h\sqrt{n}/\varphi (h)\) and \(\delta =1/\sqrt{n}\). By definition (14) and the fact that \(h\le ax\), we see that
This, in conjunction with (1), shows claim (34).
From Theorem 3 and (34), we have
where \(\nu _n(x)\) is defined in (29). Recalling the definitions of \(\epsilon _n(x)\) and \(\delta _n(x)\) given in Lemma 4, we see that
where \(P_3(\cdot )\) is a polynomial of degree three and c is a positive constant not depending on n and x. Observe that, whenever \(t_n\rightarrow \infty \), as \(n\rightarrow \infty \), we have
Let \(\tau _n\) be as in Theorem 2. From (35) and (36), we get
By (37) and the fact that \(\tau _n\rightarrow \infty \), as \(n\rightarrow \infty \), this implies that
which shows (7), since \(0<a<1\) is arbitrary.
On the other hand, let \(x\in (0,1/n)\). Consider the function
Observe that \(\omega _2^{\varphi }(f_x;1/\sqrt{n})=1\), as well as
thus implying that \(K_2\ge (1-x)^n\). Therefore, letting \(x\rightarrow 0\), we see that \(K_2\ge 1\). This shows (8) and completes the proof.
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The authors would like to thank an anonymous referee for her/his careful reading of the manuscript and valuable suggestions that led to a corrected and improved final version.
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This work is partially supported by Research Project PGC2018-097621-B-I00. The second author is also supported by Junta de Andalucía Research Group FQM-0178.
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Adell, J.A., Cárdenas-Morales, D. Asymptotic and Non-asymptotic Results in the Approximation by Bernstein Polynomials. Results Math 77, 166 (2022). https://doi.org/10.1007/s00025-022-01680-x
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DOI: https://doi.org/10.1007/s00025-022-01680-x