1. Introduction
Many mathematicians have studied in the area of the Bernoulli numbers and polynomials, Euler numbers and polynomials, Genocchi numbers and polynomials, and tangent numbers and polynomials. The class of Appell polynomial sequences is one of the important classes of polynomial sequences. The Appell polynomial sequences arise in numerous problems of applied mathematics, mathematical physics and several other mathematical branches (see [
1,
2,
3,
4,
5,
6,
7,
8,
9,
10,
11,
12,
13,
14]). The Appell polynomials can be defined by considering the following generating function:
where
Alternatively, the sequence
is Appell sequence for
if and only if
where
Differentiating generating Equation (
1) with respect to
x and equating coefficients of
, we have
The typical examples of Appell polynomials are the Bernoulli and Euler polynomials (see [
1,
2,
3,
4,
5,
6,
7,
8,
9,
10,
11,
12,
13,
14]). It is well known that the Bernoulli polynomials are defined by the generating function to be
When
are called the Bernoulli numbers. The Euler polynomials are given by the generating function to be
When are called the Euler numbers.
The Bernoulli polynomials
of order
r are defined by the following generating function
The Frobenius–Euler polynomials of order
denoted by
are defined as
The values at are called Frobenius–Euler numbers of order r; when the polynomials or numbers are called ordinary Frobenius–Euler polynomials or numbers.
In this paper, we study some special polynomials which are related to Euler and Bernoulli polynomials. In addition, we give some identities for these polynomials. Finally, we investigate the zeros of these polynomials by using the computer.
2. Cosine–Bernoulli, Sine–Bernoulli, Cosine–Euler and Sine–Euler Polynomials
In this section, we define the cosine–Bernoulli, sine–Bernoulli, cosine–Euler and sine–Euler polynomials. Now, we consider the Euler polynomials that are given by the generating function to be
On the other hand, we observe that
From Equations (6) and (7), we have
and
Thus, by (8) and (9), we can derive
and
It follows that we define the following cosine–Euler polynomials and sine–Euler polynomials.
Definition 1. The cosine–Euler polynomials and sine–Euler polynomials are defined by means of the generating functionsandrespectively. Note that
. The cosine–Euler and sine–Euler polynomials can be determined explicitly. A few of them are
and
Clearly, we can get the following explicit representations of
Then, by Taylor expansions of
and
, we get
and
where
denotes taking the integer part. By (14)–(16), we get
and
The two polynomials can be determined explicitly. A few of them are
and
Therefore, we obtain the following theorem:
Therefore, we obtain the following theorem:
Therefore, we obtain the following theorem:
By comparing the coefficients on the both sides, we get
Therefore, we obtain the following theorem:
From (14) and (15), we have
Therefore, by Theorem 4 and (23), we obtain the following corollary:
Therefore, by comparing the coefficients on the both sides, we obtain the following theorem:
Theorem 5. For , we haveand Taking in Theorem 5, we obtain the following corollary:
From Corollary 2, we note that
and
Comparing the coefficients on the both sides of (27), we have
Similarly, for
, we have
Now, we consider the Bernoulli polynomials that are given by the generating function to be
Thus, by (28) and (29), we can derive
and
It follows that we define the following cosine–Bernoulli and sine–Bernoulli polynomials.
Definition 2. The cosine–Bernoulli polynomials and sine–Bernoulli polynomials are defined by means of the generating functionsand respectively.
By (30), (31), (32), and (33), we have
Note that
are the Bernoulli polynomials. The cosine–Bernoulli and sine–Bernoulli polynomials can be determined explicitly. A few of them are
and
Comparing the coefficients on the both sides of (34), we obtain the following theorem:
By replacing
x by
in (32), we get
Therefore, we obtain the following theorem:
Therefore, by (37), we obtain the following theorem:
Now, we define the new type polynomials that are given by the generating functions to be
and
respectively.
Note that
,
,
. The new type polynomials can be determined explicitly. A few of them are
and
From (38) and (39), we derive the following equations:
and
From (12), (13), (38) and (39), we derive the following theorem:
Now, we define the new type polynomials that are given by the generating functions to be
and
respectively.
Note that
,
,
. The new type polynomials can be determined explicitly. A few of them are
and
From (44) and (45), we derive the following equations:
and
From (32), (33), (44) and (45), we derive the following theorem:
We remember that the classical Stirling numbers of the first kind
and
are defined by the relations (see [
12])
respectively. Here,
denotes the falling factorial polynomial of order
n. The numbers
also admit a representation in terms of a generating function
By (12), (51) and by using Cauchy product, we get
where
with
.
By comparing the coefficients on both sides of (52), we have the following theorem:
By (12), (38), (50), (51) and by using Cauchy product, we have
By comparing the coefficients on both sides of (53), we have the following theorem:
By (4), (12), (38), (50), (51) and by using Cauchy product, we have
By comparing the coefficients on both sides, we have the following theorem:
Theorem 13. For and , we have By (5), (12), (38), (50), (51) and by using the Cauchy product, we get
By comparing the coefficients on both sides, we have the following theorem:
Theorem 14. For and , we have By Theorems 12–14, we have the following corollary.
Corollary 3. For and , we have 3. Distribution of Zeros of the Cosine–Euler and Sine–Euler Polynomials
This section aims to demonstrate the benefit of using numerical investigation to support theoretical prediction and to discover a new interesting pattern of the zeros of the cosine–Euler and sine–Euler polynomials. Using a computer, a realistic study for the cosine–Euler polynomials
and sine–Euler polynomials
is very interesting. It is the aim of this paper to observe an interesting phenomenon of “scattering” of the zeros of the the cosine–Euler polynomials
and sine–Euler polynomials
in a complex plane. We investigate the beautiful zeros of the cosine–Euler and sine–Euler polynomials by using a computer. We plot the zeros of the cosine–Euler polynomials
(
Figure 1).
In
Figure 1 (top-left), we choose
and
. In
Figure 1 (top-right), we choose
and
. In
Figure 1 (bottom-left), we choose
and
. In
Figure 1 (bottom-right), we choose
and
.
We plot the zeros of the sine–Euler polynomials
(
Figure 2).
In
Figure 2 (top-left), we choose
and
. In
Figure 2 (top-right), we choose
and
. In
Figure 2 (bottom-left), we choose
and
. In
Figure 2 (bottom-right), we choose
and
.
We observe that
has
reflection symmetry in addition to the usual
reflection symmetry analytic complex functions, where
(
Figure 1 and
Figure 2).
Hence, we have the following theorem:
Theorem 15. If , then If , then Our numerical results for numbers of real and complex zeros of the cosine–Euler polynomials
are displayed (
Table 1).
Our numerical results for numbers of real and complex zeros of the sine–Euler polynomials
are displayed (
Table 2).
Stacks of zeros of the cosine–Euler polynomials
for
from a 3D structure are presented (
Figure 3).
In
Figure 3 (left), we choose
. In
Figure 3 (right), we choose
. The plot of real zeros of the cosine–Euler polynomials
for
structure are presented (
Figure 4).
In
Figure 4 (left), we choose
. In
Figure 4 (right), we choose
. Stacks of zeros of the sine–Euler polynomials
for
from a 3D structure are presented (
Figure 5).
In
Figure 5 (left), we choose
. In
Figure 3 (right), we choose
. The plot of real zeros of the sine–Euler polynomials
for
structure are presented (
Figure 6).
We observe a remarkable regular structure of the complex roots of the cosine–Euler polynomials
. We also hope to verify a remarkable regular structure of the complex roots of the cosine–Euler polynomials
. Next, we calculated an approximate solution satisfying
. The results are given in
Table 3.
Next, we calculated an approximate solution satisfying
. The results are given in
Table 4.