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Article

Some New Families of Special Polynomials and Numbers Associated with Finite Operators

Department of Mathematics, Faculty of Science, University of Akdeniz, Antalya TR-07058, Turkey
Symmetry 2020, 12(2), 237; https://doi.org/10.3390/sym12020237
Submission received: 26 December 2019 / Revised: 14 January 2020 / Accepted: 29 January 2020 / Published: 4 February 2020

Abstract

:
The aim of this study was to define a new operator. This operator unify and modify many known operators, some of which were introduced by the author. Many properties of this operator are given. Using this operator, two new classes of special polynomials and numbers are defined. Many identities and relationships are derived, including these new numbers and polynomials, combinatorial sums, the Bernoulli numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers. By applying the derivative operator to these new polynomials, derivative formulas are found. Integral representations, including the Volkenborn integral, the fermionic p-adic integral, and the Riemann integral, are given for these new polynomials.

1. Introduction

Special polynomials, special numbers, special functions, and operators are widely used in mathematics, physics, and engineering. Our motivation was to construct new classes special polynomials and numbers with the help of an operator. By applying a derivative operator and p-adic integrals to these new special polynomials, many interesting identities, relations, and formulas were found. The results of this paper include some well-known special numbers, such as the Bernoulli numbers, the Cauchy numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers.
The following notations and definitions are used throughout this paper: Let
N = { 1 , 2 , 3 , } , N 0 = N { 0 } .
Let Z denote the set of integers, R denote the set of real numbers, and C denote the set of complex numbers.
0 n = 1 , ( n = 0 ) 0 , ( n N )
and
λ 0 = 1 and λ v = λ ( λ 1 ) ( λ v + 1 ) v ! = λ v v ! ( v N , λ C )
(cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
The Bernoulli numbers of first kind B n are defined by:
t e t 1 = n = 0 B n t n n ! ,
where t < 2 π (cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
The Euler numbers of first kind E n are defined by:
2 e t + 1 = n = 0 E n t n n ! ,
where t < π (cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
The Euler polynomials of second kind E n x are defined by:
2 e t + e t e t x = n = 0 E n x t n n ! ,
where t < π 2 . For x = 0 , we have:
E n = E n 0 ,
which denotes the Euler numbers of the second kind (cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
Let k N 0 . The Stirling numbers of the second kind S 2 ( n , k ) are defined by:
e t 1 k k ! = n = 0 S 2 ( n , k ) t n n ! ,
Using Equation (2), we have S 2 ( n , k ) = 0 if n < k or k < 0 (cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
The Stirling numbers of the first kind S 1 ( n , k ) are defined by:
( log ( 1 + t ) ) k k ! = n = 0 S 1 ( n , k ) t n n ! .
Using Equation (3), we have S 1 ( n , k ) = 0 if k > n or k < 0 (cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]).
The λ -array polynomials S k n ( x ; λ ) are defined by:
1 k ! e t x λ e t 1 k = n = 0 S k n ( x ; λ ) t n n !
(cf. [2,6,30]).
The Bernoulli numbers of the second kind (or the Cauchy numbers of the first kind) b n ( 0 ) are defined by:
t log ( 1 + t ) = n = 0 b n ( 0 ) t n n ! .
The numbers b n ( 0 ) are also given by:
b n ( 0 ) = 0 1 u n d u
(cf. [26] (p. 116)).
The central factorial numbers of the second kind T ( n , k ) are defined by:
1 ( 2 k ) ! e t + e t 2 k = n = 0 T ( n , k ) t 2 n ( 2 n ) !
(cf. [4,8,9]).

Operators O λ f ; a , b and T λ f ; a , b

Let a , x R and
E a f ( x ) = f ( x + a )
(cf. [1,2,9,11,27,36,37]). The operators O λ f ; a , b and T λ f ; a , b are as follows, respectively:
O λ f ; a , b ( x ) = λ E a f ( x ) + E b f ( x ) ,
and
T λ f ; a , b ( x ) = O λ f ; a , b x a + b + 1 ,
where λ , a, and b are real parameters. (cf. [1]). In [1], the following special cases of the operator T λ f ; a , b were provided. These special cases have many different applications in mathematics, engineering, etc.:
1 2 T 1 f ; 0 , 0 ( x ) = I f ( x ) , ( Identity Operator ) 2 T 1 f ; 1 , 0 ( x ) = Δ f ( x ) , ( Forward Difference Operator ) I f ( x ) + 1 2 T 1 f ; 1 , 1 ( x ) = f ( x ) , ( Backward Difference Operator ) T 1 f ; 1 , 0 ( x ) = M f ( x ) , ( Means Operator ) T 1 f ; 1 2 , 1 2 ( x ) = δ f ( x ) , ( Central Difference Operator ) 1 2 T 1 f ; 1 2 , 1 2 ( x ) = μ f ( x ) , ( Averaging Difference Operator ) ( 2 a + b + 1 ) T 1 f ; a + b , a ( x ) = Δ b E a f ( x ) , ( a b , Gould Operator ) 2 T λ f ; 1 , 0 ( x ) = Δ λ f ( x ) .
For details about the above operators and their applications, see [1,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36].
The remainder of this paper is structured as follows: Section 2 outlines a new finite operator is defined. Some properties of this operator are given. In Section 3, using this new operator, two new classes of special polynomials and numbers are defined. The derivative formulas for these new polynomials are given. In Section 4, some integral representations related to the Volkenborn integral, the fermionic p-adic integral, and the Riemann integral for these new polynomials are given. Using these integral representations, many new identities and formulas are derived including the Bernoulli numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers. Finally, Section 5 provides the conclusions.

2. A New Operator

In this section, we define a new operator that modifies the operators O λ f ; a , b and T λ f ; a , b . Some properties of this operator are given.
Let a and b be real parameters. Let λ and β be real or complex parameters. A new operator Y λ , β f ; a , b is defined by:
Y λ , β f ; a , b ( x ) = λ E a f ( x ) + β E b f ( x ) .
Some special values of this operator are given as follows:
Y λ , β f ; a , b x = β O λ β f ; a , b x
and
Y λ , β f ; a , b x = β a + b + 1 T λ β f ; a , b ( x )
(cf. [1]).
Y λ , 1 f ; 1 , 0 ( x ) = Δ λ f ( x ) = λ f ( x + 1 ) + f ( x )
(cf. [2]).
Y 1 , 0 f ; a , 0 ( x ) = E a f ( x ) .
Y 1 , 1 f ; a , 0 ( x ) = Δ a f ( x ) = f ( x + a ) f ( x ) ,
where Δ a denotes the forward difference operator.
Y 1 , 1 f ; 0 , b ( x ) = b f ( x ) = Y 1 , 1 f ; b , 0 Y 1 , 0 f ; b , 0 f ( x ) = Y 1 , 1 f ; b , 0 Y 1 , 0 f ; 0 , b f ( x ) = E b I E b f ( x ) = f ( x ) f ( x b ) ,
where b denotes the backward difference operator.
Y 1 , 1 f ; a 2 , a 2 ( x ) = δ a f ( x ) = E a 2 E a 2 f ( x ) = f x + a 2 f x a 2 ,
where δ a denotes the central difference operator.
Y 1 , 1 f ; a 2 , a 2 = Y 1 , 1 f ; a , 0 Y 1 , 0 f ; a 2 , 0 = Y 1 , 1 f ; 0 , a Y 1 , 0 f ; a 2 , 0 = δ a f
(cf. [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36]). The Gould operator is:
Y 1 , 0 f ; a + b , 0 Y 1 , 0 f ; a , 0 = G a , b f ,
where a b (cf. [25]).
a Δ 1 = Y 1 , 0 f ; a , 0 I f a
(cf. [11] (p. 27, Equation (1.17))).
The operator f is provided by Goldstine [11] (p. 128). Applying this operator to f ( x ) = E n ( x ) , we have:
f ( x ) = Y 1 , 0 f ; 1 , 0 ( x ) + f ( x ) 2 = x n ,
where n N 0 . Therefore,
k = 0 m 1 ( 1 ) k k n = 1 2 k = 0 m 1 ( 1 ) k Y 1 , 0 f ; 1 , 0 ( k ) + f ( k ) = 1 2 E n ( 0 ) ( 1 ) m E n ( m ) ,
(cf. [11] (p. 136)).
Let,
Y λ , β k f ; a , b = Y λ , β f ; a , b Y λ , β k 1 f ; a , b
where k N .
By applying the operator in Equation (10) k-times to the function f, and using Equation (11), we obtain:
Y λ , β k f ; a , b ( x ) = j = 0 k k j λ k j β j f ( x + j b + ( k j ) a ) .
Remark 1.
Substituting b = 0 and β = 1 into (12), we have:
Y λ , 1 k f ; 1 , 0 ( x ) = j = 0 k k j λ k j ( 1 ) j f ( x + ( k j ) a ) = Δ λ k f ( x )
(cf. [2] (p. 155, Equation (29))).
Remark 2.
Substituting f ( x ) = x n , b = 0 , and β = 1 into Equation (12), the polynomials Y λ , 1 k x n ; 1 , 0 ( 0 ) reduce to λ-array polynomials S k n ( x ; λ ) :
Y λ , 1 k x n ; 1 , 0 ( x ) = Δ λ k x n ( x ) = S k n x ; λ
(cf. [2] (p. 155)).
Substituting a = 1 2 , b = 1 2 , λ = 1 and β = 1 into Equation (12), we have:
δ f ( x ) = Y 1 , 1 k f ; 1 2 , 1 2 ( x ) = j = 0 k ( 1 ) j k j f x j + k 2 .
Substituting f ( x ) = x n ( n N 0 ) into the previous equation, we have:
Y 1 , 1 k x n ; 1 2 , 1 2 ( x ) = j = 0 k ( 1 ) j k j x j + k 2 n .
Let:
Y λ , β j f ; a , b ( 0 ) = Y λ , β j f ; a , b ( x ) x = 0 .
Substituting x = 0 into Equation (13), we obtain:
T ( n , k ) = 1 k ! Y 1 , 1 k x n ; 1 2 , 1 2 ( 0 ) .
where n , k N 0 and:
δ f ( 0 ) = Y 1 , 1 k x n ; 1 2 , 1 2 ( 0 ) .
Equation (14) is also provided in ([4] Equation (2.8)), [20,32].

3. New Families of Special Polynomials and Numbers

In this section, we define two new classes of special polynomials and numbers.
Substituting f ( x ) = l = 1 n d l x l ( n N 0 and d l R ) into (12), we define a new class of special polynomials as follows:
P n ( x , k ; a , b ; λ , β , d ) = l = 1 n d l Y λ , β k x l ; a , b ( x ) ,
where,
d = ( d 1 , d 2 , , d n ) .
Therefore,
P n ( x , k ; a , b ; λ , β , d ) = j = 0 k k j λ k j β j l = 1 n ( x + j b + ( k j ) a ) l d l .
Observe that for β = 1 , Equation (15) is unification of Equation (21) in [1]. Using Equation (15), we obtain:
P n ( x , k ; a , b ; λ , β , d ) = j = 0 k k j λ k j β j l = 1 n d l v = 0 l l v x v ( j b + ( k j ) a ) l v
After some elementary calculations, we obtain:
P n ( x , k ; a , b ; λ , β , d ) = l = 1 n v = 0 l l v d l x v Y λ , β k x l v ; a , b ( 0 ) .
With the help of the previous equation, a new class of special numbers can now be defined as follows:
y 5 ( n , k ; a , b ; λ , β ) = l = 1 n d l Y λ , β k x l ; a , b ( 0 ) .
Combining the above definition with Equation (12), we have:
y 5 ( n , k ; a , b ; λ , β ) = j = 0 k k j λ k j β j l = 1 n d l ( j b + ( k j ) a ) l .
Observe that for β = 1 , Equation (16) is unification of Equation (22) in [1].
By applying the derivative operator d k d x k to Equation (15), we obtain the derivative formula for polynomials P n ( x , k ; a , b ; λ , β ) as follows:
d k d x k P n ( x , k ; a , b ; λ , β , d ) = j = 0 k k j λ k j β j l = 1 n ( l ) k ( x + j b + ( k j ) a ) l k d l .
Combining the above equation with the following well-known formula (cf. [26]):
( y ) k = j = 0 k S 1 ( k , j ) y j ,
we obtain a derivative formula for the polynomials P n ( x , k ; a , b ; λ , β ) by the following theorem:
Theorem 1.
Let n N and k N 0 with k n . Then, we have:
d k d x k P n ( x , k ; a , b ; λ , β , d ) = j = 0 k k j λ k j β j l = 1 n d l m = 0 k S 1 ( k , m ) l m ( x + j b + ( k j ) a ) l k .
We now define another class of special polynomials as follows:
Q n x ; a , b ; λ , β = j = 0 n x j Y λ , β j f ; a , b ( 0 ) .
In Equation (19), we assume that the values f ( 0 ) and f ( m b + ( j m ) a ) are finite.
Using Equation (19), we obtain:
Q n x ; a , b ; λ , β = j = 0 n m = 0 j x j j m λ j m β m f ( m b + ( j m ) a ) .
Some special values of the polynomials Q n x ; a , b ; λ , β are given as follows:
Substituting n = 2 , f ( y ) = e y , and
Y λ , β j e y ; a , b ( 0 ) = m = 0 j j m λ j m β m e m b + ( j m ) a
into Equation (19), we have:
Q 2 x ; a , b ; λ , β = 1 + x m = 0 1 1 m λ 1 m β m e m b + ( 1 m ) a + x 2 m = 0 2 2 m λ 2 m β m e m b + ( 2 m ) a .
Therefore,
Q 2 x ; a , b ; λ , β = 1 + λ e a + β e b λ e a + β e b 2 x + λ e a + β e b 2 x 2 .
Substituting λ = 1 , β = 1 , and b = a into (21), we have:
Q 2 x ; a , a ; 1 , 1 = 1 + 2 x sinh ( a ) cosh ( 2 a ) + 1 + 4 x 2 sinh 2 ( a ) = 1 + 2 x sinh ( a ) 2 sinh 2 ( a ) + 4 x 2 sinh 2 ( a ) .
Substituting λ = 1 , β = 1 , and b = a into (21), we have:
Q 2 x ; a , a ; 1 , 1 = 1 + 2 x e 2 a .
Substituting a = 0 into the aforementioned equation, we have:
Q 2 x ; 0 , 0 ; 1 , 1 = 1 + 2 x .
Substituting f ( x ) = x n , a = λ = 1 and β = 1 and b = 0 into Equation (20), we obtain:
Q n x ; 1 , 0 ; 1 , 1 = j = 0 n x j j ! S 2 ( n , j ) .
Therefore,
Q n x ; 1 , 0 ; 1 , 1 = x n .
Combining Equations (22) and (17), we obtain the following corollary:
Corollary 1.
Let n N 0 . Then, we have:
Q n x ; 1 , 0 ; 1 , 1 = j = 0 n l = 0 j S 2 ( n , j ) S 1 ( j , l ) x l .

Derivative Formula for Polynomials Q n x ; a , b ; λ , β

Here, we provide a derivative formula for the polynomials Q n x ; a , b ; λ , β .
Taking derivative of Equation (19) with respect to x, and using the following well-known derivative formula for the function x n (cf. [24,33]):
d d x x n = x n m = 0 n 1 1 x m ,
we obtain:
d d x Q n x ; a , b ; λ , β = d d x j = 0 n x j Y λ , β j f ; a , b ( 0 ) = j = 1 n Y λ , β j f ; a , b ( 0 ) j ! ( x ) j m = 0 j 1 1 x m .
After some elementary calculations in the above equation, we arrive at the following theorem:
Theorem 2.
Let n N . Then, we have:
d d x Q n x ; a , b ; λ , β = j = 1 n x j Y λ , β j f ; a , b ( 0 ) m = 0 j 1 1 x m .

4. Integral Representations for the Polynomials Qn (x; a, b; λ, β)

In this section, we provide the Riemann integral and p-adic integrals representations for the polynomials Q n x ; a , b ; λ , β . Using these integrals representations, many new identities and formulas are derived including combinatorial sums, the Bernoulli numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers.

4.1. Riemann Integral Formulas of Polynomials Q n x ; a , b ; λ , β

Here, we provide some integral formulas for Q n x ; a , b ; λ , β polynomials. Using these formulas, some new identities and combinatorial sums are derived including the Stirling numbers and the Bernoulli numbers of the second kind.
Integrating Equation (20) from 0 to 1 and using ( refLamdaFun-1p), we obtain:
0 1 Q n x ; a , b ; λ , β d x = j = 0 n m = 0 j j m b j ( 0 ) λ j m β m f ( m b + ( j m ) a ) j ! .
Integrating Equations (22)–(24) from 0 to 1, we obtain:
0 1 Q n x ; 1 , 0 ; 1 , 1 d x = j = 0 n S 2 ( n , j ) b j ( 0 ) ,
0 1 Q n x ; 1 , 0 ; 1 , 1 d x = 1 n + 1 ,
and
0 1 Q n x ; 1 , 0 ; 1 , 1 d x = j = 0 n l = 0 j 1 l + 1 S 2 ( n , j ) S 1 ( j , l ) .
Combining Equations (26) and (28), we arrive at the following theorem:
Theorem 3.
Let n, k N 0 . Then, we have:
j = 0 n l = 0 j 1 l + 1 S 2 ( n , j ) S 1 ( j , l ) = j = 0 n S 2 ( n , j ) b j ( 0 ) .
Remark 3.
Considering the method reported by Simsek and Cakic [34], using the orthogonality relation of the Stirling numbers, Equation (29) reduces to the following well-known relation:
j = 0 n S 2 ( n , j ) b j ( 0 ) = 1 n + 1
(cf. [5,7,9,12,25,26,34,35,36,37]). Additionally, by combining (26) with (27), we obtain Equation (30).

4.2. p-Adic Integrals Formulas of the Polynomials Q n x ; a , b ; λ , β

Here, by applying p-adic integrals to the polynomials Q n x ; a , b ; λ , β , many p-adic integral formulas are derived. Using these p-adic integral formulas, some new combinatorial sums including the Bernoulli numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers are given.
We need the following definitions and notations for p-adic integrals:
Let Z p and Q p denote the set of p-adic integers and the set of p-adic rational numbers, respectively. Let C p denote the field of p-adic completion of algebraic closure of Q p . Let f : Z p C p be a uniformly differentiable function. C 1 ( Z p C p ) denotes a set of uniformly differentiable functions.
Let f C 1 ( Z p C p ) . The Volkenborn integral of the function f on Z p is defined by:
Z p f x d μ 1 x = lim N 1 p N x = 0 p N 1 f x ,
where μ 1 x denotes the Haar distribution:
μ 1 x = 1 p N
(cf. [16,18,19,27,32,38]).
The fermionic p-adic integral of the function f is defined by:
Z p f x d μ 1 x = lim N x = 0 p N 1 1 x f x ,
where:
μ 1 x = 1 x
(cf. [17,18,19] see also [21,32]).
Some p-adic integrals formulas are given as follows:
B n = Z p x n d μ 1 x ,
(cf. [16,17,27,32]).
Z p x n d μ 1 x = ( 1 ) n n + 1 = D n n ! ,
where D n denotes the Daehee numbers (cf. [14,27,32]).
E n = Z p x n d μ 1 x
(cf. [17]).
Z p x n d μ 1 x = ( 1 ) n 2 n = C h n n ! ,
where C h n denotes the Changhee numbers (cf. ([15] Theorem 2.3), [32]).
By applying the Volkenborn integral to Equation (20), using Equations (33) and (34), we obtain the following results, respectively:
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j j m 1 j j + 1 λ j m β m f ( m b + ( j m ) a ) ,
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j j m D j j ! λ j m β m f ( m b + ( j m ) a ) ,
and
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l B l λ j m β m f ( m b + ( j m ) a ) .
Combining Equations (37) and (39), we obtain the following theorem:
Theorem 4.
Let n N 0 . Then, we have:
j = 0 n m = 0 j j m 1 j j + 1 λ j m β m f ( m b + ( j m ) a ) = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l B l λ j m β m f ( m b + ( j m ) a ) .
Combining Equations (38) and (39), we obtain the following theorem:
Theorem 5.
Let n N 0 . Then we have
j = 0 n m = 0 j j m D j j ! λ j m β m f ( m b + ( j m ) a ) = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l B l λ j m β m f ( m b + ( j m ) a ) .
Substituting a = 1 , b = 0 , λ = 1 , β = 1 into (40), we arrive at the following result:
Corollary 2.
Let n N 0 . Then, we have:
j = 0 n l = 0 j B l S 2 ( n , j ) S 1 ( j , l ) = j = 0 n S 2 ( n , j ) D j .
Remark 4.
Using the orthogonality relation of the Stirling numbers, Equation (41) reduces to the following well-known formula:
B n = j = 0 n S 2 ( n , j ) D j
(cf. [14,26,32,34]).
By applying the fermionic p-adic to Equation (20), using Equations (35) and (36), we obtain the following results, respectively:
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j j m 1 j 2 j λ j m β m f ( m b + ( j m ) a ) ,
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j j m λ j m β m f ( m b + ( j m ) a ) C h j j ! ,
and
Z p Q n x ; a , b ; λ , β d μ 1 x = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l E l λ j m β m f ( m b + ( j m ) a ) .
Combining Equations (42) and (44), we arrive at the following theorem:
Theorem 6.
Let n N 0 . Then, we have:
j = 0 n m = 0 j j m 1 j 2 j λ j m β m f ( m b + ( j m ) a ) = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l E l λ j m β m f ( m b + ( j m ) a ) .
Combining Equations (42) and (44), we obtain the following theorem:
Theorem 7.
Let n N 0 . Then, we have:
j = 0 n m = 0 j j m λ j m β m f ( m b + ( j m ) a ) C h j j ! = j = 0 n m = 0 j 1 j ! l = 0 j j m S 1 j , l E l λ j m β m f ( m b + ( j m ) a ) .
Substituting a = 1 , b = 0 , λ = 1 , β = 1 into Equation (45), we obtain the following corollary:
Corollary 3.
Let n N 0 . Then, we have:
j = 0 n l = 0 j E l S 2 ( n , j ) S 1 ( j , l ) = j = 0 n S 2 ( n , j ) C h j .
Remark 5.
Using the orthogonality relation of the Stirling numbers, Equation (46) reduces to the following well-known formula:
E n = j = 0 n S 2 ( n , j ) C h j
(cf. [12,15,26,32,34]).

5. Conclusions

This paper introduced a new operator and new two classes of special polynomials and numbers. Many properties of this new operator, polynomials, and numbers were outlined. Using this operator, some special values of these special numbers and polynomials were derived. Many fundamental properties of these numbers and polynomials were investigated. p-adic integrals and the Riemann integral representations for these polynomials were provided. Using these integral representations, identities and formulas were derived including combinatorial sums, the Bernoulli numbers, the Euler numbers, the Stirling numbers, the Daehee numbers, and the Changhee numbers. The results of this paper may potentially be used in mathematics, physics, and engineering.

Funding

This research received no external funding.

Acknowledgments

The present investigation was supported by Scientific Research Project Administration of Akdeniz University. The author would like to thank the referees for their suggestions and comments.

Conflicts of Interest

The author declares no conflict of interest.

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Simsek, Y. Some New Families of Special Polynomials and Numbers Associated with Finite Operators. Symmetry 2020, 12, 237. https://doi.org/10.3390/sym12020237

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Simsek Y. Some New Families of Special Polynomials and Numbers Associated with Finite Operators. Symmetry. 2020; 12(2):237. https://doi.org/10.3390/sym12020237

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Simsek, Yilmaz. 2020. "Some New Families of Special Polynomials and Numbers Associated with Finite Operators" Symmetry 12, no. 2: 237. https://doi.org/10.3390/sym12020237

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