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Some approximation results for generalized Kantorovich-type operators

Abstract

In this paper, we construct a new family of operators, prove some approximation results in A-statistical sense and establish some direct theorems for Kantorovich-type integral operators.

MSC: Primary 41A10, 41A25, 41A36.

1 Introduction and preliminaries

Statistical convergence [1] and its variants, extensions and generalizations have been proved to be an active area of recent research in summability theory, e.g., lacunary statistical convergence [2], λ-statistical convergence [3], A-statistical convergence [4], statistical A-summability [5], statistical summability (C,1) [6], statistical summability (H,1) [7], statistical summability ( N ¯ ,p) [8] and statistical σ-summability [9]etc. Following the work of Gadjiv and Orhan [10], these statistical summability methods have been used in establishing many approximation theorems (e.g., [5, 1120] and [21]). Recently, the statistical approximation properties have also been investigated for several operators. For instance, in [22] Butzer and Hahn operators; in [23] and [24]q-analogue of Stancu-Beta operators; in [25] Bleimann, Butzer and Hahn operators; in [26] Baskakov-Kantorovich operators; in [27] Szász-Mirakjan operators; in [28] analogues of Bernstein-Kantorovich operators; and in [29]q-Lagrange polynomials were defined and their statistical approximation properties were investigated. Most recently, the statistical summability of Walsh-Fourier series has been discussed in [30]. In this paper, we construct a new family of operators with the help of Erkuş-Srivastava polynomials, establish some A-statistical approximation properties and direct theorems.

Let us recall the following definitions.

Let denote the set of all natural numbers. Let KN and K n ={kn:kK}. Then the natural density of K is defined by δ(K)= lim n n 1 | K n | if the limit exists, where | K n | denotes the cardinality of the set K n . A sequence x=( x k ) of real numbers is said to be statistically convergent to L (cf. Fast [1]) provided that for every ϵ>0 the set {kN:| x k L|ϵ} has natural density zero, i.e., for each ϵ>0,

lim n 1 n | { k n : | x k L | ϵ } | =0.

In this case, we write st- lim k x k =L. Note that every convergent sequence is statistically convergent but not conversely.

Let A=( a n k ), n,k=1,2,3, , be an infinite matrix. For a given sequence x=( x k ), the A-transform of x is defined by Ax=( ( A x ) n ), where ( A x ) n = k = 1 a n k x k , provided the series converges for each n. We say that A is regular if lim n ( A x ) n =L=limx. Let A be a regular matrix.

We say that a sequence x=( x k ) is A-statistically convergent to a number L (cf. Kolk [4]) if for every ϵ>0,

lim n k : | x k L | ϵ a n k =0.

In this case, we denote this limit by st A - lim n x n =L.

Note that for A= C 1 :=( c j n ), the Cesàro matrix of order 1, A-statistical convergence reduces to the statistical convergence.

2 Construction of a new operator and its properties

The well-known (two-variable) polynomials g n ( α , β ) (x,y), which are generated by

( 1 x z ) α ( 1 y z ) β = n = 0 g n ( α , β ) (x,y) z n ( | z | < min { | x | 1 , | y | 1 } ) ,
(2.1)

are the Lagrange polynomials which occur in certain problems in statistics [31]. Recently, Chan [32] introduced and systematically investigated the multivariable extension of the classical Lagrange polynomials g n ( α , β ) (x,y). These multivariable Lagrange polynomials, which are popularly known in the literature as the Chan-Chyan-Srivastava polynomials, are generated by (see [32] and [33])

j = 1 r { ( 1 x j z ) α j } = n = 0 g n ( α 1 , , α r ) ( x 1 , , x r ) z n , α j C ( j = 1 , 2 , , r ) ; | z | < min { | x 1 | 1 , , | x r | 1 } .
(2.2)

Clearly, the defined generating function (2.2) yields the explicit representation given by [[34], p.140, Eq. (6)]

g n ( α 1 , , α r ) ( x 1 ,, x r )= k 1 + + k r = n ( α 1 ) k 1 ( α r ) k r x 1 k 1 ! k 1 x r k r ! k r
(2.3)

or, equivalently, by [[14], p.522, Eq. (17)]

g n ( α 1 , , α r ) ( x 1 , , x r ) = n r 1 = 0 n n r 2 = 0 n r 1 n 1 = 0 n 2 ( α 1 ) n 1 ( α 2 ) n 2 n 1 ( α r ) n n r 1 n 1 ! ( n 2 n 1 ) ! ( n n r 1 ) ! x 1 n 1 x 2 n 2 n 1 x r n n r 1 .
(2.4)

On the other hand, Altin and Erkuş [34] presented a multivariable extension of the so-called Lagrange-Hermite polynomials generated by

j = 1 r { ( 1 x j z j ) α j } = n = 0 h n ( α 1 , , α r ) ( x 1 , , x r ) z n , α j C ( j = 1 , 2 , , r ) ; | z | < min { | x 1 | 1 , , | x r | 1 / r } .
(2.5)

The case r=2 of the polynomials given by (2.5) corresponds to the familiar (two-variable) Lagrange-Hermite polynomials considered by Dattoli et al. [23].

The multivariable polynomials

U n , 1 , , r ( α 1 , , α r ) ( x 1 ,, x r ),

which are defined by the following generating function [[32], p.268, Eq. (3)]:

j = 1 r { ( 1 x j z j ) α j } = n = 0 U n , 1 , , r ( α 1 , , α r ) ( x 1 , , x r ) z n , α j C ( j = 1 , 2 , , r ) ; j N ( j = 1 , 2 , , r ) ; | z | < min { | x 1 | 1 / 1 , , | x r | 1 / r } ,
(2.6)

are a unification (and generalization) of several known families of multivariable polynomials including (for example) Chan-Chyan-Srivastava polynomials

g n ( α 1 , , α r ) ( x 1 ,, x r )

defined by (2.2) (see [35] for details). Obviously, the Chan-Chyan-Srivastava polynomials

g n ( α 1 , , α r ) ( x 1 ,, x r )

follow as a special case of the polynomials due to Erkuş and Srivastava [35]

U n , 1 , , r α 1 , , α r ( x 1 ,, x r ),

when

j =1(j=1,,r),

where (as well as in what follows)

N={1,2,3,}and N 0 ={0,1,2,}=N{0}.

Moreover, the Lagrange-Hermite polynomials

h n ( α 1 , , α r ) ( x 1 ,, x r )

follow as a special case of the polynomials [35]

U n , 1 , , r ( α 1 , , α r ) ( x 1 ,, x r ),

when

j =1(j=1,,r).

The generating function (2.6) yields the following explicit representation ([[35], p.268, Eq. (4)]):

U n , 1 , , r ( α 1 , , α r ) ( x 1 ,, x r )= 1 k 1 + + r k r = n ( α 1 ) k 1 ( α r ) k r x 1 k 1 k 1 ! x r k r k r ! ,
(2.7)

which, in the special case when

j =1(j=1,,r),

corresponds to (2.3).

The following relationship is established between the polynomials due to Erkuş and Srivastava [35] and the Chan-Chyan-Srivastava polynomials by applying the generating functions (2.2) and (2.6) in [36].

n = 0 U n , 1 , , r ( α 1 , , α r ) ( x 1 , , x r ) z n = i = 1 r { ( 1 x i z i ) α i } = i = 1 r j = 1 i { ( 1 ω ( i , j ) z ) α i } = n = 0 g n ( α 1 , , α 1 , , α r , , α r ) ( ω 11 , , ω 1 1 , , ω r 1 , , ω r r ) z n ,
(2.8)

where it is tacitly assumed that the following set:

ω ( i , j ) :1irand1j i ( i N;i=1,,r),

which depends upon the i distinct values of the factor x i 1 i occurring in the expression

1 ( x i 1 i z ) i (i=1,,r),

exists such that

( 1 x i z i ) α i = j = 1 i { ( 1 ω ( i , j ) z ) j } (i=1,,r).

Thus, by assertion (2.8), we obtain the desired relationship as follows:

U n , 1 , , r ( α 1 , , α r ) ( x 1 ,, x r )= g n ( α 1 , , α 1 , , α r , , α r ) ( ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) ) .

Now by using the Erkuş-Srivastava multivariable polynomials given by (2.2), we introduce the following family of positive linear operators on C[0,1]:

T n ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) ( f ; x ) = i = 1 r { ( 1 x i z i ) } n m = 0 U m , 1 , , r ( α 1 , , α r ) ( x 1 , , x r ) z m k r n + k r 1 k r + 1 n + k r 1 f ( t ) d t = i = 1 r j = 1 i { ( 1 ω ( i , j ) z ) } n m = 0 g m ( ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) ) z n × ( n + k r 1 ) k r n + k r 1 k r + 1 n + k r 1 f ( t ) d t ,
(2.9)

where

α j C(j=1,2,,r); j N(j=1,2,,r);|z|<min { | x 1 | 1 / 1 , , | x r | 1 / r } .

Throughout this paper, we assume that

ω ( i , j ) = { ω ( n ) ( i , j ) } n N ,1ir and 1j i ( i N;i=1,,r),

are sequences of real numbers such that

0< ω ( i , j ) <1.

For convenience, taking r=1, i =2, α 1 = α 2 =n in (2.9), we have

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f ; x ) = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 g m ( n , n ) ( ω ( 1 , 1 ) , ω ( 1 , 2 ) ) x m k n + k 1 k + 1 n + k 1 f ( t ) d t = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 { k 1 = m ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 k n + k 1 k + 1 n + k 1 f ( t ) d t } x m .
(2.10)

Lemma 2.1 For each x[0,1] and nN,

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 0 ;x)=1 ( f 0 ( x ) = 1 ) .

Lemma 2.2 For each x[0,1] and nN,

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ;x)x ω n ( 1 , 1 ) + 1 2 n ( f 1 ( x ) = x ) .

Proof Let each x[0,1] be fixed. Then from (2.10) we get

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ; x ) = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 ( n + k 1 1 ) { k 1 = m ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 k n + k 1 k + 1 n + k 1 t d t } x m = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 ( n + k 1 1 ) { k 1 = m ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 [ t 2 2 ] k n + k 1 k + 1 n + k 1 } x m = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 k 1 = m ( 2 k 1 + 1 ) 2 ( n + k 1 ) ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 x m = x ω n ( 1 , 1 ) x ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 1 k 1 = 1 m ( ω n ( 1 , 1 ) ) k 1 1 k 1 1 ! ( n ) k 1 1 x m 1 = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 k 1 = m 1 2 ( n + k 1 ) ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 x m ω n ( 1 , 1 ) x + 1 2 n , 0 < ω n ( 1 , 1 ) < 1 , ω n ( 1 , 1 ) 1 .

 □

Lemma 2.3 For each x[0,1] and nN,

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ;x) x 2 ( ω n ( 1 , 1 ) ) 2 + 2 x ( ω n ( 1 , 1 ) ) n + 1 3 n 2 ( f 2 ( x ) = x 2 ) .

Proof Let each x[0,1] be fixed. Then from (2.10) we get

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ; x ) = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 ( n + k 1 1 ) { k 1 = m ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 k n + k 1 k + 1 n + k 1 t 2 d t } x m = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 ( n + k 1 1 ) { k 1 = m ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 [ t 3 3 ] k n + k 1 k + 1 n + k 1 } x m = ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 0 k = m ( n + k 1 ) ( ω n ( 1 , 1 ) ) k 1 ( k 1 ) ! ( n ) k 1 × { k 1 2 ( n + k 1 1 ) 3 + k 1 ( n + k 1 1 ) 3 + 1 3 ( n + k 1 1 ) 3 } x m = x ω n ( 1 , 1 ) ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 1 k = 1 m ( k n + k 1 ) { ( ω n ( 1 , 1 ) ) k 1 1 ( k 1 1 ) ! ( n ) k 1 1 } x m 1 + x ω n ( 1 , 1 ) ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 1 k = 1 m ( 1 n + k 1 ) × { ( ω n ( 1 , 1 ) ) k 1 1 ( k 1 1 ) ! ( n ) k 1 1 } x m 1 + x ω n ( 1 , 1 ) ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 1 k = 1 m ( 1 3 ( n + k 1 ) 2 ) { ( ω n ( 1 , 1 ) ) k 1 k 1 ! ( n ) k 1 } x m x 2 ( ω n ( 1 , 1 ) ) 2 ( 1 ω ( 1 , 1 ) x ) n ( 1 ω ( 1 , 2 ) x ) n m = 2 k = 2 m ( ( n + k 2 ) n + k 1 ) × { ( ω n ( 1 , 1 ) ) k 1 2 ( k 1 2 ) ! ( n ) k 1 2 } x m 2 + 2 x ω n ( 1 , 1 ) n + 1 3 n 2 x 2 ( ω n ( 1 , 1 ) ) 2 + 2 x ω n ( 1 , 1 ) n + 1 3 n 2 , T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ; x ) f 2 ( x ) x 2 ( ( ω n ( 1 , 1 ) ) 2 1 ) + 2 x ω n ( 1 , 1 ) n + 1 3 n 2 .
(2.11)

On the other hand, since

0 T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( y x ) 2 ; x ) = T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ;x)2x T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ;x)+ x 2 ,

it follows from Lemma 2.1 and Lemma 2.2 that

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ;x) f 2 (x)2 x 2 ( ( ω n ( 1 , 1 ) ) 2 1 ) .
(2.12)

Combining (2.11) and (2.12), we have

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ; x ) f 2 ( x ) | x 2 ( 1 ( ω n ( 1 , 1 ) ) 2 ) + 2 x ω n ( 1 , 1 ) n + 1 3 n 2 .

Then, taking supremum over x[0,1], we have

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ; x ) f 2 ( x ) x 2 ( 1 ( ω n ( 1 , 1 ) ) 2 ) + 2 x ω n ( 1 , 1 ) n + 1 3 n 2 .
(2.13)

 □

Remark 2.1

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

Remark 2.2 Let x[0,1], since T n ω ( 1 , 1 ) , ω ( 1 , 2 ) is linear, we get

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( y x ) 2 ; x ) = T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ; x ) 2 x T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ; x ) + x 2 T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 0 ; x ) x 2 ( ω ( 1 , 1 ) ) 2 + 2 x ω ( 1 , 1 ) n 2 x 2 ω ( 1 , 1 ) + x 2 2 x [ x ω n ( 1 , 1 ) + 1 2 n ] + x 2 x 2 ( ω ( 1 , 1 ) ) 2 + 2 x ω ( 1 , 1 ) n 2 x 2 ω ( 1 , 1 ) + x 2 + 1 3 n 2 x n .

3 A-statistical approximation

Let C[a,b] be a linear space of all real-valued continuous functions f on [a,b], and let T be a linear operator which maps C[a,b] into itself. We say that T is positive if for every non-negative fC[a,b], we have T(f,x)0 for all x[a,b] . We know that C[a,b] is a Banach space with the norm

f C [ a , b ] := sup x [ a , b ] | f ( x ) | ,fC[a,b].

For typographical convenience, we will write in place of C [ a , b ] if no confusion arises.

Theorem 3.1 Let A=( a j n ) be a non-negative regular summability matrix. Then

st A - lim n ω n ( 1 , 1 ) =1
(3.1)

if and only if for all fC[0,1],

st A - lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f ) f =0.
(3.2)

Proof Suppose that (3.2) holds for all fC[0,1]. Then we have

st A - lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ) f 1 =0
(3.3)

since f 1 C[0,1]. By Lemma 2.2, we have

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ) f 1 =1 ω n ( 1 , 1 ) .
(3.4)

By (3.3) and (3.4), we immediately get

st A - lim n ω n ( 1 , 1 ) =1.

Conversely, suppose that (3.1) holds. Then from Lemma 2.1 we have lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 0 ) f 0 =0. Hence

st A - lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 0 ) f 0 =0 ( f 0 ( x ) = 1 ) .
(3.5)

Also from Lemma 2.2 it follows that

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ) f 1 =1 ω n ( 1 , 1 ) .

Therefore, by using (3.1), we get

st A - lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 1 ) f 1 =0 ( f 1 ( x ) : = x ) .
(3.6)

Now we claim that

st A - lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ) f 2 =0 ( f 2 ( x ) : = x 2 ) .
(3.7)

By Lemma 2.3, we have

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ) f 2 2 ( 1 ω n ( 1 , 1 ) ) + 2 ω n ( 1 , 1 ) n + 1 3 n 2 .
(3.8)

Now, for a given ϵ>0, we define the following sets:

D : = { n : T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f 2 ) f 2 ϵ } , D 1 : = { n : 1 ω n ( 1 , 1 ) ϵ 4 } , D 2 : = { n : ω ( 1 , 1 ) n n ϵ 2 } , D 3 : = { n : 1 n 2 ϵ } .

From (3.8), it is easy to see that D D 1 D 2 D 3 . Then, for each jN, we get

n D a j n n D 1 a j n + n D 2 a j n + n D 3 a j n .
(3.9)

Using (3.3), we get

st A - lim n ( 1 ω n ( 1 , 1 ) ) =0

and

st A - lim n ω n ( 1 , 1 ) n =0.

Now, using the above facts and taking the limit as j in (3.9), we conclude that

lim j n D a j n =0,

which gives (3.7). Now, combining (3.5)-(3.7), and using the statistical version of the Korovkin approximation theorem (see Gadjiv and Orhan [10], Theorem 1), we get the desired result.

This completes the proof of the theorem. □

In a similar manner, we can extend Theorem 3.1 to the (i,j)-dimensional case for the operators T n ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) (f;x) given by (2.9) as follows.

Theorem 3.2 Let A=( a j n ) be a non-negative regular summability matrix. Then

st A - lim n ω n ( i , j ) =1

if and only if for all fC[0,1],

st A - lim n T n ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) ( f ) f =0.

Remark 3.1 If in Theorem 3.2 we replace A=( a j n ) by the identity matrix, we immediately get the following theorem which is a classical case of Theorem 3.2.

Theorem 3.3 lim n ω n ( i , j ) =1 if and only if for all fC[0,1], the sequence

T n ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) (f)

is uniformly convergent to f on [0,1].

Finally, we display an example which satisfies all the hypotheses of Theorem 3.2, but not of Theorem 3.3. Therefore, this indicates that our A-statistical approximation in Theorem 3.2 is stronger than its classical case.

Take A= C 1 :=( c j n ), the Cesàro matrix of order 1 and

ω ( i , j ) := ( ω n ( i , j ) ) n N (j=1,,r1)

are sequences of real numbers defined by

ω n ( i , j ) :={ 1 2 if  n = m 2 ( m N ) ; 1 1 n + i j otherwise .
(3.10)

We then observe that

0< ω n ( i , j ) <1(nN)

and also that

st A - lim n ω n ( i , j ) =1.

Therefore, by Theorem 3.2, we have that for all fC[0,1],

st A - lim n T n ω ( 1 , 1 ) , , ω ( 1 , 1 ) , , ω ( r , 1 ) , , ω ( r , r ) ( f ) f =0.

However, since the sequence ω n ( i , j ) defined by (3.10) is non-convergent, Theorem 3.3 does not hold in this case.

4 Direct theorems

By C B [0,1], we denote the space of all real-valued continuous bounded functions f on the interval [0,1], the norm on the space C B [0,1] is given by

f= sup 0 x 1 | f ( x ) | .

Peetre’s K-functional is defined by

K 2 (f,δ)=inf [ { f g + δ g : g W 2 } ] ,

where

W 2 = { g C B [ 0 , 1 ] : g , g C B [ 0 , 1 ] } .

By [14] there exists a positive constant c>0 s.t.

K 2 (f,δ)c w 2 ( f , δ 1 / 2 ) ,δ>0,

where the second-order modulus of smoothness is

w 2 (f, δ )= sup 0 h δ sup 0 x 1 | f ( x + 2 h ) 2 f ( x + h ) + f ( x ) | .

Also, for f C B [0,1], the usual modulus of continuity is given by

w(f,δ)= sup 0 h δ sup 0 x 1 | f ( x + h ) f ( x ) | .

Theorem 4.1 Let f C B [0,1] and 0 ω n ( i , j ) <1. Then, for all x[0,1] and nN, there exists an absolute constant C>0 s.t.

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f ; x ) f ( x ) | C w 2 ( f , δ n ( x ) ) ,

where

δ n 2 (x)= x 2 [ ( ω n ( 1 , 1 ) ) 2 2 ω n ( 1 , 1 ) + 1 ] + x ω n ( 1 , 1 ) n .

Proof Let g W 2 . From Taylor’s expansion

g(t)=g(x)+ g (x)(tx)+ x t (tx) g udu,t[0,1],

and from Lemmas (2.1), (2.2) and (2.3), we get

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (g,x)=g(x)+ T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( x t ( t x ) g ( u ) d u , x ) ,

hence

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( g , x ) g ( x ) | | T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( x t ( t x ) g ( u ) d u , x ) | | L n u ( 1 ) , u ( 2 ) ( ( t x ) 2 , x ) | g .

Using Remark 2.2, we obtain

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (g,x)g(x)| [ x 2 ( ω ( 1 , 1 ) ) 2 + 2 x ω ( 1 , 1 ) n 2 x 2 ω ( 1 , 1 ) + x 2 + 1 3 n 2 x n ] g .

On the other hand, by the definition of T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (f,x), we have

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (f;x)|f.

Next

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f , x ) f ( x ) | | T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( f g ) ; x ) ( f g ) ( x ) | + | T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( g , x ) g ( x ) | f g + [ x 2 ( ω ( 1 , 1 ) ) 2 + 2 x ω ( 1 , 1 ) n 2 x 2 ω ( 1 , 1 ) + x 2 + 1 3 n 2 x n ] g .

Hence, taking infimum on the right-hand side over all g W 2 , we get

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (f,x)f(x)|C K 2 ( f , δ n 2 ( x ) ) .

In view of the property of K-functional, for every 0< ω n ( i , j ) <1, we get

| T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (f,x)f(x)|C w 2 ( f , δ n ( x ) ) .

This completes the proof of the theorem. □

Theorem 4.2 Let f C B [0,1] be such that f , f C B [0,1] and 0< ω n ( i , j ) <1, j=1,2,3,,n, such that ω n ( i , j ) 1 as n. Then the following equality holds:

lim n n ( T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f , x ) f ( x ) ) = x 2 f (x)

uniformly on [0,1].

Proof By the Taylor’s formula, we may write

f(t)=f(x)+ f (x)(tx)+ 1 2 f (x) ( t x ) 2 +r(t,x) ( t x ) 2 ,
(4.1)

where r(t,x) is the remaining term and lim t x r(t,x)=0. Applying T n ω ( 1 , 1 ) , ω ( 1 , 2 ) (f;x) to (4.1), we obtain

n ( T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f , x ) f ( x ) ) = n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( t x ; x ) f ( x ) + n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( t x ) 2 ; x ) f ( x ) 2 + n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r ( t , x ) ( t x ) 2 ; x ) .

By the Cauchy-Schwartz inequality, we have

T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r ( t , x ) ( t x ) 2 ; x ) T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r 2 ( t , x ) 2 ; x ) T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( t x ) 4 ; x ) .
(4.2)

Observe that r 2 (x,x)=0 and r 2 (,x)C[0,1]. Then it follows from Theorem 4.1 that

lim n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r 2 ( t , x ) ; x ) = r 2 (x,x)=0
(4.3)

uniformly with respect to x[0,1].

Now, from (4.2), (4.3) and Remark 2.2, we get

lim n n T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r ( t , x ) ( t x ) 2 ; x ) =0.

Finally, using Remark 2.1, we get the following:

lim n n ( T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( f , x ) f ( x ) ) = lim n n ( f ( x ) T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( t x ) ; x ) ) + 1 2 f ( x ) T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( t x ) 2 ; x ) + 1 2 f ( x ) T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( ( t x ) 2 ; x ) + T n ω ( 1 , 1 ) , ω ( 1 , 2 ) ( r ( t , x ) ( t x ) 2 ; x ) = x 2 f ( x ) .

 □

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Mursaleen, M., Khan, F., Khan, A. et al. Some approximation results for generalized Kantorovich-type operators. J Inequal Appl 2013, 585 (2013). https://doi.org/10.1186/1029-242X-2013-585

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