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Article

Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials

1
Department of Mathematics, Sogang University, Seoul 04107, Korea
2
Department of Mathematics, Kwangwoon University, Seoul 01897, Korea
3
Department of Mathematics, Pusan National University, Busan 46241, Korea
*
Author to whom correspondence should be addressed.
Symmetry 2019, 11(5), 613; https://doi.org/10.3390/sym11050613
Submission received: 13 April 2019 / Revised: 24 April 2019 / Accepted: 28 April 2019 / Published: 2 May 2019
(This article belongs to the Special Issue Current Trends in Symmetric Polynomials with Their Applications Ⅱ)

Abstract

:
The main purpose of this paper is to give several identities of symmetry for type 2 Bernoulli and Euler polynomials by considering certain quotients of bosonic p-adic and fermionic p-adic integrals on Z p , where p is an odd prime number. Indeed, they are symmetric identities involving type 2 Bernoulli polynomials and power sums of consecutive odd positive integers, and the ones involving type 2 Euler polynomials and alternating power sums of odd positive integers. Furthermore, we consider two random variables created from random variables having Laplace distributions and show their moments are given in terms of the type 2 Bernoulli and Euler numbers.

1. Introduction

In this section, we are going to review some known results. We first recall the definitions of Bernoulli and Euler polynomials together with their type 2 polynomials. Then, we introduce the bosonic p-adic integrals and the fermionic p-adic integrals on Z p that we need for the derivation of an identity of symmetry. As is well known, the Bernoulli polynomials are defined by
t e t 1 e x t = n = 0 B n ( x ) t n n ! ,
(see [1,2]).
In particular, the Bernoulli numbers are the constant terms B n = B n ( 0 ) of the Bernoulli polynomials. By making use of (1), we can deduce that
l = 0 n 1 l k = 1 k + 1 ( B k + 1 ( n ) B k + 1 ) , for k = 0 , 1 , 2 , .
The type 2 Bernoulli polynomials are defined by generating function
t e t e t e x t = n = 0 b n ( x ) t n n ! ,
(see [3,4]).
In particular, b n = b n ( 0 ) are called type 2 Bernoulli numbers. From (3), it can be seen that
b n ( x ) = k = 0 n n k b k x n k ,
(see [3,4]).
Analogously to (2), we observe that
l = 0 n 1 e ( 2 l + 1 ) t = 1 e t e t ( e 2 n t 1 ) = k = 0 b k + 1 ( 2 n ) b k + 1 k + 1 t k k ! .
Thus, by (5), we get
l = 0 n 1 ( 2 l + 1 ) k = 1 k + 1 ( b k + 1 ( 2 n ) b k + 1 ) , k = 0 , 1 , 2 , .
Let p be a fixed odd prime number. Throughout this paper, we will use the notations Z p , Q p , C p , and C to denote the ring of p-adic rational integers, the field of p-adic rational numbers, the completion of an algebraic closure of Q p , and the field of complex numbers, respectively. The normalized valuation in C p is denoted by | · | p , with | p | p = 1 p . For a uniformly differentiable function f on Z p , the bosonic p-adic integral on Z p (or p-adic invariant integral on Z p ) is defined by
Z p f ( x ) d μ 0 ( x ) = lim N x = 0 p N 1 f ( x ) μ 0 ( x + p N Z p ) = lim N 1 p N x = 0 p N 1 f ( x ) .
Then, by (7), we easily get
Z p f ( x + 1 ) d μ 0 ( x ) Z p f ( x ) d μ 0 ( x ) = f ( 0 ) ,
(see [5,6]).
The fermionic integral on Z p is defined by Kim [6] as
Z p f ( x ) d μ 1 ( x ) = lim N x = 0 p N 1 f ( x ) μ 1 ( x + p N Z p ) = lim N x = 0 p N 1 f ( x ) ( 1 ) x .
From (9), we can show that
Z p f ( x + 1 ) d μ 1 ( x ) + Z p f ( x ) d μ 1 ( x ) = 2 f ( 0 ) ,
(see [4,7,8,9,10]).
It is well known that the Euler polynomials are defined by
2 e t + 1 e x t = n = 0 E n * ( x ) t n n ! .
We denote the Euler numbers by E n * = E n * ( 0 ) , ( n 0 ) . Clearly, we have
2 l = 0 n 1 ( 1 ) l e l t = 2 e t + 1 ( e n t + 1 ) , where n 1 ( mod 2 ) .
From (11) and (12), we obtain that
2 l = 0 n 1 ( 1 ) l l k = E k * ( n ) + E k * ,
where n is a positive odd integer.
Now, we consider the type 2 Euler polynomials which are given by
2 e t + e t e x t = sec h ( t ) e x t = n = 0 E n ( x ) t n n ! .
In particular, when x = 0 , E n = E n ( 0 ) are called the type 2 Euler numbers.
In this paper, we obtain some identities of symmetry involving the type 2 Bernoulli polynomials, the type 2 Euler polynomials, power sums of odd positive integers and alternating power sums of odd positive integers which are derived from certain quotients of bosonic p-adic and fermionic p-adic integrals on Z p . In the following section, we will construct two random variables from random variables having Laplace distributions whose moments are closely related to the type 2 Bernoulli and Euler numbers. All the results in Section 2 and Section 3 are newly developed. Finally, we note that the results here have applications in such diverse areas as combinatorics, probability, algebra and analysis (see [11,12,13]).

2. Some Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials

In virtue of (8), we readily see that
1 2 Z p e ( 2 x + 1 ) t d μ 0 ( x ) = t e t e t .
Hence, by (15), we get
1 2 Z p ( 2 x + 1 ) n d μ 0 ( x ) = b n , ( n 0 ) .
In addition, it follows from (15) that
1 2 Z p e ( 2 y + x + 1 ) t d μ 0 ( y ) = t e t e t e x t = n = 0 b n ( x ) t n n ! .
Hence, by (17), we get
1 2 Z p ( 2 y + x + 1 ) n d μ 0 ( y ) = b n ( x ) , ( n 0 ) .
Using (15) and (17), one can easily check that
1 2 Z p e ( 2 x + 2 n + 1 ) t d μ 0 ( x ) Z p e ( 2 x + 1 ) t d μ 0 ( x ) = t l = 0 n 1 e ( 2 l + 1 ) t .
Next, we let T k ( n ) = l = 0 n ( 2 l + 1 ) k , ( k N { 0 } ) . Note that T k ( n ) represents the kth power sums of consecutive positive odd integers. By (19), we easily get
Z p e ( 2 x + 1 + 2 n ) t d μ 0 ( x ) Z p e ( 2 x + 1 ) t d μ 0 ( x ) = 2 n t Z p e ( 2 x + 1 ) t d μ 0 ( x ) Z p e 2 n x t d μ 0 ( x ) .
Let w 1 , w 2 be positive integers. Then, we observe that
w 1 Z p e ( 2 x + 1 ) t d μ 0 ( x ) Z p e 2 w 1 x t d μ 0 ( x ) = l = 0 w 1 1 e ( 2 l + 1 ) t = k 0 l = 0 w 1 1 ( 2 l + 1 ) k t k k ! = k = 0 T k ( w 1 1 ) t k k ! .
Now, we consider the next quotient of bosonic p-adic integrals on Z p from which the identities of symmetry for the type 2 Bernoulli polynomials follow:
I ( w 1 , w 2 ) = w 1 w 2 2 Z p Z p e ( 2 w 1 x 1 + w 1 + 2 w 2 x 2 + w 2 + w 1 w 2 x ) t d μ 0 ( x 1 ) d μ 0 ( x 2 ) Z p e 2 w 1 w 2 x t d μ 0 ( x ) .
From (22), we have
I ( w 1 , w 2 ) = w 2 2 Z p e ( 2 x 1 + w 2 x + 1 ) w 1 t d μ 0 ( x ) w 1 Z p e ( 2 w 2 x 2 + w 2 ) t d μ 0 ( x 2 ) Z p e 2 w 1 w 2 x t d μ 0 ( x ) = w 2 k = 0 b k ( w 2 x ) w 1 k k ! t k l = 0 T l ( w 1 1 ) w 2 l l ! t l = n = 0 k = 0 n n k b k ( w 2 x ) T n k ( w 1 1 ) w 1 k w 2 n k + 1 t n n ! .
We note from (22) that I ( w 1 , w 2 ) = I ( w 2 , w 1 ) . Interchanging w 1 and w 2 , we get
I ( w 2 , w 1 ) = n = 0 k = 0 n n k b k ( w 1 x ) T n k ( w 2 1 ) w 2 k w 1 n k + 1 t n n ! .
Therefore, by (23) and (24), we obtain the following theorem.
Theorem 1.
For w 1 , w 2 N and n N { 0 } , we have
k = 0 n n k b k ( w 2 x ) T n k ( w 1 1 ) w 1 k w 2 n k + 1 = k = 0 n n k b k ( w 1 x ) T n k ( w 2 1 ) w 2 k w 1 n k + 1 .
Setting x = 0 in Theorem 1, we obtain the following corollary.
Corollary 1.
For w 1 , w 2 N and n N { 0 } , we have
k = 0 n n k b k T n k ( w 1 1 ) w 1 k w 2 n k + 1 = k = 0 n n k b k T n k ( w 2 1 ) w 2 k w 1 n k + 1 .
Furthermore, let us take w 2 = 1 in Corollary 1. Then, we have
k = 0 n n k b k w 1 n k + 1 = k = 0 n n k b k T n k ( w 1 1 ) w 1 k .
Therefore, by (4) and (25), we obtain the following corollary.
Corollary 2.
For w 1 N and n N { 0 } , we have
b n ( w 1 ) = k = 0 n n k b k T n k ( w 1 1 ) w 1 k 1 = k = 0 n n k b k w 1 k 1 l = 0 w 1 1 ( 2 l + 1 ) n k .
From (22), we observe that
I ( w 1 , w 2 ) = w 2 2 e w 1 w 2 x t Z p e 2 w 1 x 1 t + w 1 t d μ 0 ( x 1 ) w 1 Z p e ( 2 w 2 x 2 + w 2 ) t d μ 0 ( x 1 ) Z p e 2 w 1 w 2 x t d μ 0 ( x ) = w 2 2 e w 1 w 2 x t Z p e ( 2 w 1 x 1 + w 1 ) t d μ 0 ( x 1 ) l = 0 w 1 1 e ( 2 l + 1 ) w 2 t = w 2 2 l = 0 w 1 1 Z p e 2 x 1 + 1 + w 2 x + ( 2 l + 1 ) w 2 w 1 w 1 t d μ 0 ( x 1 ) = n = 0 w 2 l = 0 w 1 1 b n w 2 x + ( 2 l + 1 ) w 2 w 1 w 1 n t n n ! .
By interchanging w 1 and w 2 , we obtain the following equation:
I ( w 2 , w 1 ) = n = 0 w 1 l = 0 w 2 1 b n w 1 x + ( 2 l + 1 ) w 1 w 2 w 2 n t n n ! .
As I ( w 1 , w 2 ) = I ( w 2 , w 1 ) , the following theorem is immediate from (26) and (27).
Theorem 2.
For w 1 , w 2 N and n N { 0 } , we have
w 1 n w 2 l = 0 w 1 1 b n w 2 x + ( 2 l + 1 ) w 2 w 1 = w 2 n w 1 l = 0 w 2 1 b n w 1 x + ( 2 l + 1 ) w 1 w 2 .
Example 1.
We check the result in Theorem 2 in the case of n = 2 , w 1 = 3 , and w 2 = 7 . We first note that b 2 ( x ) = 1 2 ( x 2 1 3 ) . This can be obtained from B 2 ( x ) = x 2 x + 1 6 and the relation b n ( x ) = 2 n 1 B n ( x + 1 2 ) which follows from (1) and (3). Thus, we have to see that
l = 0 2 7 x + 7 3 ( 2 l + 1 ) 2 1 3 = 7 3 l = 0 6 3 x + 3 7 ( 2 l + 1 ) 2 1 3 .
Now, we can easily show that both the left and the right side of (28) are equal to 147 x 2 + 294 x + 1706 9 .
Let us take w 1 = 1 . Then, by Theorem 2, we get
w 2 b n ( w 2 x + w 2 ) = w 2 n l = 0 w 2 1 b n x + ( 2 l + 1 ) 1 w 2 .
Equivalently, by (29), we have
b n ( w 2 x + w 2 ) = w 2 n 1 l = 0 w 2 1 b n x + ( 2 l + 1 ) 1 w 2 .
Similarly to (13), we observe that
2 l = 0 n 1 ( 1 ) l e ( 2 l + 1 ) t = k = 0 E k + E k ( 2 n ) t k k ! ,
where n N with n 1 (mod 2). Thus, by (31), we get
2 l = 0 n 1 ( 1 ) l ( 2 l + 1 ) k = E k + E K ( 2 n ) ,
where k N { 0 } and n N with n 1 (mod 2).
From (14), we easily note that
E n ( x ) = k = 0 n n k E k x n k , ( n 0 ) .
By (10), we get
Z p e ( 2 y + x + 1 ) t d μ 1 ( y ) = 2 e t + e t e x t = n = 0 E n ( x ) t n n ! .
Thus, we have
Z p ( 2 y + x + 1 ) n d μ 1 ( y ) = E n ( x ) , ( n 0 ) .
The next equation follows immediately from (10):
Z p e ( 2 y + 2 n + 1 ) t d μ 1 ( y ) + Z p e ( 2 x + 1 ) t d μ 1 ( x ) = 2 l = 0 n 1 e ( 2 l + 1 ) t ( 1 ) l ,
where n N with n 1 (mod 2).
Now, we let A k ( n ) = l = 0 n ( 1 ) l ( 2 l + 1 ) k , ( k N { 0 } ) . Here we note that A k ( n ) is the alternating kth power sums of consecutive odd positive integers. From (35), we have
Z p e ( 2 x + 2 n + 1 ) t d μ 1 ( x ) + Z p e ( 2 x + 1 ) t d μ 1 ( x ) = 2 Z p e ( 2 x + 1 ) t d μ 1 ( x ) Z p e 2 n x t d μ 1 ( x ) .
Let a , b be positive integers with a 1 (mod 2) and b 1 (mod 2). Then, by using the fermionic p-adic integral on Z p , we get
2 Z p e ( 2 x + 1 ) t d μ 1 ( x ) Z p e 2 a x t d μ 1 ( x ) = 2 l = 0 a 1 e ( 2 l + 1 ) t ( 1 ) l = k = 0 2 l = 0 a 1 ( 2 l + 1 ) k ( 1 ) l t k k ! = k = 0 2 A k ( a 1 ) t k k ! .
We now consider the next quotient of the fermionic p-adic integrals on Z p from which the identities of symmetry for the type 2 Euler polynomials follow:
J ( a , b ) = Z p Z p e ( 2 a x 1 + a + 2 b x 2 + b + a b x ) t d μ 1 ( x 1 ) d μ 1 ( x 2 ) Z p e 2 a b x t d μ 1 ( x ) .
From (38), we can derive the following equation given by
J ( a , b ) = 1 2 Z p e a ( 2 x 1 + 1 + b x ) t d μ 1 ( x 1 ) 2 Z p e ( 2 b x 2 + b ) t d μ 1 ( x 2 ) Z p e 2 a b x t d μ 1 ( x ) = 1 2 k = 0 E k ( b x ) a k t k k ! 2 l = 0 A l ( a 1 ) b l t l l ! = n = 0 k = 0 n n k E k ( b x ) A n k ( a 1 ) a k b n k t n n ! .
We note from (38) that J ( a , b ) = J ( b , a ) . Interchanging a and b, we get
J ( b , a ) = n = 0 k = 0 n n k E k ( a x ) A n k ( b 1 ) b k a n k t n n ! .
The following theorem is an immediate consequence of (39) and (40).
Theorem 3.
For n 0 , a , b N with a 1 (mod 2) and b 1 (mod 2), we have
k = 0 n n k E k ( b x ) A n k ( a 1 ) a k b n k = k = 0 n n k E k ( a x ) A n k ( b 1 ) b k a n k .
The next corollary is now obtained by setting x = 0 in Theorem 3.
Corollary 3.
For n 0 , a , b N , with a 1 (mod 2) and b 1 (mod 2), we have
k = 0 n n k E k A n k ( a 1 ) a k b n k = k = 0 n n k E k A n k ( b 1 ) b k a n k .
Taking b = 1 in Corollary 3 gives us the following identities.
Corollary 4.
For n 0 , a N with a 1 (mod 2), we have
E n ( a ) = k = 0 n n k E k A n k ( a 1 ) a k = k = 0 n n k E k a k l = 0 a 1 ( 1 ) l ( 2 l + 1 ) n k .
From (38), we have
J ( a , b ) = e a b x t 2 Z p e ( 2 a x 1 + a ) t d μ 1 ( x 1 ) 2 Z p e ( 2 b x 2 + b ) t d μ 1 ( x 2 ) Z p e 2 a b x t d μ 1 ( x ) = e a b x t 2 Z p e ( 2 a x 1 + a ) t d μ 1 ( x 1 ) 2 l = 0 a 1 ( 1 ) l e ( 2 l + 1 ) b t = l = 0 a 1 ( 1 ) l Z p e ( 2 x 1 + 1 + b x + ( 2 l + 1 ) b a ) a t d μ 1 ( x 1 ) = n = 0 a n l = 0 a 1 ( 1 ) l E n ( b x + ( 2 l + 1 ) b a ) t n n ! ,
where a , b N with a 1 (mod 2) and b 1 (mod 2). Interchanging a and b, we get
J ( b , a ) = n = 0 b n l = 0 b 1 ( 1 ) l E n ( a x + ( 2 l + 1 ) a b ) t n n ! .
As J ( a , b ) = J ( b , a ) , by (41) and (42), we obtain the following theorem.
Theorem 4.
For n 0 , a , b N with a 1 (mod 2) and b 1 (mod 2), we have
a n l = 0 a 1 ( 1 ) l E n ( b x + ( 2 l + 1 ) b a ) = b n l = 0 b 1 ( 1 ) l E n ( a x + ( 2 l + 1 ) a b ) .
Let us take a = 1 in Theorem 4. Then, we have
E n ( b x + b ) = b n l = 0 b 1 ( 1 ) l E n ( x + ( 2 l + 1 ) 1 b ) .
Example 2.
Here, we illustrate Theorem 2 in the case of n = 2 , a = 7 , and b = 3 . First, we note that E 2 ( x ) = x 2 1 . This follows from E 2 * ( x ) = x 2 x and the relation E n ( x ) = 2 n E n * ( x + 1 2 ) that can be deduced from (11) and (14). Here, we need to show that
l = 0 6 ( 1 ) l 3 x + 3 7 ( 2 l + 1 ) 2 1 = 3 7 2 l = 0 2 ( 1 ) l 7 x + 7 3 ( 2 l + 1 ) 2 1 .
Indeed, we can easily check that both the left- and right-hand side of (43) are equal to 9 x 2 + 18 x + 824 49 .

3. Further Remarks

For s C , the Riemann zeta function is defined by
ζ ( s ) = n = 1 1 n s , ( R e ( s ) > 1 ) ,
(see [14,15,16]).
It is well known that
ζ ( 2 n ) = ( 1 ) n 1 2 2 n 1 ( 2 n ) ! π 2 n B 2 n , ( n 0 ) ,
(see [14,16]).
By (44), we get
z cot ( z ) = z cos ( z ) sin ( z ) = z e i z + e i z 2 e i z e i z 2 i , ( i = 1 ) = i z 1 + 2 e 2 i z 1 = i z + k = 0 B k ( 2 i z ) k k ! = 1 + k = 1 B 2 k ( 2 k ) ! 2 2 k i 2 k z 2 k = 1 2 k = 1 ζ ( 2 k ) π 2 k z 2 k = 1 2 n = 1 k = 1 z 2 k ( n π ) 2 k = 1 2 n = 1 z n π 2 1 z n π 2 1 .
Thus, by (45), we get
cot ( z ) 1 z = n = 1 2 z ( n π ) 2 1 z n π 2 1 .
From (39), we easily note that
d d z log ( sin ( z ) ) log ( z ) = n = 1 d d z log 1 z n π 2 .
By (47), we easily get
sin ( z ) z = n = 1 1 z n π 2 .
It is not difficult to show that
z cot ( z ) 2 z cot ( 2 z ) = z tan ( z ) .
From (45) and (49), we have
z tan ( z ) = z cot ( z ) 2 z cot ( 2 z ) = 2 n = 1 2 z n π 2 1 2 z n π 2 1 2 n = 1 z n π 2 1 z n π 2 1 .
By (50), we get
d d z log ( cos ( z ) ) = n = 1 d d z log 1 4 z 2 ( n π ) 2 + n = 1 d d z log 1 z n π 2 .
Thus, from (51), we have
sec ( z ) = n = 1 1 z n π 2 1 2 z n π 2 = n = 1 1 2 z ( 2 n 1 ) π 2 1 ,
which is equivalent to
cos ( z ) = n = 1 1 2 z ( 2 n 1 ) π 2 .
A random variable has the Laplace distribution with positive parameter μ and b if its probability density function is
f ( x | μ , b ) = 1 2 b exp | x μ | b ,
(see [17]).
The shorthand notation X Laplace( μ , b ) is used to indicate that the random variable X has the Laplace distribution with positive parameters μ and b. If μ = 0 and b = 1 , the positive half-time is exactly an exponential scaled by 1 2 .
We assume that the independent random variables X 1 , X 2 , X 3 , have the Laplace distribution with parameters 0 and 1, (i.e., X k Laplace( 0 , 1 ), k N ). Let us put
Y = k = 1 X k ( 2 k 1 ) π .
Then, the characteristic function of Y is given by
n = 0 E [ Y n ] ( 2 i t ) n n ! = E n = 0 Y n ( 2 i t ) n n ! = E [ e 2 i Y t ] = E e ( k = 1 X k ( 2 k 1 ) π ) 2 i t = k = 1 E e X k ( 2 k 1 ) π 2 i t .
Now, we observe that
E e X k ( 2 k 1 ) π 2 i t = 1 2 e 2 i t ( 2 k 1 ) π x e | x | d x = 1 2 0 e 2 i t ( 2 k 1 ) π x e x d x + 1 2 0 e 2 i t ( 2 k 1 ) π x e x d x = 1 2 1 1 + 2 i t ( 2 k 1 ) π + 1 2 1 1 2 i t ( 2 k 1 ) π = 1 + 2 t ( 2 k 1 ) π 2 1 .
By (53), (56) and (57), we get
n = 0 E [ Y n ] ( 2 i t ) n n ! = k = 1 E e X k ( 2 k 1 ) π 2 i t = k = 1 1 + 2 t ( 2 k 1 ) π 2 1 = 2 e t + e t = n = 0 E n t n n ! .
Therefore, by comparing the coefficients on both sides of (58), we get
2 n i n E [ Y n ] = E n , ( n 0 ) .
Now, we assume that
Z = k = 1 X k 2 k π .
Then, the characteristic function of Z is given by
n = 0 E [ Z n ] ( i t ) n n ! = E n = 0 Z n ( i t ) n n ! = E [ e Z i t ] = E e k = 1 X k 2 k π i t = k = 1 E e X k 2 k π i t .
Now, we note that
E e X k 2 k π i t = 1 2 e i t 2 k π x e | x | d x = 1 2 0 e i t 2 k π x e x d x + 1 2 0 e i t 2 k π x e x d x = 1 2 1 1 + i t 2 k π + 1 2 1 1 i t 2 k π = 1 1 + t k π 2 .
From (61) and (62), we have
n = 0 E [ Z n ] ( i t ) n n ! = k = 1 E e X k 2 k π i t = k = 1 1 + t 2 k π 2 1 .
On the other hand, by (48), we get
n = 1 1 + t n π 2 1 = i t sin ( i t ) = 2 t e t e t .
By replacing t by t 2 , we have
n = 1 1 + t 2 n π 2 1 = t e t 2 e t 2 = n = 0 1 2 n 1 b n t n n ! .
Therefore, by (63) and (65), we obtain the following equation
i n E [ Z n ] = 1 2 n 1 b n , ( n 0 ) .

4. Conclusions

In this paper, we obtained several identities of symmetry for the type 2 Bernoulli and Euler polynomials (see Theorems 1–4). Indeed, they are symmetric identities involving type 2 Bernoulli polynomials and power sums of consecutive odd positive integers, and the ones involving type 2 Euler polynomials and alternating power sums of odd positive integers. For the derivation of those identities, we introduced certain quotients of bosonic p-adic and fermionic p-adic integrals on Z p , which have built-in symmetries. We note that this idea of using certain quotients of p-adic integrals has produced abundant symmetric identities (see [5,7,8,18,19,20,21] and references therein).
We emphasize here that, even though there have been many results on symmetric identities relating to some special numbers and polynomials, this paper is the first one that deals with symmetric identities involving type 2 Bernoulli polynomials, type 2 Euler polynomials, power sums of odd positive integers and alternating power sums of odd positive integers.
In [22,23], we derived some identities involving special numbers and moments of random variables by using the generating functions of the moments of certain random variables. The related special numbers are Stirling numbers of the first and second kinds, degenerate Stirling numbers of the first and second kinds, derangement numbers, higher-order Bernoulli numbers and Bernoulli numbers of the second kind.
In this paper, we considered two random variables created from random variables having Laplace distributions and showed that their moments are closely connected with the type 2 Bernoulli and Euler numbers. Again, this is the first paper that interprets the type 2 Bernoulli and Euler numbers as the moments of certain random variables.

Author Contributions

Conceptualization, T.K.; Formal analysis, D.S.K. and T.K.; Funding acquisition, D.K.; Investigation, D.S.K., H.Y.K., D.K. and T.K.; Methodology, D.S.K. and T.K.; Project administration, D.K. and T.K.; Supervision, D.S.K. and T.K.; Validation, H.Y.K. and D.K.; Writing—original draft, T.K.; Writing—review and editing, D.S.K., H.Y.K. and D.K.

Funding

This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2019R1C1C1003869).

Conflicts of Interest

The authors declare no conflict of interest.

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MDPI and ACS Style

Kim, D.S.; Kim, H.Y.; Kim, D.; Kim, T. Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials. Symmetry 2019, 11, 613. https://doi.org/10.3390/sym11050613

AMA Style

Kim DS, Kim HY, Kim D, Kim T. Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials. Symmetry. 2019; 11(5):613. https://doi.org/10.3390/sym11050613

Chicago/Turabian Style

Kim, Dae San, Han Young Kim, Dojin Kim, and Taekyun Kim. 2019. "Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials" Symmetry 11, no. 5: 613. https://doi.org/10.3390/sym11050613

APA Style

Kim, D. S., Kim, H. Y., Kim, D., & Kim, T. (2019). Identities of Symmetry for Type 2 Bernoulli and Euler Polynomials. Symmetry, 11(5), 613. https://doi.org/10.3390/sym11050613

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