Home (λ, ψ)-Bernstein-Kantorovich operators
Article Open Access

(λ, ψ)-Bernstein-Kantorovich operators

  • Hüseyin Aktuğlu EMAIL logo , Mustafa Kara , Erdem Baytunç and Saner Fidan
Published/Copyright: June 6, 2025
Become an author with De Gruyter Brill

Abstract

In this article, we introduce a new family of ( λ , ψ ) -Bernstein-Kantorovich operators which depends on a parameter λ , derived from the basis functions of Bézier curves and an integrable function ψ . In this approach, all moments and central moments of the new operators can be obtained in terms of two numbers M 1 , ψ and M 2 , ψ , which are the integrals of ψ and ψ 2 , respectively. For operators L n ( f ; x ) with L n ( 1 ; x ) = 1 , the order of approximation to a function f by L n ( f ; x ) is more controlled by the term L n ( ( t x ) 2 ; x ) . For our operators K n , λ , ψ ( f ; x ) , the second central moment K n , λ , ψ ( ( t x ) 2 ; x ) depend on M 1 , ψ and M 2 , ψ . This means that in our new approach, it is possible to search for a function ψ with different values of M 1 , ψ and M 2 , ψ to make K n , λ , ψ ( ( t x ) 2 ; x ) smaller. Using this new approach, we show that there exists a function ψ such that the order of approximation to a function f by our new ( λ , ψ ) -Bernstein-Kantorovich operators is better than the classical λ -Bernstein-Kantorovich operators on the interval [0, 1]. Moreover, we obtain some direct and local approximation properties of new operators. We also show that our operators preserve monotonicity properties. Furthermore, we illustrate the approximation results of our operators graphically and numerically.

MSC 2010: 41A10; 41A25; 41A36; 41A60

1 Introduction

In 1912, Bernstein introduced the Bernstein polynomials [1] to prove the Weierstrass approximation theorem [2]. Bernstein polynomials have many noteworthy approximation properties, which have led to intensive research. The Bernstein operators are defined as

(1) B n ( f ; x ) = k = 0 n b n , k ( x ) f k n ,

where

(2) b n , k ( x ) = n k x k ( 1 x ) n k , x [ 0 , 1 ] .

The classical Bernstein operators are a widely used tool for approximating functions in the bounded function space on the interval [0, 1] (see [1,38]).

In 2010, Ye et al. [9] introduced and studied a new sort of basis functions of the Bézier curve in terms of shape parameter λ [ 1, 1 ] . Based on this, Cai et al. [10] introduced and considered a new generalization of Bernstein polynomials depending on the parameter λ as follows:

(3) B n , λ ( f ; x ) = k = 0 n b ˜ n , k ( λ ; x ) f k n ,

where λ [ 1, 1 ] and b ˜ n , k ( λ ; x ) , k = 0, 1 , , n , are defined as

(4) b ˜ n , k ( λ ; x ) = b n , 0 ( x ) λ n + 1 b n + 1,1 ( x ) , if k = 0 , b n , k ( x ) + λ n 2 k + 1 n 2 1 b n + 1 , k ( x ) λ n 2 k 1 n 2 1 b n + 1 , k + 1 ( x ) , if ( 1 k n 1 ) , b n , n ( x ) λ n + 1 b n + 1 , n ( x ) , if k = n .

Cai et al. [10] have extensively investigated various approximation properties of λ -Bernstein operators (3) such as uniform convergence and rate of convergence in terms of modulus of continuity and shape-preserving properties. For more details and recent published about these operators, we refer [1115]. Bernstein operators have limitations when approximating functions have singularities or discontinuities. To address this limitation, Kantorovich introduced the Bernstein-Kantorovich operators for the Lebesgue integrable function space, accommodating functions that may have singularities or discontinuities [6]:

K n ( f ; x ) = ( n + 1 ) k = 0 n b n , k ( x ) k n + 1 k + 1 n + 1 f ( t ) d t ,

or equivalently,

(5) K n ( f ; x ) = k = 0 n b n , k ( x ) 0 1 f k + t n + 1 d t ,

for all x [ 0, 1 ] and n N .

Later, in [16] the following modification of Bernstein-Kantorovich operators was considered and studied,

(6) K n , α ( f ; x ) = k = 0 n b n , k ( x ) 0 1 f k + t α n + 1 d t ,

for all x [ 0, 1 ] , α > 0 and n N .

In recent years, the Bernstein-Kantorovich operators and their modifications have also been used by reasearchers in many research studies (see [6,7,1623]). Two studies, in particular, have caught our attention. These are, respectively, [18] and [19] as follows:

Acu et al. [18] defined the Kantorovich modification of the λ -Bernstein operator (4) as follows:

(7) K n , λ ( f ; x ) = ( n + 1 ) k = 0 n b ˜ n , k ( λ ; x ) k n + 1 k + 1 n + 1 f ( t ) d t ,

where b ˜ n , k ( λ ; x ) are defined in equation (4).

Aktuğlu et al. [19] have introduced a new generalization of the Bernstein-Kantorovich operators as

(8) K n , ψ ( f ; x ) = k = 0 n b n , k ( x ) 0 1 f k + ψ ( t ) n + 1 d t ,

where b n , k ( x ) are defined in equation (2) and ψ is a function satisfying conditions given in (10). By choosing an appropriate function ψ , the order of approximation of the operators K n , ψ ( f ; x ) to a function f is at least as good as the classical Bernstein-Kantorovich operators K n ( f ; x ) on the interval [0, 1] [19].

In this study, inspired by operators (7) and (8), we introduce the ( λ , ψ ) -Bernstein-Kantorovich operators as follows:

(9) K n , λ , ψ ( f ; x ) = k = 0 n b ˜ n , k ( λ ; x ) 0 1 f k + ψ ( t ) n + 1 d t ,

for all x [0, 1], where b ˜ n , k ( λ ; x ) is defined in (4). The function ψ is any integrable function on [0, 1] such that

(10) 0 ψ ( t ) 1 , ψ ( 0 ) = 0 , ψ ( 1 ) = 1 , and M p , ψ 0 1 ψ p ( t ) d t ,

exist, where p is any non-negative integer. Obviously, 0 M p , ψ 1 for all p .

Remark 1

The operators K n , λ , ψ ( f ; x ) have the following special cases:

  1. If ψ ( t ) = t , then K n , λ , ψ ( f ; x ) = K n , λ ( f ; x ) .

  2. If λ = 0 , then K n , λ , ψ ( f ; x ) = K n , ψ ( f ; x ) .

  3. If λ = 0 and ψ ( t ) = t , then K n , λ , ψ ( f ; x ) = K n ( f ; x ) .

  4. If ψ ( t ) = t α and λ = 0 , then K n , λ , ψ ( f ; x ) = K n , α ( f ; x ) , which is given in [16].

Throughout this article, we examine the approximation properties of K n , λ , ψ ( f ; x ) . Our aim is to demonstrate that, for certain functions ψ , the modified operator K n , λ , ψ ( f ; x ) yields improved approximation results compared to the operators defined in (6) and (7).

2 Basic results

In this section, we present some results and properties of the operator K n , λ , ψ ( f ; x ) , which will be utilized in the following sections. Thanks to the next lemma, we can find the moments of the operators K n , λ , ψ ( f ; x ) by utilizing the moments of the classical Bernstein operators B n , λ ( f ; x ) , as given in equation (3).

Lemma 1

For each ψ , given in (10), we have the following relation:

(11) K n , λ , ψ ( t m ; x ) = 1 ( n + 1 ) m i = 0 m m i n i M m i , ψ B n , λ ( t i ; x ) ,

where m N and B n , λ ( f ; x ) is given in (3).

Proof

For any m N ,

K n , λ , ψ ( t m ; x ) = k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 m d t = 1 ( n + 1 ) m k = 0 n b ˜ n , k ( λ ; x ) 0 1 ( k + ψ ( t ) ) m d t = 1 ( n + 1 ) m k = 0 n b ˜ n , k ( λ ; x ) i = 0 m m i k i M m i , ψ = 1 ( n + 1 ) m i = 0 m m i n i M m i , ψ k = 0 n b ˜ n , k ( λ ; x ) k i n i

= 1 ( n + 1 ) m i = 0 m m i n i M m i , ψ B n , λ ( t i ; x ) ,

where M m i , ψ is given in (10).□

Lemma 2

[10] For any n N , and λ [ 1, 1 ] , we have

  1. B n , λ ( 1 ; x ) = 1 ,

  2. B n , λ ( t ; x ) = x + λ 1 2 x + x n + 1 ( 1 x ) n + 1 n ( n 1 ) ,

  3. B n , λ ( t 2 ; x ) = x 2 + x ( 1 x ) n + λ 2 x 4 x 2 + 2 x n + 1 n ( n 1 ) + x n + 1 + ( 1 x ) n + 1 1 n 2 ( n 1 ) .

Using Lemma 2, we can state the following lemma.

Lemma 3

For any function ψ , given in (10), we have

  1. K n , λ , ψ ( 1 ; x ) = 1 .

  2. K n , λ , ψ ( t ; x ) = n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ .

  3. K n , λ , ψ ( t 2 ; x ) = n 2 x 2 ( n + 1 ) 2 + n x ( 1 x ) ( n + 1 ) 2 + λ n 2 ( n + 1 ) 2 2 x 4 x 2 + 2 x n + 1 n ( n 1 ) + x n + 1 + ( 1 x ) n + 1 1 n 2 ( n 1 ) + 2 n M 1 , ψ ( n + 1 ) 2 x + 1 2 x + x n + 1 ( 1 x ) n + 1 n ( n 1 ) λ + M 2 , ψ ( n + 1 ) 2 .

Corollary 1

We have the following special cases of the aforementioned lemma.

  1. For ψ ( t ) = t , K n , λ , ψ ( t i ; x ) = K n , λ ( t i ; x ) with M 1 , ψ = 1 2 and M 2 , ψ = 1 3 , for i = 0, 1, 2.

  2. For λ = 0 and ψ ( t ) = t , K n , λ , ψ ( t i ; x ) = K n ( t i ; x ) , with M 1 , ψ = 1 2 and M 2 , ψ = 1 3 for i = 0, 1, 2.

The following lemma establishes the relation between central moments of the operators K n , λ , ψ ( f , x ) and moments of B n , λ ( f ; x ) .

Lemma 4

For any ψ , given in (10), we have

K n , λ , ψ ( ( t x ) m ; x ) = r = 0 m m r ( 1 ) m r x m r ( n + 1 ) r i = 0 r r i n i M r i , ψ B n , λ ( t i ; x ) ,

where m N and B n , λ ( f ; x ) are defined in (3).

Proof

Using the linearity property of K n , λ , ψ , we can write

K n , λ , ψ ( ( t x ) m ; x ) = K n , ψ , λ r = 0 m m r t r ( x ) m r ; x = r = 0 m m r ( x ) m r K n , λ , ψ ( t r ; x ) = r = 0 m m r ( 1 ) m r x m r K n , λ , ψ ( t r ; x ) .

From Lemma 1, we obtain

K n , λ , ψ ( ( t x ) m ; x ) = r = 0 m m r ( 1 ) m r x m r ( n + 1 ) r i = 0 r r i n i M r i , ψ B n , λ ( t i ; x ) ,

which completes the proof.□

From Lemma 4, we obtain the following lemma.

Lemma 5

For any ψ , given in (10), we have

( i ) K n , λ , ψ ( t x ; x ) = x n + 1 + M 1 , ψ n + 1 + λ 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 . ( i i ) K n , λ , ψ ( ( t x ) 2 ; x ) = n 2 x 2 ( n + 1 ) 2 + n x ( 1 x ) ( n + 1 ) 2 + λ n 2 ( n + 1 ) 2 2 x 4 x 2 + 2 x n + 1 n ( n 1 ) + x n + 1 + ( 1 x ) n + 1 1 n 2 ( n 1 ) + 2 n x M 1 , ψ ( n + 1 ) 2 + 2 n M 1 , ψ ( n + 1 ) 2 1 2 x + x n + 1 ( 1 x ) n + 1 n ( n 1 ) λ + M 2 , ψ ( n + 1 ) 2 2 x n x n + 1 + λ 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 + M 1 , ψ n + 1 + x 2 .

Also, using Remark 1, the following central moments for K n , λ ( f ; x ) and K n ( f ; x ) can be obtained from Lemma 5.

Corollary 2

Taking M 1 , ψ = 1 2 and M 2 , ψ = 1 3 in Lemma 4 [6], we obtain

  1. K n , λ ( t x ; x ) = 1 2 x 2 ( n + 1 ) + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ .

  2. K n , λ ( ( t x ) 2 ; x ) = 3 x ( 1 x ) ( n 1 ) + 1 3 ( n + 1 ) 2 + 2 x λ ( 1 x ) ( n 1 ) ( n + 1 ) 2 ( [ ( 1 x ) n + x n ] ( n + 1 ) 2 ) .

Corollary 3

Taking λ = 0 , M 1 , ψ = 1 2 , and M 2 , ψ = 1 3 in Lemma 5 [6], we obtain

  1. K n ( t x ; x ) = x n + 1 + 1 2 ( n + 1 ) ,

  2. K n ( ( t x ) 2 ; x ) = x 2 ( n + 1 ) 2 + n x ( 1 x ) ( n + 1 ) 2 x ( n + 1 ) 2 + 1 3 ( n + 1 ) 2 .

3 Direct and local approximation properties

In this section, we give direct and local approximation properties of the operators K n , λ , ψ ( f , x ) . First, we can state the following Bohman-Korovkin-type theorem [24] and [25].

Theorem 1

For any ψ , given in (10) and f C [0, 1], K n , λ , ψ ( f ; x ) converge uniformly to f on [0, 1], i.e.,

lim n K n , λ , ψ ( f ) f C [ 0,1 ] = 0 .

Proof

Let f C [0, 1]. Since M 1 , ψ and M 2 , ψ are the positive real numbers, we obtain from Lemma 3 that

lim n K n , λ , ψ ( 1 ; x ) = 1 ,

lim n K n , λ , ψ ( t ; x ) = x ,

and

lim n K n , λ , ψ ( t 2 ; x ) = x 2 .

Hence, by the Korovkin theorem, we obtain

lim n K n , λ , ψ ( f ) f C [ 0,1 ] = 0 .

Since the operator K n , ψ satisfies the property K n , ψ ( 1 ; x ) = 1 , it also satisfies the following inequality:

(12) K n , λ , ψ ( f ; x ) f ( x ) ε + 2 f C [ 0,1 ] δ 2 K n , λ , ψ ( ( t x ) 2 ; x ) ,

where δ is determined by the uniform continuity of the function f that is being approximated, i.e., inequality (12) demonstrates that the order of approximation to a function f by K n , λ , ψ ( f ; x ) is more influenced by the term K n , λ , ψ ( ( t x ) 2 ; x ) . Therefore, we can evaluate which of the operators K n , λ , ψ ( f ; x ) and K n , λ ( f ; x ) approximate the function f better, by examining their second central moments. In view of the aforementioned information, the following inequality can be used to compare the order of the approximation to a function f by operators K n , λ , ψ ( f ; x ) and K n , λ ( f ; x ) :

(13) K n , λ , ψ ( ( t x ) 2 ; x ) < K n , λ ( ( t x ) 2 ; x ) .

Since the terms K n , λ , ψ ( ( t x ) 2 ; x ) depend on the parameters M 1 , ψ and M 2 , ψ , different values of K n , λ , ψ ( ( t x ) 2 ; x ) are obtained for different functions ψ given in (10). This allows for the exploration of various values of M 1 , ψ and M 2 , ψ to achieve a better approximation. Therefore, to obtain a better approximation, we need to solve the following two problems.

  1. Under which conditions on λ , M 1 , ψ , and M 2 , ψ , inequality (13) holds?

  2. Is there any function ψ that gives these M 1 , ψ and M 2 , ψ values?

This study demonstrates that solutions exist for both problems.

Now, using Lemma 5 and Corollary 2, inequality (13) holds for n > 1 , if

(14) ( 1 2 M 1 , ψ ) x + M 2 , ψ 1 3 + λ ( 1 2 M 1 , ψ ) ( x n + 1 + ( 1 x ) n + 1 + 2 x 1 ) < 0 .

Lemma 6

For all x [ 0, 1 ] ,

(15) 1 x n + 1 + ( 1 x ) n + 1 + 2 x 1 1 .

Theorem 2

Let ψ be a function satisfying (10), the approximation order of f by K n , λ , ψ ( f ; x ) is at least as good as the approximation order of f by K n , λ ( f ; x ) for the following cases:

  1. For all x satisfying,

    x < 1 3 M 2 , ψ ( 1 2 M 1 , ψ ) λ ,

    when λ > 0 and 1 2 M 1 , ψ > 0 .

  2. For all x satisfying,

    x > 1 3 M 2 , ψ ( 1 2 M 1 , ψ ) λ ,

    when λ < 0 and 1 2 M 1 , ψ < 0 .

  3. For all x satisfying,

    x > 1 3 M 2 , ψ ( 1 2 M 1 , ψ ) + λ ,

    when λ > 0 and 1 2 M 1 , ψ < 0 .

  4. For all x satisfying,

    x < 1 3 M 2 , ψ ( 1 2 M 1 , ψ ) + λ ,

    when λ < 0 and 1 2 M 1 , ψ > 0 .

Proof

Each item can be proved by using (14) and the following inequalities:

  1. If λ ( 1 2 M 1 , ψ ) > 0 , then from (15), we have

    λ ( 1 2 M 1 , ψ ) ( x n + 1 + ( 1 x ) n + 1 + 2 x 1 ) λ ( 1 2 M 1 , ψ ) .

  2. If λ ( 1 2 M 1 , ψ ) < 0 , then

    λ ( 1 2 M 1 , ψ ) ( x n + 1 + ( 1 x ) n + 1 + 2 x 1 ) λ ( 1 2 M 1 , ψ ) .

In Theorem 2, the solutions of the first problem were obtained. Now we will move on to the second problem which is, “is there at least one function ψ α with values of M 1 , ψ α and M 2 , ψ α and λ satisfying each item of Theorem 2.”

Now, consider the the following functions:

(16) ψ α * ( t ) a α 1 α t 1 α , 0 t a t α , a t 1 ,

where a [ 0, 1 ] and α > 0 . Obviously, ψ α * ( t ) is continuous for all a [ 0, 1 ] , α > 0 , and satisfies (10), with

M 1 , ψ α * = α 1 α + 1 a α + 1 + 1 α + 1 and M 2 , ψ α * = 2 ( α 1 ) ( α + 1 ) ( α + 2 ) ( 2 α + 1 ) a 2 α + 1 + 1 2 α + 1 .

Remark 2

Using the function ψ α * given in (16) and Theorem 2, we have the following cases, where K n , λ , ψ α * ( f ; x ) has better error estimation than λ -Bernstein-Kantorovich operators K n , λ ( f ; x ) :

  1. For λ = 0.1 , α = 1.1 and a = 0.65 , M 1 , ψ α * = 0.4955 , M 2 , ψ α * = 0.3232 , and 1 2 M 1 , ψ α * = 0.0091 therefore from Theorem 2, i) the order of approximation to f by K n , λ , ψ α * ( f : x ) is as good as K n , λ ( f ; x ) on the interval:

    x < 1 3 M 2 , ψ α * 1 2 M 1 , ψ α * λ = 1.0199 ,

    which includes [0, 1].

  2. For λ = 0.8 , α = 1.1 and a = 0.75 , M 1 , ψ α * = 0.5022 , M 2 , ψ α * = 0.3294 , and 1 2 M 1 , ψ α * = 0.0044 , therefore from Theorem 2, ii) the order of approximation to f by K n , λ , ψ α * ( f : x ) is as good as K n , λ ( f ; x ) on the interval:

    x > 1 3 M 2 , ψ α * 1 2 M 1 , ψ α * λ = 0.0956 ,

    which includes [0, 1].

  3. For λ = 0.8 , α = 1.1 , and a = 0.75 , M 1 , ψ α * = 0.5022 , M 2 , ψ α * = 0.3294 , and 1 2 M 1 , ψ α * = 0.0044 , therefore from Theorem 2, ii) the order of approximation to f by K n , λ , ψ α * ( f : x ) is as good as K n , λ ( f ; x ) on the interval:

    x > 1 3 M 2 , ψ α * 1 2 M 1 , ψ α * + λ = 0.0956 ,

    which includes [0, 1].

  4. For λ = 0.1 , α = 1.1 , and a = 0.65 , M 1 , ψ α * = 0.4955 , M 2 , ψ α * = 0.3232 , and 1 2 M 1 , ψ α * = 0.0091 , therefore from Theorem 2, (ii) the order of approximation to f by K n , λ , ψ α * ( f : x ) is as good as K n , λ ( f ; x ) on the interval:

    x < 1 3 M 2 , ψ α * 1 2 M 1 , ψ α * + λ = 1.0199 ,

    which includes [0, 1].

x K 10,0.1 , ψ α * ( ( t x ) 2 ; x ) K 10,0.1 ( ( t x ) 2 ; x )
0 0.002671 0.002755
0.1 0.009402 0.009479
0.2 0.014562 0.014632
0.3 0.018248 0.018310
0.4 0.020467 0.020521
0.5 0.021213 0.021259
0.6 0.020482 0.020521
0.7 0.018278 0.018310
0.8 0.014608 0.014632
0.9 0.009463 0.009479
1 0.002746 0.002755

Recall that the first-order modulus of continuity,

w ( f ; δ ) = sup t 1 , t 2 [ 0,1 ] sup t 1 t 2 δ f ( t 1 ) f ( t 2 ) ,

where f C [0, 1], has the following properties [26,27]:

  1. f ( t 1 ) f ( t 2 ) ω ( f ; t 1 t 2 ) ,

  2. ω ( f ; λ δ ) ( 1 + λ ) ω ( f ; δ ) , where λ > 0 .

Theorem 3

If f C [0, 1], for any ψ , given in (10), then we have

K n , ψ , λ ( f ; x ) f ( x ) 2 ω ( f , K n , λ , ψ ( ( t x ) 2 ; x ) ) ,

where x [ 0,1 ] and n N .

Proof

Since K n , λ , ψ ( 1 ; x ) = 1 and b ˜ n , k ( λ ; x ) 0 on [0, 1], we can write

(17) K n , ψ , λ ( f ; x ) f ( x ) k = 0 n b ˜ n , k ( λ ; x ) 0 1 f k + ψ ( t ) n + 1 f ( x ) d t .

Additionally, by applying the properties of the modulus of continuity, we obtain

(18) f k + ψ ( t ) n + 1 f ( x ) ω f ; 1 δ k + ψ ( t ) n + 1 x δ 1 + 1 δ k + ψ ( t ) n + 1 x ω ( f ; δ ) .

By using (18) into (17), we obtain

(19) K n , λ , ψ ( f ; x ) f ( x ) k = 0 n b ˜ n , k ( x ) 0 1 1 + 1 δ k + ψ n + 1 x ω ( f ; δ ) d t = 1 + 1 δ k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x d t ω ( f ; δ ) .

Using the Cauchy-Schwartz inequality, we can state the following inequality:

(20) k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x d t k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x 2 d t 1 2 = K n , λ , ψ ( ( t x ) 2 ; x ) .

Combining (19) and (20), we obtain the following inequality:

K n , λ , ψ ( f ; x ) f ( x ) 1 + K n , λ , ψ ( ( t x ) 2 ; x ) δ ω ( f ; δ ) .

Hence, Theorem 3 can be obtained by choosing δ = K n , λ , ψ ( ( t x ) 2 ; x ) .□

Let W 2 [ 0, 1 ] = { g C [ 0, 1 ] : g , g C [ 0, 1 ] } . For δ > 0 and f C [0, 1], the Peetre’s K -functional is defined by

K 2 ( f ; δ ) inf g W 2 [ 0,1 ] { f g C [ 0,1 ] + δ g C [ 0,1 ] } .

Moreover, there exists R > 0 [4] such that

K 2 ( f ; δ ) R ω 2 ( f ; δ ) ,

where ω 2 ( f ; δ ) is called the second-order modulus of continuity of f C [0, 1], i.e.,

ω 2 ( f ; δ ) = sup 0 < h δ sup x , x + h , x + 2 h [ 0,1 ] f ( x + 2 h ) 2 f ( x + h ) + f ( x ) .

To prove the local approximation properties of the operators K n , λ , ψ based on the second-order modulus of continuity, we need to state the following lemma.

Lemma 7

For any f C [0, 1] and ψ , given in (10), we have

(21) K n , λ , ψ ( f ; x ) f C [ 0,1 ] ,

where . C [ 0,1 ] is the uniform norm of C [0, 1].

Theorem 4

Let f C [0, 1], and ψ be a function satisfying (10), then there exists R R + such that

K n , λ , ψ ( f ; x ) f ( x ) R ω 2 f ; 1 2 K n , λ , ψ ( ( t x ) 2 ; x ) + ( K n , λ , ψ ( ( t x ) ; x ) ) 2 + ω ( f ; K n , λ , ψ ( ( t x ) ; x ) ) .

Proof

First, we define the auxiliary operator as

(22) K n , λ , ψ * ( f ; x ) K n , λ , ψ ( f ; x ) + f ( x ) f n x n + 1 + M 1 , ψ n + 1 + [ 1 2 x + x n + 1 ( 1 x ) n + 1 ] n 2 1 λ .

From Lemma 3, we have

K n , λ , ψ * ( 1 ; x ) = 1

and

(23) K n , λ , ψ * ( t x ; x ) = 0 ,

where x [ 0, 1 ] and n N .

Let g W 2 [0, 1], by Taylor’s expansion,

(24) g ( t ) = g ( x ) + ( t x ) g ( x ) + x t ( t u ) g ( u ) d u ,

and (23), we have

K n , λ , ψ * ( g ; x ) = g ( x ) + K n , λ , ψ * x t ( t u ) g ( u ) d u ; x = g ( x ) + K n , λ , ψ x t ( t u ) g ( u ) d u ; x x n x n + 1 + M 1 , ψ n + 1 + [ 1 2 x + x n + 1 ( 1 x ) n + 1 ] n 2 1 λ n x n + 1 + M 1 , ψ n + 1 + [ 1 2 x + x n + 1 ( 1 x ) n + 1 ] n 2 1 λ u g ( u ) d u .

Therefore,

(25) K n , ψ α , λ * ( g ; x ) g ( x ) = K n , ψ α , λ x t ( t u ) g ( u ) d u ; x x n x n + 1 + M 1 , ψ n + 1 + [ 1 2 x + x n + 1 ( 1 x ) n + 1 ] n 2 1 λ n x n + 1 + M 1 , ψ α n + 1 + [ 1 2 x + x n + 1 ( 1 x ) n + 1 ] n 2 1 λ u g ( u ) d u .

By applying the absolute value to both sides of (25) and using the triangle inequality, we obtain

(26) K n , λ , ψ * ( g ; x ) g ( x ) K n , λ , ψ x t ( t u ) g ( u ) d u ; x + x n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ u g ( u ) d u K n , λ , ψ x t ( t u ) g ( u ) d u ; x + x n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ u g ( u ) d u K n , λ , ψ x t ( t u ) d u ; x g + x n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ u d u g C [ 0,1 ] K n , λ , ψ ( ( t x ) 2 ; x ) g C [ 0,1 ] + n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ x 2 g C [ 0,1 ] [ K n , λ , ψ ( ( t x ) 2 ; x ) + ( K n , λ , ψ ( ( t x ) ; x ) ) 2 ] g C [ 0,1 ] .

So,

K n , λ , ψ * ( g ; x ) g ( x ) [ K n , λ , ψ ( ( t x ) 2 ; x ) + ( K n , λ , ψ ( ( t x ) ; x ) ) 2 ] g C [ 0,1 ] .

Combining (21) and (22), we obtain

(27) K n , λ , ψ * ( f ; x ) K n , λ , ψ ( f ; x ) + f ( x ) + f n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ f C [ 0,1 ] K n , λ , ψ ( 1 ; x ) + 2 f C [ 0,1 ] 3 f C [ 0,1 ] ,

for all f C [0, 1] and x [ 0, 1 ] .

Equations (26) and (27) imply

K n , λ , ψ ( f ; x ) f ( x ) = K n , λ , ψ * ( f ; x ) f ( x ) + f n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ f ( x ) = K n , λ , ψ * ( f ; x ) K n , λ , ψ * ( g ; x ) + K n , λ , ψ * ( g ; x ) g ( x ) + g ( x ) f ( x ) + f n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ f ( x ) K n , λ , ψ * ( f ; x ) K n , λ , ψ * ( g ; x ) + K n , λ , ψ * ( g ; x ) g ( x ) + g ( x ) f ( x ) + f n x n + 1 + M 1 , ψ n + 1 + 1 2 x + x n + 1 ( 1 x ) n + 1 n 2 1 λ f ( x ) 4 f g + [ K n , λ , ψ ( ( t x ) 2 ; x ) + ( K n , λ , ψ ( ( t x ) ; x ) ) 2 ] g C [ 0,1 ] + ω ( f ; K n , λ , ψ ( ( t x ) ; x ) ) .

Taking infimum on the right-hand side over all g W 2 [0, 1], we obtain

K n , λ , ψ ( f ; x ) f ( x ) 4 K 2 f ; K n , λ , ψ ( ( t x ) 2 ; x ) + ( K n , λ , ψ ( ( t x ) ; x ) ) 2 4 + ω ( f ; K n , λ , ψ ( ( t x ) ; x ) ) ,

which completes the proof.□

The following theorem examines the rate of convergence of the operators K n , λ , ψ ( f ; x ) in terms of the Lipschitz class functions. For R > 0 and 0 < μ 1 , the usual Lipschitz class is defined by

Lip R ( μ ) { f C [ 0, 1 ] : f ( x ) f ( t ) R x t μ } ,

where x , t [ 0, 1 ] .

Theorem 5

If f Lip R ( μ ) , for any ψ , given in (10), we have

K n , λ , ψ ( f ; x ) f ( x ) R ( K n , λ , ψ ( ( t x ) 2 ; x ) μ ) ,

where x [ 0, 1 ] , R > 0 , and 0 < μ 1 .

Proof

Using linearity and positivity properties of K n , λ , ψ ( f ; x ) , we obtain

K n , λ , ψ ( f ; x ) f ( x ) K n , λ , ψ ( f ( t ) f ( x ) ; x ) = k = 0 n b ˜ n , k ( λ ; x ) 0 1 f k + ψ ( t ) n + 1 f ( x ) d t R k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x μ d t .

Applying Hölder’s inequality with p = 2 μ and q = 2 2 μ ,

K n , λ , ψ ( f ; x ) f ( x ) R k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x 2 d t μ 2 = R [ K n , λ , ψ ( ( t x ) 2 ; x ) ] μ 2 ,

which gives the desired result.□

Now, we investigate the rate of convergence of the operators K n , ψ , λ ( f ; x ) for a function space C 1 [0, 1].

Theorem 6

For all f C 1 [0, 1] and ψ , given in (10), we have

K n , λ , ψ ( f ; x ) f ( x ) K n , λ , ψ ( t x ; x ) f ( x ) + 2 K n , λ , ψ ( ( t x ) 2 ; x ) × ω ( f ; K n , λ , ψ ( ( t x ) 2 ; x ) ) .

Proof

Let f C 1 [0, 1]. By the mean value theorem of differential calculus, we have

f k + ψ ( t ) n + 1 f ( x ) = k + ψ ( t ) n + 1 x f ( x ) + k + ψ ( t ) n + 1 x [ f ( c ) f ( x ) ] ,

where c x , k + ψ ( t ) n + 1 .

Multiplying both sides of the aforementioned equality by b ˜ n , k and summing from 0 to n , we obtain

k = 0 n b ˜ n , k ( λ ; x ) f k + ψ ( t ) n + 1 f ( x ) = k = 0 n b ˜ n , k ( λ ; x ) k + ψ ( t ) n + 1 x f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) k + ψ ( t ) n + 1 x ( f ( c ) f ( x ) ) .

Taking integral from 0 to 1, we obtain

k = 0 n b ˜ n , k ( λ ; x ) 0 1 f k + ψ ( t ) n + 1 f ( x ) d t = k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x f ( x ) d t + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x ( f ( c ) f ( x ) ) d t ,

i.e.,

K n , λ , ψ ( f ; x ) f ( x ) = K n , λ , ψ ( t x ; x ) f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x ( f ( c ) f ( x ) ) d t .

Thus,

(28) K n , ψ α , λ ( f ; x ) f ( x ) K n , ψ ( t x ; x ) f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x f ( c ) f ( x ) d t .

On the other hand, we have

(29) f ( c ) f ( x ) = 1 + 1 δ c x ω ( f ; δ ) 1 + 1 δ k + ψ ( t ) n + 1 x ω ( f ; δ ) ,

where δ is any positive number that does not depend on k .

Combining (28) and (29), we obtain

K n , λ , ψ ( f ; x ) f ( x ) K n , λ , ψ ( t x ; x ) f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x d t ω ( f ; δ ) + 1 δ k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x 2 d t ω ( f ; δ ) K n , λ , ψ ( t x ; x ) f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x d t ω ( f ; δ ) + 1 δ K n , λ , ψ ( ( t x ) 2 ; x ) ω ( f ; δ ) .

Using the Cauchy-Schwarz inequality, we obtain

K n , λ , ψ ( f ; x ) f ( x ) K n , λ , ψ ( t x ; x ) f ( x ) + k = 0 n b ˜ n , k ( λ ; x ) 0 1 k + ψ ( t ) n + 1 x 2 d t 1 2 ω ( f ; δ ) + 1 δ K n , λ , ψ ( ( t x ) 2 ; x ) ω ( f ; δ ) = K n , λ , ψ ( t x ; x ) f ( x ) + [ K n , λ , ψ ( ( t x ) 2 ; x ) ] 1 2 ω ( f ; δ ) + 1 δ K n , λ , ψ ( ( t x ) 2 ; x ) ω ( f ; δ ) = K n , λ , ψ ( t x ; x ) f ( x ) + 1 + [ K n , λ , ψ ( ( t x ) 2 ; x ) ] 1 2 δ [ K n , λ , ψ ( ( t x ) 2 ; x ) ] 1 2 ω ( f ; δ ) .

Choosing δ = K n , λ , ψ ( ( t x ) 2 ; x ) completes the proof.□

4 Monotonicity-preserving properties

This section is devoted to the shape-preserving properties of the operators K n , λ , ψ ( f ; x ) , which can be written in the following form [28]:

(30) K n , λ , ψ ( f ; x ) = B n , ψ ( f ; x ) + λ k = 1 n n 2 k + 1 n 2 1 b n + 1 , k ( x ) h k , ψ ( f ) λ k = 1 n n 2 k + 1 n 2 1 b n + 1 , k ( x ) h k 1 , ψ ( f ) ,

where

h k , ψ ( f ) = 0 1 f k + ψ ( t ) n + 1 d t

and

B n , ψ ( f ; x ) = k = 0 n b n , k ( x ) h k , ψ ( f ) .

Moreover, by applying derivative operators d d x and d 2 d x 2 to the operators (30), for each λ [ 1, 1 ] and f C [0, 1], we have the following equation:

(31) d d x K n , λ , ψ ( f ; x ) = k = 0 n 1 n k + λ n 2 k 1 n 1 b n , k ( x ) [ h k + 1 , ψ ( f ) h k , ψ ( f ) ] + k = 0 n 1 k + 1 λ n 2 k 1 n 1 b n , k + 1 ( x ) [ h k + 1 , ψ ( f ) h k , ψ ( f ) ] .

Theorem 7

For all n N and λ [ 1, 1 ] , then K n , λ , ψ ( f ; x ) preserves the monotonocity property. In other words, if f is increasing (decreasing) on the interval [0, 1], then K n , λ , ψ ( f ; x ) is increasing (decreasing) on [0, 1].

Proof

Let f be an increasing function on the interval [0, 1]. Then, obviously, h k + 1 , ψ ( f ) h k , ψ ( f ) 0 . On the other hand, using the following inequalities [28]:

(32) 0 n k 1 n k + λ 1 2 k n 1

and

(33) 0 ( k + 1 ) 1 ( k + 1 ) λ 1 2 k n 1 ,

we have d d x K n , λ , ψ ( f ; x ) 0 . The aforementioned proof can be easily modified for decreasing function.□

5 Graphical analysis and error estimation

In this section, we give some graphics to illustrate the approximation of K n , λ , ψ ( f ; x ) to certain function f in Figure 1 when f ( x ) = 2 x 3 9 4 x 2 + 13 6 x 3 32 for α = 1.1 , λ = 0.1 , and a = 0.65 . Similarly, shape-preserving properties of K n , λ , ψ ( f ; x ) are illustrated in Figures 2 and 3 for functions f ( x ) = x 3 + 3 x 2 + 9 and function f ( x ) = 2 x 2 4 x 3 , respectively, for α = 1.1 , λ = 0.1 , and a = 0.65 . For the following figures, ψ α * ( t ) is the function given in (16).

Figure 1 
               Approximation of 
                     
                        
                        
                           
                              
                                 K
                              
                              
                                 n
                                 ,
                                 λ
                                 ,
                                 
                                    
                                       ψ
                                    
                                    
                                       α
                                    
                                    
                                       *
                                    
                                 
                              
                           
                           
                              (
                              
                                 f
                                 ;
                                 
                                 x
                              
                              )
                           
                        
                        {K}_{n,\lambda ,{\psi }_{\alpha }^{* }}\left(f;\hspace{0.33em}x)
                     
                   to 
                     
                        
                        
                           f
                           
                              (
                              
                                 x
                              
                              )
                           
                           =
                           2
                           
                              
                                 x
                              
                              
                                 3
                              
                           
                           −
                           
                              
                                 9
                              
                              
                                 4
                              
                           
                           
                              
                                 x
                              
                              
                                 2
                              
                           
                           +
                           
                              
                                 13
                              
                              
                                 6
                              
                           
                           x
                           −
                           
                              
                                 3
                              
                              
                                 32
                              
                           
                        
                        f\left(x)=2{x}^{3}-\frac{9}{4}{x}^{2}+\frac{13}{6}x-\frac{3}{32}
                     
                   for 
                     
                        
                        
                           α
                           =
                           1.1
                        
                        \alpha =1.1
                     
                  , 
                     
                        
                        
                           λ
                           =
                           0.1
                        
                        \lambda =0.1
                     
                  , and 
                     
                        
                        
                           a
                           =
                           0.65
                        
                        a=0.65
                     
                  .
Figure 1

Approximation of K n , λ , ψ α * ( f ; x ) to f ( x ) = 2 x 3 9 4 x 2 + 13 6 x 3 32 for α = 1.1 , λ = 0.1 , and a = 0.65 .

Figure 2 
               
                  
                     
                        
                        
                           
                              
                                 K
                              
                              
                                 n
                                 ,
                                 λ
                                 ,
                                 
                                    
                                       ψ
                                    
                                    
                                       α
                                    
                                    
                                       *
                                    
                                 
                              
                           
                           
                              (
                              
                                 f
                                 ;
                                 
                                 x
                              
                              )
                           
                        
                        {K}_{n,\lambda ,{\psi }_{\alpha }^{* }}\left(f;\hspace{0.33em}x)
                     
                   is increasing for an increasing function 
                     
                        
                        
                           f
                           
                              (
                              
                                 x
                              
                              )
                           
                           =
                           −
                           
                              
                                 x
                              
                              
                                 3
                              
                           
                           +
                           3
                           
                              
                                 x
                              
                              
                                 2
                              
                           
                           +
                           9
                        
                        f\left(x)=-{x}^{3}+3{x}^{2}+9
                     
                  , 
                     
                        
                        
                           α
                           =
                           1.1
                           ,
                           λ
                           =
                           0.1
                        
                        \alpha =1.1,\lambda =0.1
                     
                  , and 
                     
                        
                        
                           a
                           =
                           0.65
                        
                        a=0.65
                     
                  .
Figure 2

K n , λ , ψ α * ( f ; x ) is increasing for an increasing function f ( x ) = x 3 + 3 x 2 + 9 , α = 1.1 , λ = 0.1 , and a = 0.65 .

Figure 3 
               
                  
                     
                        
                        
                           
                              
                                 K
                              
                              
                                 n
                                 ,
                                 λ
                                 ,
                                 
                                    
                                       ψ
                                    
                                    
                                       α
                                    
                                    
                                       *
                                    
                                 
                              
                           
                           
                              (
                              
                                 f
                                 ;
                                 
                                 x
                              
                              )
                           
                        
                        {K}_{n,\lambda ,{\psi }_{\alpha }^{* }}\left(f;\hspace{0.33em}x)
                     
                   is decreasing for a decreasing function 
                     
                        
                        
                           f
                           
                              (
                              
                                 x
                              
                              )
                           
                           =
                           2
                           
                              
                                 x
                              
                              
                                 2
                              
                           
                           −
                           4
                           x
                           −
                           3
                        
                        f\left(x)=2{x}^{2}-4x-3
                     
                  , 
                     
                        
                        
                           α
                           =
                           1.1
                           ,
                           λ
                           =
                           0.1
                        
                        \alpha =1.1,\lambda =0.1
                     
                  , and 
                     
                        
                        
                           a
                           =
                           0.65
                        
                        a=0.65
                     
                  .
Figure 3

K n , λ , ψ α * ( f ; x ) is decreasing for a decreasing function f ( x ) = 2 x 2 4 x 3 , α = 1.1 , λ = 0.1 , and a = 0.65 .

6 Conclusion

In this article, we introduce a family of λ -Bernstein-Kantorovich-type operators that depend on a function ψ , which satisfies specific conditions as given in Equation (10). We derive all moments and central moments of these new operators in terms of two variables, M 1 , ψ and M 2 , ψ , which represent the integrals of ψ and ψ 2 over [0, 1], respectively. Using this approach, and recognizing that the approximation order of a function f by L n ( f ; x ) is closely tied to the term L n ( ( t x ) 2 ; x ) , we address two main questions: are there values of M 1 , ψ and M 2 , ψ for which K n , λ , ψ ( ( t x ) 2 ; x ) < K n , λ ( ( t x ) 2 ; x ) , and is there a function ψ with these values of M 1 , ψ and M 2 , ψ ? We establish that both questions have affirmative answers (Figure 4). Additionally, we identify operators with superior approximation properties compared to the classical Bernstein-Kantorovich operators across [0, 1], as well as operators from [18] on [0, 1]. This article also provides results on the uniform convergence and rate of convergence of these new operators, characterized by the first- and second-order modulus of continuity, and demonstrates that the operators exhibit monotonicity-preserving property (Figures 2 and 3). Finally, numerical examples are presented to support our findings.

Figure 4 
               Graphical representations of 
                     
                        
                        
                           
                              
                                 K
                              
                              
                                 n
                                 ,
                                 λ
                                 ,
                                 
                                    
                                       ψ
                                    
                                    
                                       α
                                    
                                    
                                       *
                                    
                                 
                              
                           
                           
                              (
                              
                                 
                                    
                                       
                                          (
                                          
                                             t
                                             −
                                             x
                                          
                                          )
                                       
                                    
                                    
                                       2
                                    
                                 
                                 ;
                                 
                                 x
                              
                              )
                           
                        
                        {K}_{n,\lambda ,{\psi }_{\alpha }^{* }}\left({\left(t-x)}^{2};\hspace{0.33em}x)
                     
                   and 
                     
                        
                        
                           
                              
                                 K
                              
                              
                                 n
                                 ,
                                 λ
                              
                           
                           
                              (
                              
                                 
                                    
                                       
                                          (
                                          
                                             t
                                             −
                                             x
                                          
                                          )
                                       
                                    
                                    
                                       2
                                    
                                 
                                 ;
                                 
                                 x
                              
                              )
                           
                        
                        {K}_{n,\lambda }\left({\left(t-x)}^{2};\hspace{0.33em}x)
                     
                   for 
                     
                        
                        
                           α
                           =
                           1.1
                        
                        \alpha =1.1
                     
                  , 
                     
                        
                        
                           a
                           =
                           0.65
                        
                        a=0.65
                     
                  , 
                     
                        
                        
                           λ
                           =
                           0.1
                        
                        \lambda =0.1
                     
                  , and 
                     
                        
                        
                           n
                           =
                           10
                        
                        n=10
                     
                  .
Figure 4

Graphical representations of K n , λ , ψ α * ( ( t x ) 2 ; x ) and K n , λ ( ( t x ) 2 ; x ) for α = 1.1 , a = 0.65 , λ = 0.1 , and n = 10 .

Acknowledgements

The authors would like to thank the referee for his/her careful reading and valuable suggestions for improving this article.

  1. Funding information: The authors state no funding involved.

  2. Author contributions: All authors of the manuscript have made equal contributions.

  3. Conflict of interest: The authors have no conflict of interest.

  4. Ethical approval: The conducted research is not related to either human or animal use.

  5. Data availability statement: Data sharing is not applicable to this article as no datasets were generated or analyzed during this study.

References

[1] S. Bernstein, Démonstration du théorème de Weierstrass fondeé sur le calcul des probabilités, Commun. Kharkov Math. Soc. 13 (1912), 1–2. Search in Google Scholar

[2] V. K. Weierstrass, Uber die analytische Darstellbarkeit sogennanter willkürlicher Functionen einer reellen Veränderlichen, in: Sitzungsberichte der Akademie zu Berlin, 1885, pp. 633–639, and 789–805. Search in Google Scholar

[3] P. J. Davis, Interpolation and Approximation, Dover Publications, Inc., New York, NY, 1975. Search in Google Scholar

[4] R. A. Devore and G. G Lorentz, Constructive Approximation, Springer, Berlin, Germany, 1993. 10.1007/978-3-662-02888-9Search in Google Scholar

[5] M. Felten, Local and global approximation theorems for positive linear operators, J. Approx. Theory 94 (1998), no. 3, 396–419, https://doi.org/10.1006/jath.1998.3212. Search in Google Scholar

[6] L. V. Kantorovich, Sur certains développements suivant les polynômes de la forme de S. Bernstein, I, II, CR Acad. URSS 563 (1930), no. 568, 595–600. Search in Google Scholar

[7] A. Kumar, Approximation properties of generalized λ-Bernstein-Kantorovich type operators, Rend. Circ. Mat. Palermo two, 70 (2021), no. 1, 505–520, https://doi.org/10.1007/s12215-020-00509-2. Search in Google Scholar

[8] G. G. Lorentz, Bernstein Polynomials, Chelsea Publ. Co., New York, 1986. Search in Google Scholar

[9] Z. Ye, X. Long, and X. M. Zeng, Adjustment algorithms for Bézier curve and surface, In: International Conference on Computer Science and Education, 2010, pp. 1712–1716. 10.1109/ICCSE.2010.5593563Search in Google Scholar

[10] Q. B. Cai, B. Y. Lian, and G. Zhou, Approximation properties of λ-Bernstein operators, J. Inequal. Appl. 2018 (2018), 61, https://doi.org/10.1186/s13660-018-1653-7. Search in Google Scholar PubMed PubMed Central

[11] R. Aslan, Approximation properties of univariate and bivariate new class λ-Bernstein-Kantorovich operators and its associated GBS operators, Comput. Appl. Math. 42 (2023), 34, https://doi.org/10.1007/s40314-022-02182-w. Search in Google Scholar

[12] H. M. Srivastava, F. Özger, and S. A. Mohiuddine, Construction of Stancu-type Bernstein operators based on Bézier bases with shape parameter λ, Symmetry 11 (2019), no. 3, 316, https://doi.org/10.3390/sym11030316. Search in Google Scholar

[13] R. Aslan and M. Mursaleen, Some approximation results on a class of new type Bernstein polynomials, J. Math. Inequal. 16 (2022), no. 2, 445–462, https://doi.org/10.7153/jmi-2022-16-32. Search in Google Scholar

[14] Q. B. Cai, Approximation by a new kind of (λ,μ)-Bernstein-Kantorovich operators, J. Comput. Appl. Math. 43 (2024), no. 5, 283, https://doi.org/10.1007/s40314-024-02801-8. Search in Google Scholar

[15] S. Rahman, M. Mursaleen, and A. M. Acu, Approximation properties of λ-Bernstein-Kantorovich operators with shifted knots, Math. Methods Appl. Sci. 42 (2019), no. 11, 4042–4053, https://doi.org/10.1002/mma.5632. Search in Google Scholar

[16] M. A. Özarslan and O. Duman, Smoothness properties of modified Bernstein-Kantorovich operators, Numer. Funct. Anal. Optim. 37 (2016), no. 1, 92–105, https://doi.org/10.1080/01630563.2015.1079219. Search in Google Scholar

[17] T. Acar, S. Kursun, and M. Turgay, Multidimensional Kantorovich modifications of exponential sampling series, Quaest. Math. 46 (2023), no.1, 57–72, https://doi.org/10.2989/16073606.2021.1992033. Search in Google Scholar

[18] A. M. Acu, N. Manav, and D. F. Sofonea, Approximation properties of λ-Kantorovich operators, J. Inequal. Appl. 2018 (2018), 202, https://doi.org/10.1186/s13660-018-1795-7. Search in Google Scholar PubMed PubMed Central

[19] H. Aktuğlu, M. Kara, and E. Baytunç, ψ-Bernstein Kantorovich operators, Math. Methods Appl. Sci. 48 (2025), no. 1, 1124–1141, https://doi.org/10.1002/mma.10375. Search in Google Scholar

[20] F. Altomare and M. N. Cappelletti, On a generalization of Szasz–Mirakjan-Kantorovich operators, Results Math. 63 (2013), no. 3–4, 837–863, https://doi.org/10.1007/s00025-012-0236-z. Search in Google Scholar

[21] C. Bardaro, G. Vinti, P. L. Butzer, and R. L. Stens, Kantorovich type generalized sampling series in the setting of the Orlicz spaces, Sampl. Theory Signal Process. Data Anal. 6 (2007), no. 1, 29–52, https://doi.org/10.1007/BF03549462. Search in Google Scholar

[22] H. Gonska, M. Heilmann, and I. Rasa, Kantorovich operators of order k, Numer. Funct. Anal. Optim. 32 (2011), no. 7, 717–738, https://doi.org/10.1080/01630563.2011.580877. Search in Google Scholar

[23] S. Sucu and E. Ibikli, Approximation by means of Kantorovich Stancu type operators, Numer. Funct. Anal. Optim. 34 (2013), no. 5, 557–575, https://doi.org/10.1080/01630563.2012.716806. Search in Google Scholar

[24] Z. Finta, Note on a Korovkin type theorem, J. Math. Anal. Appl. 415 (2014), no. 2, 750–759, https://doi.org/10.1016/j.jmaa.2014.02.010. Search in Google Scholar

[25] P. P. Korovkin, Linear Operators and Approximation Theory, Hindustan Publishing Corporation, Delhi, 1960. Search in Google Scholar

[26] G. A. Anastassiou and S. G. Gal, Approximation Theory: Moduli of Continuity and Global Smoothness Preservation, Birkhäuser, Boston, Inc., Boston, MA., 2000. 10.1007/978-1-4612-1360-4_9Search in Google Scholar

[27] Z. Ditzian and V. Totik, Moduli of Smoothness, Springer, New York, 1987. 10.1007/978-1-4612-4778-4Search in Google Scholar

[28] L.-T. Su, G. Mutlu, and B. Çekim, On the shape-preserving properties of λ-Bernstein operators, J. Inequal. Appl. 2022 (2022), Art. No. 151, https://doi.org/10.1186/s13660-022-02890-1. Search in Google Scholar

Received: 2024-11-08
Revised: 2025-02-05
Accepted: 2025-02-28
Published Online: 2025-06-06

© 2025 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

Articles in the same Issue

  1. Research Articles
  2. On approximation by Stancu variant of Bernstein-Durrmeyer-type operators in movable compact disks
  3. Circular n,m-rung orthopair fuzzy sets and their applications in multicriteria decision-making
  4. Grand Triebel-Lizorkin-Morrey spaces
  5. Coefficient estimates and Fekete-Szegö problem for some classes of univalent functions generalized to a complex order
  6. Proofs of two conjectures involving sums of normalized Narayana numbers
  7. On the Laguerre polynomial approximation errors and lower type of entire functions of irregular growth
  8. New convolutions for the Hartley integral transform imbedded in the Banach algebras and convolution-type integral equations
  9. Some inequalities for rational function with prescribed poles and restricted zeros
  10. Lucas difference sequence spaces defined by Orlicz function in 2-normed spaces
  11. Evaluating the efficacy of fuzzy Bayesian networks for financial risk assessment
  12. Fixed point results for contractions of polynomial type
  13. Estimation for spatial semi-functional partial linear regression model with missing response at random
  14. Investigating the controllability of differential systems with nonlinear fractional delays, characterized by the order 0 < η ≤ 1 < ζ ≤ 2
  15. New forms of bilateral inequalities for K-g-frames
  16. Rate of pole detection using Padé approximants to polynomial expansions
  17. Existence results for nonhomogeneous Choquard equation involving p-biharmonic operator and critical growth
  18. Note on the shape-preservation of a new class of Kantorovich-type operators via divided differences
  19. Geršhgorin-type theorems for Z1-eigenvalues of tensors with applications
  20. New topologies derived from the old one via operators
  21. Blow up solutions for two-dimensional semilinear elliptic problem of Liouville type with nonlinear gradient terms
  22. Infinitely many normalized solutions for Schrödinger equations with local sublinear nonlinearity
  23. Nonparametric expectile shortfall regression for functional data
  24. Advancing analytical solutions: Novel wave insights and methodologies for beta fractional Kuralay-II equations
  25. A generalized p-Laplacian problem with parameters
  26. A study of solutions for several classes of systems of complex nonlinear partial differential difference equations in ℂ2
  27. Towards finding equalities involving mixed products of the Moore-Penrose and group inverses by matrix rank methodology
  28. ω -biprojective and ω ¯ -contractible Banach algebras
  29. Coefficient functionals for Sakaguchi-type-Starlike functions subordinated to the three-leaf function
  30. Solutions of several general quadratic partial differential-difference equations in ℂ2
  31. Inequalities for the generalized trigonometric functions with respect to weighted power mean
  32. Optimization of Lagrange problem with higher-order differential inclusion and special boundary-value conditions
  33. Hankel determinants for q-starlike functions connected with q-sine function
  34. System of partial differential hemivariational inequalities involving nonlocal boundary conditions
  35. A new family of multivalent functions defined by certain forms of the quantum integral operator
  36. A matrix approach to compare BLUEs under a linear regression model and its two competing restricted models with applications
  37. Weighted composition operators on bicomplex Lorentz spaces with their characterization and properties
  38. Behavior of spatial curves under different transformations in Euclidean 4-space
  39. Commutators for the maximal and sharp functions with weighted Lipschitz functions on weighted Morrey spaces
  40. A new kind of Durrmeyer-Stancu-type operators
  41. A study of generalized Mittag-Leffler-type function of arbitrary order
  42. On the approximation of Kantorovich-type Szàsz-Charlier operators
  43. Split quaternion Fourier transforms for two-dimensional real invariant field
  44. Review Article
  45. Characterization generalized derivations of tensor products of nonassociative algebras
  46. Special Issue on Differential Equations and Numerical Analysis - Part II
  47. Existence and optimal control of Hilfer fractional evolution equations
  48. Persistence of a unique periodic wave train in convecting shallow water fluid
  49. Existence results for critical growth Kohn-Laplace equations with jumping nonlinearities
  50. Monotonicity and oscillation for fractional differential equations with Riemann-Liouville derivatives
  51. Nontrivial solutions for a generalized poly-Laplacian system on finite graphs
  52. Stability and bifurcation analysis of a modified chemostat model
  53. Special Issue on Nonlinear Evolution Equations and Their Applications - Part II
  54. Analytic solutions of a generalized complex multi-dimensional system with fractional order
  55. Extraction of soliton solutions and Painlevé test for fractional Peyrard-Bishop DNA model
  56. Special Issue on Recent Developments in Fixed-Point Theory and Applications - Part II
  57. Some fixed point results with the vector degree of nondensifiability in generalized Banach spaces and application on coupled Caputo fractional delay differential equations
  58. On the sum form functional equation related to diversity index
  59. Special Issue on International E-Conference on Mathematical and Statistical Sciences - Part II
  60. Simpson, midpoint, and trapezoid-type inequalities for multiplicatively s-convex functions
  61. Converses of nabla Pachpatte-type dynamic inequalities on arbitrary time scales
  62. Special Issue on Blow-up Phenomena in Nonlinear Equations of Mathematical Physics - Part II
  63. Energy decay of a coupled system involving a biharmonic Schrödinger equation with an internal fractional damping
  64. Special Issue on Some Integral Inequalities, Integral Equations, and Applications - Part II
  65. Nonlinear heat equation with viscoelastic term: Global existence and blowup in finite time
  66. New Jensen's bounds for HA-convex mappings with applications to Shannon entropy
  67. Special Issue on Approximation Theory and Special Functions 2024 conference
  68. Ulam-type stability for Caputo-type fractional delay differential equations
  69. Faster approximation to multivariate functions by combined Bernstein-Taylor operators
  70. (λ, ψ)-Bernstein-Kantorovich operators
  71. Some special functions and cylindrical diffusion equation on α-time scale
  72. (q, p)-Mixing Bloch maps
  73. Orthogonalizing q-Bernoulli polynomials
  74. On better approximation order for the max-product Meyer-König and Zeller operator
  75. Moment-based approximation for a renewal reward process with generalized gamma-distributed interference of chance
  76. Special Issue on Variational Methods and Nonlinear PDEs
  77. A note on mean field type equations
  78. Ground states for fractional Kirchhoff double-phase problem with logarithmic nonlinearity
  79. Solution of nonlinear Langevin equations involving Hilfer-Hadamard fractional order derivatives and variable coefficients
Downloaded on 8.9.2025 from https://www.degruyterbrill.com/document/doi/10.1515/dema-2025-0126/html
Scroll to top button