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Article

Series of Floor and Ceiling Functions—Part II: Infinite Series

1
School of Liberal Studies, Pandit Deendayal Energy University, Gandhinagar 382426, India
2
Department of Mathematics, School of Technology, Pandit Deendayal Energy University, Gandhinagar 382426, India
3
Faculty of Economics and Administrative Sciences, Universidad Católica de la Santísima Concepción, Concepción 4090541, Chile
4
Department of Economics and Administrative, Universidad Autónoma de Occidente, Culiacan 80139, Mexico
*
Author to whom correspondence should be addressed.
Mathematics 2022, 10(9), 1566; https://doi.org/10.3390/math10091566
Submission received: 12 April 2022 / Revised: 27 April 2022 / Accepted: 29 April 2022 / Published: 6 May 2022

Abstract

:
In this part of a series of two papers, we extend the theorems discussed in Part I for infinite series. We then use these theorems to develop distinct novel results involving the Hurwitz zeta function, Riemann zeta function, polylogarithms and Fibonacci numbers. In continuation, we obtain some zeros of the newly developed zeta functions and explain their behaviour using plots in complex plane. Furthermore, we provide particular cases for the theorems and corollaries that show that our results generalise the currently available functions and series such as the Riemann zeta function and the geometric series. Finally, we provide four miscellaneous examples to showcase the vast scope of the developed theorems and showcase that these two theorems can provide hundreds of new results and thus can potentially create an entirely new field under the realm of number theory and analysis.

1. Introduction

In the year 1650, Pietro Mengoli posed a mathematical problem, which is now known as the Basel Problem. Its solution was achieved nearly 85 years later, in 1735 by Leonard Euler [1], who used Taylor’s series of sine functions in an ingenious way and then generalised the formula for all real powers greater than 1. The approach, however, to implementing a fundamental theorem of algebra (which is for finite zeros) on an infinite polynomial (with infinite zeros) was based on Euler’s intuition and remained unproved for another century, when in the early 1800s, Wierstrass gave a validation of Euler’s work using the so-called Weierstrass factorisation theorem. Following these findings, in 1859, nearly two centuries after Mengoli’s work, Bernard Riemann extended the formula defined by Euler to the domain of complex numbers with the motivation to find a relation between zeros of the function and the distribution of prime numbers.
The slow progress in the development of this field over the first two centuries suddenly surged after Riemann’s study displayed the (zeta) function’s relation with the prime counting function. Over the next two centuries, researchers discovered that not only is the zeta function crucial in understanding the distribution of prime numbers but also the function and its generalisations have many direct or indirect applications in many advanced fields such as cryptography (applications of prime number theory), cosmology [2], quantum field theory [3,4] and string theory [5].
Due to such impactful applications, researchers have studied different infinite series and zeta functions in depth [6,7,8,9,10] over the past few decades. Coffey [6] obtained a faster convergent series representation of the Hurwitz zeta function, whereas Kanemitus et al. [7] provided integral representations and gave proofs of certain available results, including the Ramanujan formula. Vepštas [8] provided a technique to obtain faster convergence of oscillatory sequences and applied them to Hurwitz zeta functions and polylogarithms. Nisar [9] generalised the Hurwitz–Lerch zeta function of two variables. Riguidel [10] utilised the computational approach to propose the morphogenic interpretation of Riemann zeta function.
Moreover, as we showcased in Part I [11], the floor–ceiling and ceiling–floor theorems allow researchers to derive, study and analyse new results, and corresponding novel real-life applications can be found with the emergence of such results.
Hence, continuing the study in a similar direction, in this part, we attempted to generalise different infinite series and zeta functions (such as geometric series, Hurwitz zeta function, and polylogarithms) using the theorems developed in Part I [11].

Outline of the Article

Section 2 contains the preliminary results that are utilised in our study. Section 3 provides the cases for n for the floor–ceiling theorem and the ceiling–floor theorem of Part I [11]. These cases provide foundations for the results obtained in Section 4, Section 5 and Section 6. Section 7 specifically presents the corollaries of the results proved in the previous three sections. In Section 8, some of the zeros of newly developed zeta functions are given and their behaviours are discussed in a bounded interval using domain colouring. Section 9 gives the results on particular values. Section 10 provides some miscellaneous results. Section 11 discusses the scope for further studies, and finally, Section 12 concludes the work conducted in this pair of articles.

2. Preliminaries

The following results and definitions are useful for our study:

2.1. Hurwitz Zeta Function

The Hurwitz zeta function [3] ζ s , t is a function of complex variables s and t defined as an infinite sum:
ζ s , t = n = 0 1 n + t s = 1 Γ s 0 x s 1 e t x 1 e x d x , w h e r e Γ s = 0 x s 1 e x d x .
The series is absolutely convergent for all complex values of s and t when R e s > 1 and y C \ Z .

2.2. Polylogarithm

The polylogarithm function [12] is an infinite series of the following form:
L i s ( z ) = n = 1 z n n s ,
where z < 1 , y C \ Z 0 , ( s ) > 0 .

2.3. Riemann Zeta Function

The Riemann zeta function [5] ζ s is a function of the complex variable s defined as an infinite sum:
ζ s = n = 1 1 n s = 1 Γ s 0 x s 1 e x 1 d x , w h e r e Γ s = 0 t s 1 e t d t .
The function converges for all complex values of s when R e s > 1 and is defined as
ζ s = 1 1 s + 1 2 s + 1 3 s + .

2.4. Fibonacci Numbers and Reciprocal Fibonacci Constant

The nth Fibonacci number [13] is given by the following formula:
F n = φ n ( φ ) n 5 w h e r e φ = 1 + 5 2 .
Furthermore, a series of reciprocals of all Fibonacci numbers gives a constant (irrational) value:
n = 1 1 F n = 3.35988566243 ,
where 3.35988566243 is the reciprocal Fibonacci constant.

2.5. Floor and Ceiling Functions

The floor function [14] of any real number x (denoted by x ) gives the greatest integer not greater than x, i.e., x = m a x { w Z w x } . For example, 1.4 = 1 , 2 = 2 , 3.4 = 4 and 2 = 2 .
The ceiling function [14] (denoted by x ) similarly gives the smallest integer not smaller than x, i.e., x = min { k Z k x } . For example, 1.4 = 2 , 2 = 2 , 3.4 = 3 and 2 = 2 .
From the above, we can see that x = x = x if and only if x Z .

3. Foundations

3.1. Floor–Ceiling Theorem

Theorem 1.
Let a , b R + , m Z , and let k n be any sequence and let corresponding series n = 1 k ( b n ) a + m be convergent; then, the following equalities hold true.
n = 1 k ( b n ) a + m = n = 1 ( n + 1 ) 1 a b n 1 a b k n + m ,
or alternatively,
n = 1 k ( b n ) a + m = n = 1 ( k n 1 + m k n + m ) n 1 a b 1 b k m .
Proof. 
We have ([11], Section 3, Equation (12))
i = 1 n k ( b i ) a + m = t = 1 ( b n ) a ( t + 1 ) 1 a b t 1 a b k t + m ( ( b n ) a ) 1 a b n k ( b n ) a + m .
Now, the following observation can be easily made:
( ( b n ) a ) 1 a b n a s n lim n ( ( b n ) a ) 1 a b n = 0 .
Hence, by applying limit n , the previous equation reduces to Equation (5).
Furthermore, consider the right-hand side of Equation (5):
n = 1 ( n + 1 ) 1 a b n 1 a b k n + m = n = 1 ( n + 1 ) 1 a b k n + m n = 1 n 1 a b k n + m = n = 2 n 1 a b k n 1 + m n = 1 n 1 a b k n + m = n = 1 n 1 a b k n 1 + m 1 b k m n = 1 n 1 a b k n + m
which is the right-hand side of Equation (6). □

3.2. Ceiling–Floor Theorem

Theorem 2.
Let a , b R + , m Z , let k n be any sequence and let corresponding series n = 1 k ( b n ) a + m be convergent; then, the following equalities hold true.
n = 1 k ( b n ) a + m = n = 1 n 1 a b ( n 1 ) 1 a b k n + m ,
or alternatively,
n = 1 k ( b n ) a + m = n = 1 ( k n + m k n + 1 + m ) n 1 a b .
Proof. 
We have ([11], Section 3, Equation (16))
i = 1 n k ( b i ) a + m = t = 1 ( b n ) a t 1 a b ( t 1 ) 1 a b k t + m ( ( b n ) a ) 1 a b n k ( b n ) a + m .
Now, the following observation can be easily made:
( ( b n ) a ) 1 a b n a s n lim n ( ( b n ) a ) 1 a b n = 0 .
Hence, by applying limit n , the previous equation reduces to Equation (7).
Furthermore, consider the right-hand side of Equation (7):
n = 1 n 1 a b ( n 1 ) 1 a b k n + m = n = 1 n 1 a b k n + m n = 1 ( n 1 ) 1 a b k n + m = n = 1 n 1 a b k n + m n = 0 n 1 a b k n + 1 + m = n = 1 n 1 a b k n + m n = 1 n 1 a b k n + 1 + m
which is the right-hand side of Equation (8). □

4. ‘F’ and ‘C’ Generalised Functions

4.1. Definitions

In order to avoid misunderstanding our new results with the available definitions, we assign ’F’ or ’C’ (representing use of floor and ceiling functions, respectively) prefixes to all of the available definitions.
For example, the F-Hurwitz zeta function can be defined as the following equation:
F ζ b a ( s , t ) = n = 0 1 ( b n ) a + t s ,
whereas the C-Riemann zeta function is defined as the following equation:
C ζ b a ( s ) = n = 1 1 ( b n ) a s .
Using the same analogy, the C-Hurwitz zeta function, F-polylogarithm, C-polylogarithm and F-Riemann zeta function can also be defined.
Furthermore, by implementing floor and ceiling functions, any available infinite series can be generalised as ‘F’ or ‘C’ series (i.e., For Lerch zeta function, the corresponding F-Lerch and C-Lerch zeta functions can be defined).

4.2. Theorems

For each ‘F’ and ‘C’ generalised series, a corresponding theorem can be provided and proved, which relate them to an equivalent series (which is due to Theorem 1 or Theorem 2).
Take the F-Hurwitz zeta function and the C-polylogarithm for example:
Theorem 3. (F-Hurwitz Zeta Function)
The series has an equivalent form, given below:
F ζ b a ( s , t ) = n = 0 1 ( b n ) a + t s = n = 1 ( n + 1 ) 1 a b n 1 a b n + t s .
Proof. 
Equation (9) can be obtained by substituting m = 0 and k n = 1 ( n + t ) s in Equation (5). □
Theorem 4. (C-Polylogarithm)
The series has an equivalent form, given below:
C L i s b a ( z ) = n = 1 z ( b n ) a ( b n ) a s = n = 1 n 1 a b ( n 1 ) 1 a b z n n s .
Proof. 
Equation (10) can be obtained by substituting m = 0 and k n = z n n s in Equation (7). □
Remark 1.
Every series or function available in the literature can be generalised using the same analogy. However, to avoid repetition, we have provided just a couple of examples to depict the scope of Theorems 1 and 2 (the general rule for the notation is F G b a ( X ) and C G b a ( X ) for ‘F’ and ‘C’ generalised functions, respectively, where G ( X ) is the notation for the regular definition of the same function).

5. Generalised Geometric Series

5.1. Floor Geometric Series

Theorem 5.
Let x C , a , b R + , n N and z x < 1 , then the following equation holds true.
n = 1 z ( b n ) a x = ( z x 1 ) n = 1 z n x n 1 a b 1 b .
Proof. 
Substituting m = 0 and k n = z n · x in Equation (6), we have
n = 1 z ( b n ) a x = n = 1 z ( n 1 ) x z n x n 1 a b 1 b .
Furthermore, with basic manipulations, we arrive at Equation (11). □

5.2. Ceiling Geometric Series

Theorem 6.
Let x C , a , b R + , n N and z x < 1 ; then, following equation holds true.
n = 1 z ( b n ) a x = ( 1 z x ) n = 1 z n x n 1 a b .
Proof. 
Substituting m = 0 and k n = z n · x in Equation (8), we have
n = 1 z ( b n ) a x = n = 1 z n x z ( n + 1 ) x n 1 a b .
Furthermore, with basic manipulations, we arrive at Equation (12). □

6. Generalised Reciprocal Fibonacci Series

6.1. Shah–Pingala Function

Definition 1.
For q Z \ Z ( N { 0 } ) , we define the Shah–Pingala function using the following equation:
S ( q ) = n = 1 n q F n ,
where F n is the nth Fibonacci number (Section 2.4).
The reciprocal Fibonacci constant is a special case of the new definition for q = 0 ( S ( 0 ) = 3.35988566243 ) .
Theorem 7.
Shah–Pingala function S ( q ) converges for all q Z \ Z .
Proof. 
The nth term is n q F n . We know that
F n > 2 φ 5 n ( F n ) 1 < 2 φ 5 n .
We also know that lim n n q z n = 0 for q R z > 1 . Hence,
0 lim n n q F n lim n n q 2 φ 5 n lim n n q F n = 0 .
Therefore, the necessary condition holds.
Furthermore, considering the ratio test for series convergence, we have
L = lim n a n + 1 a n = lim n ( n + 1 ) q F n + 1 n q F n = lim n 1 + 1 n q F n F n + 1 = 1 φ < 1 .
Since the limit L < 1 , the series converges. □

6.2. Floor Reciprocal Fibonacci Function

Theorem 8.
Let a , b R + , and let F n be Fibonacci sequence; then,
n = 1 1 F ( b n ) a = n = 1 ( n + 1 ) 1 a b n 1 a b F n .
Proof. 
Substituting m = 0 and k n = 1 F n in Equation (5), we obtain Equation (14). □

6.3. Ceiling Reciprocal Fibonacci Function

Theorem 9.
Let a , b R + , and let F n be Fibonacci sequence; then,
n = 1 1 F ( b n ) a = n = 1 n 1 a b ( n 1 ) 1 a b F n .
Proof. 
Substituting m = 0 and k n = 1 F n in Equation (7), we obtain Equation (15). □

7. Corollaries

7.1. Corollaries of ‘F’ and ‘C’ Generalised Functions

Corollary 1. (F-Shah–Hurwitz Zeta Function)
For the F-Shah–Hurwitz zeta function (a special case of the F-Hurwitz zeta function at a = 1 q , q N , b = 1 ) and the Hurwitz zeta function ζ ( s , t ) , the following equation holds true.
F ζ 1 1 q s , t = n = 0 1 n q + t s = m = 0 q 1 k = 0 m q m m k t m k ζ s k , t ,
or alternatively,
F ζ 1 1 q s , t = 0 P x , s , t , q e t x 1 e x d x ,
where
P x , s , t , q = m = 0 q 1 k = 0 m q m m k ( t ) m k Γ ( s k ) 1 x s k 1 .
Given the analytic continuation of the Hurwitz zeta function, we observe that F ζ 1 1 q ( s , t ) can be defined for R e s < q , and hence, F ζ 1 1 q s can be defined s C such that s 1 , 2 , , q .
Proof. 
From Section 4, we have
F ζ b a s , t = n = 0 1 ( b n ) a + t s = n = 0 ( n + 1 ) 1 a b n 1 a b ( n + t ) s .
Substituting a = 1 q and b = 1 , we obtain
F ζ 1 1 q s , t = n = 0 1 n q + t s = n = 0 ( n + 1 ) q n q ( n + t ) s .
Considering the right-hand side of the previous equation, we have
n = 0 ( n + 1 ) q n q ( n + t ) s = n = 0 m = 0 q 1 q m n m ( n + t ) s = n = 0 m = 0 q 1 q m ( n + t t ) m ( n + t ) s = n = 0 m = 0 q 1 q m k = 0 m m k ( n + t ) k ( t ) m k ( n + t ) s = m = 0 q 1 k = 0 m q m m k ( t ) m k n = 0 1 ( n + t ) s k = m = 0 q 1 k = 0 m q m m k t m k ζ s k , t .
Finally, the alternate (integral representation) form of the equation can be obtained by substituting ζ s k , t = Γ s k 1 0 x s k 1 e t x 1 e x d x (from Equation (1)). □
Corollary 2. (C-Shah–Hurwitz zeta function)
For the C-Shah–Hurwitz zeta function (a special case of the C-Hurwitz zeta function at a = 1 q , q N , b = 1 ) and the Hurwitz zeta function ζ ( s , t ) , the following equation holds true.
C ζ 1 1 q s , t = n = 0 1 n q + t s = m = 0 q 1 k = 0 m 1 q m + 1 q m m k t m k ζ s k , t ,
or alternatively,
C ζ 1 1 q s , t = 0 Q x , s , t , q e t x 1 e x d x ,
where
Q x , s , t , q = m = 0 q 1 k = 0 m 1 q m + 1 q m m k t m k Γ ( s k ) 1 x s k 1 .
Given the analytic continuation of the Hurwitz zeta function, we observe that F ζ 1 1 q ( s , t ) can be defined even for R e s < q , and hence, F ζ 1 1 q s can be defined s C such that s 1 , 2 , , q .
Proof. 
From Section 4, we have
C ζ b a s , t = n = 0 1 ( b n ) a + t s = n = 0 n 1 a b ( n 1 ) 1 a b ( n + t ) s .
Substituting a = 1 q and b = 1 , we have
C ζ 1 1 q s , t = n = 0 1 n q + t s = n = 0 n q ( n 1 ) q ( n + t ) s .
Consider the right-hand side of the previous equation:
n = 0 n q ( n 1 ) q ( n + t ) s = n = 0 m = 0 q 1 ( 1 ) q m + 1 q m n m ( n + t ) s = n = 0 m = 0 q 1 ( 1 ) q m + 1 q m ( n + t t ) m ( n + t ) s = n = 0 m = 0 q 1 ( 1 ) q m + 1 q m k = 0 m m k ( n + t ) k ( t ) m k ( n + t ) s = m = 0 q 1 k = 0 m ( 1 ) q m + 1 q m m k ( t ) m k n = 0 1 ( n + t ) s k = m = 0 q 1 k = 0 m ( 1 ) q m + 1 q m m k t m k ζ s k , t .
Finally, the alternate (integral representation) form of the equation can be obtained by substituting ζ s k , t = Γ s k 1 0 x s k 1 e t x 1 e x d x (from Equation (1)). □
Corollary 3. (F-Shah–Riemann Zeta Function)
For any a of the form a = 1 q , q N and b = 1 , the following equation holds true.
F ζ 1 1 q s , 1 = F ζ 1 1 q s = n = 1 1 n q s = m = 0 q 1 q m ζ s m ,
or alternatively,
F ζ 1 1 q s = 0 P x , s , q e x 1 d x . w h e r e P x , s , q = t = 0 q 1 Γ s t 1 q t x s t 1 .
Furthermore, given the analytic continuation of the Riemann zeta function, we observe that F ζ 1 1 q s can be defined for R e s < q , and hence, F ζ 1 1 q s can be defined s C such that s 1 , 2 , , q .
Proof. 
Equation (20) can be obtained by substituting t = 1 in Equation (16). Moreover, we may consider an integral representation of the Riemann zeta function from Equation (3) to obtain Equation (21). □
Corollary 4. (C-Shah–Riemann Zeta Function)
For any a of the form a = 1 q , q N and b = 1 , the following equation holds true.
C ζ 1 1 q s , 1 = C ζ 1 1 q s = n = 1 1 n q s = m = 0 q 1 1 q m + 1 q m ζ s m
or alternatively,
C ζ 1 1 q s = 0 Q x , s , q e x 1 d x ; w h e r e Q x , s , q = t = 0 q 1 1 q t + 1 Γ s t q t x s t 1 .
Again, given the analytic continuation of the Riemann zeta function, we observe that C ζ 1 1 q s can be defined even for R e s < q , and hence, C ζ 1 1 q s can be define s C such that s 1 , 2 , , q .
Proof. 
Equation (22) can be obtained by substituting t = 1 in Equation (18). Moreover, we may take an integral representation of the Riemann zeta function from Equation (3) to obtain Equation (23). □
Remark 2.
All of the series in Corollaries 1–4 have poles at s = 1 , 2 , , q , but the following can be simply observed for q 1 :
F ζ 1 1 q q , t C ζ 1 1 q q , t = m = 0 q 2 k = 0 m q m m k ζ q k , t t m k + 1 q m t m k
and
F ζ 1 1 q q C ζ 1 1 q q = n = 1 1 n q q 1 n q q = t = 0 q 2 q t ζ q t 1 + 1 q t .
This shows that, even if the set of two series may individually have poles at s = 1 , 2 , , q , their difference is convergent for s = q .
Remark 3.
The analogy used in Corollaries 1–4 can be implemented to different functions such as the Lerch zeta function.
F L 1 1 q ( λ , s , t ) = m = 0 q 1 k = 0 m q m m k t m k L λ , s k , t .

7.2. Corollaries of Generalised Geometric Series

Corollary 5.
For | z | < 1 , polylogarithm L i s ( z ) and any q N , the following equation holds true.
n = 1 z n q = ( z 1 1 ) L i q ( z ) 1 .
Proof. 
Equation (26) can be obtained by substituting x = b = 1 , a = 1 q , q N in Equation (11). □
Corollary 6.
For | z | < 1 , polylogarithm L i s ( z ) and any q N , the following equation holds true.
n = 1 z n q = ( 1 z ) L i q ( z ) .
Proof. 
Equation (27) can be obtained by substituting x = b = 1 , a = 1 q , q N in Equation (12). □

7.3. Corollaries of Generalised Reciprocal Fibonacci Series

Corollary 7.
Let F n be Fibonacci sequence, q Z \ Z , and let S ( q ) denote a Shah–Pingala function; then, the following equation holds true.
n = 1 1 F n q = n = 1 n q F n 2 i = 1 n 1 F i 2 = t = 0 q 1 q t S ( t ) .
Proof. 
Equation (28) can be obtained by substituting b = 1 , a = 1 q , q N in Equation (14). □
Corollary 8.
Let F n be Fibonacci sequence, q Z \ Z , and let S ( q ) denote the Shah–Pingala function; then, the following equation holds true.
n = 1 1 F n q = n = 1 n q F n 1 i = 1 n F i 2 = t = 0 q 1 1 q t + 1 q t S ( t ) .
Proof. 
Equation (29) can be obtained by substituting b = 1 , a = 1 q , q N in Equation (15). □

8. Plots and Zeros: F-Shah–Riemann Zeta and C-Shah–Riemann Zeta Functions

For this study, we consider all of the available zeros of Riemann zeta functions, i.e., the real zeros 2 n , n N and the known complex zeros on the critical strip σ + i · t , 0 < σ < 1 , t R , as trivial solutions (already available zeros). Keeping that in view, we consider the negative solutions and the solutions in which the imaginary parts are in the radius ( t 1 , t + 1 ) (imaginary part of solutions of the Riemann zeta function) as trivial for the new zeta functions. Moreover, positive real zeros and the solutions in which imaginary parts are not in the radius ( t 1 , t + 1 ) are considered non-trivial zeros. In all six of the plots, we focused on the behaviour of the functions near their non-trivial zeros.

8.1. Zeros of F-Shah–Riemann Zeta Function

In this subsection, utilising the right-hand side of the Equation (20), we obtain the solutions (given in Table 1) of the F-Shah–Riemann zeta function. Furthermore, we give three Figure 1, Figure 2 and Figure 3, and they are plotted in the intervals of the non-trivial (positive real) zeros and the poles of F-Shah–Riemann zeta function for q = 2 , q = 3 , and q = 4 , respectively.
The function has q poles, q 1 positive real zeros (non-trivial zeros) and infinite negative real zeros (each zero corresponding to each negative even integer).
The complex zeros are achieved by implementing the Newton–Raphson method at point x 0 = 1 2 + i · t for different available values of t.

8.2. Zeros of C-Shah–Riemann Zeta Function

In this subsection, utilising the right-hand side of Equation (22), we obtain the solutions (given in Table 2) of the C-Shah–Riemann zeta function. Furthermore, we give three Figure 4, Figure 5 and Figure 6, and they are plotted in the intervals of the non-trivial (positive real) zeros and the poles of F-Shah–Riemann zeta function for q = 2 , q = 3 and q = 4 , respectively.
The function has q poles, ( q 1 ) pairs of non-trivial of complex zeros ( 2 ( q 1 ) zeros), which were observed in the plots. There are infinite real zeros (each zero corresponds to each negative even integer) with no non-trivial (positive) real zero.
The trivial complex zeros are achieved by implementing the Newton–Raphson method with an initial guess x 0 = 1 2 + i · t for different available values of t, whereas the non trivial complex zeros are obtained by considering an initial guess x 0 in the converging region of the plot (for example, we considered x 0 = 0.8 + 2 i for the C-Shah–Riemann zeta function for q = 2 ).

9. Results for Specific Values

9.1. Specific Values—‘F’ and ‘C’ Generalised Functions

For a = b = 1 , ‘F’ and ‘C’ generalised series reduce to the original series (consider the F-Hurwitz zeta function and C-Riemann zeta, for example).
F ζ 1 1 s , t = n = 0 1 1 · n 1 + t s = n = 0 1 n + t s = ζ s , t
C ζ 1 1 s = n = 0 1 1 · n 1 + 1 s = n = 1 1 n s = ζ s .

9.2. Specific Values—Generalised Geometric Series

Substituting a = b = x = 1 in Equation (11), we obtain
n = 1 z n = L i 0 ( z ) = ( z 1 1 ) L i 1 ( z ) 1 ,
or substituting a = b = x = 1 in Equation (12), we obtain
n = 1 z n = L i 0 ( z ) = ( 1 z ) L i 1 ( z )
both of which hold true.

9.3. Specific Values—Generalised Reciprocal Fibonacci Series

For a = b = 1 in Equations (14) and (15), we have S ( 0 ) 3.35988566243 .

10. Miscellaneous Results

Let the two functions be defined as F g b a ( n ) = ( n + 1 ) 1 a b n 1 a b and C g b a ( n ) = n 1 a b ( n 1 ) 1 a b , which yield the number of repetitions of ( b n ) a and ( b n ) a , respectively. Then for particular values of a and b, we provide the following assumptions (given in Table 3), which were made solely by intuitions and have been checked and verified to be true for different values (of n) using the Python programming language.
One can go further with 1 a = 4 , 5 , 6 , and different values of b for both functions. In general, our assumptions for 1 q , 2 are
(I)
For the number of repetitions of 2 n q
F g 2 1 q n = ( n + 1 ) q 2 n q 2 = q q 1 2 i = 1 n t = q 2 q 2 q 2 i t 1 + 1 q t 2 + y n ,
where
y n = 2 n 2 + 1 , q e v e n n 2 n 1 2 , q o d d
(II)
For the number of repetitions of 2 n q ,
C g 2 1 q n = n q 2 ( n 1 ) q 2 = q q 1 2 t = q 2 q 2 q 2 i = 1 n 1 i t 1 + 1 q t 2 + z n
where,
z n = 2 n 2 , q e v e n n 2 n 1 2 , q o d d
These assumptions have been verified for the values of q = 1 , 2 , 3 , 4 , 5 using the python programming language.
Remark 4.
If both of these assumptions hold true, then the following result holds:
ζ ( s ) = F ζ 2 1 q s C ζ 2 1 q s .

11. Open Problems

In this section, we propose the following open problems for future work.

11.1. Problem 1

Do Assumptions (30) and (31) hold true? Can the equality be proven for the general case?
If these assumptions hold true, one can go on to find a general formula for the equivalents of F g k 1 q s and C g k 1 q s .

11.2. Problem 2

For both ‘C’ and ‘F’ generalised series, the respective corresponding series on the right-hand side (the equivalent series) are observed to converge faster to the particular values; can it be proven mathematically?

11.3. Problem 3

Is it possible to obtain Euler-product formulae for the F-Shah–Riemann zeta function and the C-Shah–Riemann zeta function?

11.4. Problem 4

Can the floor–ceiling and ceiling–floor theorems be implemented on integrals?

11.5. Problem 5

Considering the vast number of available infinite series; studying, analysing and providing results for all of them is not possible in the scope of single article. Hence, we discuss just a few of the results that could be derived from the discussed theorems and corollaries.
Therefore, we put forth the final open problem of this series of papers for future studies to implement our results to different available infinite series (i.e., series involving (1) exponential function, (2) logarithmic function, (3) trigonometric functions, (4) different Dirichlet functions (Lerch zeta function and Dirichlet eta function), and (5) Taylor Series or any results involving infinite series).
To inspire future studies, we list a few examples for reference:
(1) For the the exponential function e z :
n = 0 z n n ! = ( 2 z + 1 ) e z ,
(2) For the polylogarithm L i s ( z ) :
n = 1 z n n s = 2 L i s 1 ( z ) + L i s ( z ) ,
(3) For Hyperbolic Functions:
n = 1 z ( 2 n + 1 ) ( 2 n + 1 ) ! = z cosh ( z ) ,
(4) For any function f ( x ) (using the Maclaurin series):
n = 0 f n ( 0 ) x n ( n ) ! = 2 x f ( x ) + f ( x ) .

12. Concluding Remarks

In this paper, we proved the floor–ceiling and ceiling–floor theorems (of Part I [11]) for infinite series and take them as a basis to provide new results involving zeta functions and Fibonacci numbers (in terms of theorems and corollaries). Furthermore, we provide some zeros of the newly derived zeta functions and plot them in a complex plane using the concept of domain colouring.
The floor–ceiling and ceiling–floor theorems can potentially develop an entire field in mathematics where, using them, one can derive hundreds, if not thousands, hitherto unknown results (such as the Shah–Pingala formula in Part I [11] or the Shah–Hurwitz and Shah–Riemann zeta functions in Part II) involving finite and infinite series. With the availability of those new results, one can further analyse their patterns and behaviour in domains of real and complex analyses and find their applications in different advanced fields, as shown earlier [2,3,4,5].

Author Contributions

Conceptualisation, D.S.; methodology, D.S.; validation, M.S., M.O.-L., E.L.-C. and R.S.; formal analysis, M.S., M.O.-L. and R.S.; writing—original draft preparation, D.S.; writing—review and editing, D.S., M.S. and E.L.-C.; supervision, M.S. and E.L.-C. All authors have read and agreed to the published version of the manuscript.

Funding

Author Leon-Castro acknowledges support from the Chilean Government through ANID InES Ciencia Abierta INCA210005.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. F-Shah–Riemann zeta function for q = 2 : F ζ 1 1 2 ( s ) . Two poles of the function are observed as s = 1 and s = 2 , whereas a positive real root can be observed at s 1.473414717168 .
Figure 1. F-Shah–Riemann zeta function for q = 2 : F ζ 1 1 2 ( s ) . Two poles of the function are observed as s = 1 and s = 2 , whereas a positive real root can be observed at s 1.473414717168 .
Mathematics 10 01566 g001
Figure 2. F-Shah–Riemann zeta function for q = 3 : F ζ 1 1 3 ( s ) . Three poles of the function are observed as s = 1 , s = 2 and s = 3 , whereas two positive real roots can be observed at s 1.34672733238 and s = 2.675764968478 .
Figure 2. F-Shah–Riemann zeta function for q = 3 : F ζ 1 1 3 ( s ) . Three poles of the function are observed as s = 1 , s = 2 and s = 3 , whereas two positive real roots can be observed at s 1.34672733238 and s = 2.675764968478 .
Mathematics 10 01566 g002
Figure 3. F-Shah–Riemann zeta function for q = 4 : F ζ 1 1 4 ( s ) . Four poles of the function are observed as s = 1 , s = 2 , s = 3 and s = 4 , whereas three positive real roots can be observed at s 1.271435903075 , s 2.551800083744 and s 3.796568180266 .
Figure 3. F-Shah–Riemann zeta function for q = 4 : F ζ 1 1 4 ( s ) . Four poles of the function are observed as s = 1 , s = 2 , s = 3 and s = 4 , whereas three positive real roots can be observed at s 1.271435903075 , s 2.551800083744 and s 3.796568180266 .
Mathematics 10 01566 g003
Figure 4. C-Shah–Riemann zeta function for q = 2 : C ζ 1 1 2 ( s ) . Two poles of the function are observed as s = 1 and s = 2 , whereas a pair of non-trivial complex roots can be observed at s 0.6078048160 ± 1.9350010902 i .
Figure 4. C-Shah–Riemann zeta function for q = 2 : C ζ 1 1 2 ( s ) . Two poles of the function are observed as s = 1 and s = 2 , whereas a pair of non-trivial complex roots can be observed at s 0.6078048160 ± 1.9350010902 i .
Mathematics 10 01566 g004
Figure 5. C-Shah–Riemann zeta function for q = 3 : C ζ 1 1 3 ( s ) . Three poles of the function are observed as s = 1 , s = 2 and s = 3 , whereas two pairs of non-trivial complex root can be observed at s 0.6997539191 ± 1.7534110356 i and s 2.2160159281 ± 2.0194666275 i .
Figure 5. C-Shah–Riemann zeta function for q = 3 : C ζ 1 1 3 ( s ) . Three poles of the function are observed as s = 1 , s = 2 and s = 3 , whereas two pairs of non-trivial complex root can be observed at s 0.6997539191 ± 1.7534110356 i and s 2.2160159281 ± 2.0194666275 i .
Mathematics 10 01566 g005
Figure 6. C-Shah–Riemann zeta function for q = 4 : C ζ 1 1 4 ( s ) . Four poles of the function are observed as s = 1 , s = 2 , s = 3 and s = 4 , whereas three pairs of non-trivial complex root can be observed at s 1.4515176098 ± 1.2122471911 i , s 0.8794024170 ± 2.3478232248 i and s 3.5554537875 ± 1.9983004535 i .
Figure 6. C-Shah–Riemann zeta function for q = 4 : C ζ 1 1 4 ( s ) . Four poles of the function are observed as s = 1 , s = 2 , s = 3 and s = 4 , whereas three pairs of non-trivial complex root can be observed at s 1.4515176098 ± 1.2122471911 i , s 0.8794024170 ± 2.3478232248 i and s 3.5554537875 ± 1.9983004535 i .
Mathematics 10 01566 g006
Table 1. All of the positive (non-trivial) real zeros and some of the complex and negative (trivial) real zeros of F-Shah–Riemann zeta function for values of q = 2, q = 3 and q = 4 up to 12 decimal places.
Table 1. All of the positive (non-trivial) real zeros and some of the complex and negative (trivial) real zeros of F-Shah–Riemann zeta function for values of q = 2, q = 3 and q = 4 up to 12 decimal places.
Values of qComplex ZerosNon-Trivial Real ZerosTrivial Real Zeros
q = 21.247595281027 + 14.148570425918i1.473414717168−1.606882014624
1.279113135722 + 21.012442575688i-−3.4037619981310
q = 31.964049664859 + 14.165353520342i1.346727332380−1.346011820212
2.032696553488 + 21.001910485581i2.675764968478−2.878069065724
2.062342325067 + 25.053176875792i-−4.623564926958
q = 42.653604262294 + 14.184700388061i1.271435903075−1.192688707675
2.763852133144 + 20.991263644295i2.551800083744−2.423972912304
2.811381226897 + 25.077915228667i3.796568180266−3.975616047809
2.852031019544 + 30.316385253077i-−5.736688777159
Table 2. Some of the non-trivial and trivial complex and real zeros of C ζ 1 1 q s for values of q = 2 , q = 3 and q = 4 up to 10 decimal places.
Table 2. Some of the non-trivial and trivial complex and real zeros of C ζ 1 1 q s for values of q = 2 , q = 3 and q = 4 up to 10 decimal places.
Values of qTrivial Complex ZerosNon-Trivial Complex ZerosReal Zeros
q = 22.0460386041 + 14.0894409779i0.6078048160 + 1.9350010902i−2.514994862054
1.9443544646 + 21.0650038610i0.6078048160 − 1.9350010902i−4.675064985091
q = 33.2683247579 + 14.0859069231i−0.6997539191 + 1.7534110356i−3.180342471496
3.1531129164 + 21.0656065389i2.2160159281 + 2.0194666275i−5.450484894914
3.1027440708 + 24.9358435149i2.2160159281 − 2.0194666275i−7.577495596468
q = 44.3760513879 + 14.0924715621i−1.4515176098 + 1.2122471911i−4.035452332431
4.2716503066 + 21.0555557135i0.8794024170 + 2.3478232248i−6.316237379469
4.2263218286 + 24.9427024675i3.5554537875 + 1.9983004535i−8.456827453077
4.1822154523 + 30.5605816189i3.5554537875 − 1.9983004535i−10.54593349392
Table 3. Some observed equivalent results for F g b a ( n ) and C g b a ( n ) .
Table 3. Some observed equivalent results for F g b a ( n ) and C g b a ( n ) .
( 1 a , b ) Observed Equivalent Result for F g b a ( n ) Observed Equivalent Result for C g b a ( n )
( 2 , 2 ) ( n + 1 ) 2 2 n 2 2 = 2 n 2 + 1 n 2 2 ( n 1 ) 2 2 = 2 n 2
( 2 , 3 ) ( n + 1 ) 2 3 n 2 3 = 2 n 3 + 1 n 2 3 ( n 1 ) 2 3 = 2 n 2
( 2 , 4 ) ( n + 1 ) 2 4 n 2 4 = n 2 + ( 1 ) n n 2 4 ( n 1 ) 2 4 = n 2
( 3 , 2 ) ( n + 1 ) 3 2 n 3 2 = 3 n ( n + 1 ) 2 + n 2 n 1 2 n 3 2 ( n 1 ) 3 2 = 3 n ( n 1 ) 2 + n 2 n 1 2
( 3 , 3 ) ( n + 1 ) 3 3 n 3 3 = n ( n + 1 ) + n 3 n 1 3 n 3 2 ( n 1 ) 3 2 = n ( n 1 ) + n 3 n 1 3
( 3 , 4 ) ( n + 1 ) 3 4 n 3 4 = 3 n ( n + 1 ) 4 + n 2 n 1 2 n 3 4 ( n 1 ) 3 4 = 3 n ( n 1 ) 4 + n 2 n 1 2
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Shah, D.; Sahni, M.; Sahni, R.; León-Castro, E.; Olazabal-Lugo, M. Series of Floor and Ceiling Functions—Part II: Infinite Series. Mathematics 2022, 10, 1566. https://doi.org/10.3390/math10091566

AMA Style

Shah D, Sahni M, Sahni R, León-Castro E, Olazabal-Lugo M. Series of Floor and Ceiling Functions—Part II: Infinite Series. Mathematics. 2022; 10(9):1566. https://doi.org/10.3390/math10091566

Chicago/Turabian Style

Shah, Dhairya, Manoj Sahni, Ritu Sahni, Ernesto León-Castro, and Maricruz Olazabal-Lugo. 2022. "Series of Floor and Ceiling Functions—Part II: Infinite Series" Mathematics 10, no. 9: 1566. https://doi.org/10.3390/math10091566

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