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New Concept of Factorials and Combinatorial Numbers and its Consequences for Algebra and Analysis

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16 January 2026

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19 January 2026

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Abstract
In this article, the usual factorials and binomial coefficients have been generalized and extended to negative integers. Based on this generalization and extension, a new kind of polynomials has been proposed, which has directly led to the non-classical hypergeometric orthogonal polynomials and the non-classical second-order hypergeometric linear ordinary differential equations. The resulting polynomials can be used in non-relativistic and relativistic quantum mechanics, particularly in the case of the Schrödinger equation and Dirac equations for an electron in a Coulomb potential field.
Keywords: 
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1. Introduction

Usually, the factorial of a positive integer n , denoted by n   ! , is defined as the product of all positive integers less than or equal to n: n   !   =   n × ( n − 1 ) × ( n − 2 ) × ( n − 3 ) ×   ⋅ ⋅ ⋅   × 3 × 2 × 1 . The value of 0! is conventionally equal to 1. However, the factorials of negative integers cannot be computed, since for n = 0, the recurrence relation ( n − 1 ) ! = n   ! / n implies division by zero, and also due to the fact that the usual binomial coefficient C n k ≡ n k = n ! / k ! n − k ! is always equal to a positive integer.
The factorials are encountered in many areas of mathematics, notably in combinatorics, probability theory, number theory, statistics, algebra, and mathematical analysis. Their most basic use is to count the possible distinct sequences of n distinct objects: there are n! permutations. Factorials can also be extended to real numbers while retaining their most important properties. This involves using the gamma function to define Γ ( x + 1 ) = x   ! , where Γ ( x ) is the gamma function. However, as mentioned earlier, this extension does not work when x is a negative integer.
The factorials have a long and fascinating history [1,2]. They were used to count permutations at least as early as the 12th century, by Indian scholars [3]. In 1677, Fabian Stedman described factorials as applied to change ringing, a musical art involving the ringing of many tuned bells [4]. In 1808, the French mathematician Christian Kramp introduced the notation n! [5].
Concerning the gamma function and the extension of factorials to real negative numbers, many famous mathematicians worked on this topic, particularly Euler, Bernoulli (Daniel) Goldbach and De Moivre [6,7].
In fact, the field of factorials has attracted many modern researchers whose goal was the generalization of factorials and/or the extension of the gamma function [8,9,10,11,12,13]. However, the purpose and expectations of the present work are radically different from what has already been published on the topic under discussion, as we will see soon.

2. Generalization of Factorials to Negative Integers

The usual factorials of positive integers can be generalized to negative integers as follows. We have:
n   !     =     1 × 2 × 3   ×     ⋅ ⋅ ⋅     × n     ,
It is quite clear that multiplying each integer on the RHS of (1) by the constant ε     =     ± 1 is equivalent to multiplying the LHS of (1) by ( ε ) n :
( ε ) n n   !     =     ( ε 1 ) × ( ε 2 ) × ( ε 3 ) ×     ⋅ ⋅ ⋅     × ( ε n   )     .
Putting ε = − 1 in (2) yields
( − 1 ) n n   !     =     ( − 1 ) × ( − 2 ) × ( − 3 ) ×     ⋅ ⋅ ⋅     × ( − n   )     .
Using the notation ( − n )   !     =     ( − 1 ) × ( − 2 ) × ( − 3 ) ×     ⋅ ⋅ ⋅     × ( − n   )     to rewrite (3) in the following compact form
( − n )   !     =   ( − 1 ) n n   !    
As we can see, the relation (4) is, in fact, a special case of
( ε n )   !     =   ( ε ) n n   !
We refer to the relation (4) as ‘factorials of negative integers’. Therefore, Eq. (5) can be seen as a generalization of factorials to negative integers and beyond. Now, let's go back to (1) and rewrite it in the following form
( n   !   )     =     ( 1 × 2 × 3   ×     ⋅ ⋅ ⋅     × n   )     ,
Multiplying the two sides of (6) by − 1 to get
− ( n   !   )   =     −     ( 1 × 2 × 3   ×     ⋅ ⋅ ⋅     × n   )
From (4) and (7), we arrive at the result: in general
− ( n   !   ) ≠ ( − n )   !
Definition 1: We call a factorial number any expression of the form
( − n )   !     = [ −   ( n ) ]   !     =     ( − 1 ) n n   ! ( − n + k )   !     = [ −   ( n − k ) ]   !     =     ( − 1 ) n − k ( n − k )   ! ( − n − k )   !     = [ −   ( n + k ) ]   !     =     ( − 1 ) n + k ( n + k )   !
Result 1: From (1), (4) and (5) we get
  ε n n   ! = n   !                         if       ε = 1 ( − n )   !         if       ε = − 1
where n∈ℤ+ ≡ ℕ and ‒n∈ℤ‒ .

3. Generalization of Binomial Coefficients to Negative Integers

The previous generalization of factorials to negative integers allows us to generalize the binomial coefficients to negative integers along these lines. We have
C n k ≡ n k = n ! k ! n − k ! = ( n ) ! ( k ) ! n − k !
Replacing n with − n on both sides of (10) to get:
C − n k = ( − n ) ! ( k ) ! − n − k !
Taking into account Eq.(4) and definition (1), the expression (11) becomes:
C − n k = ( − 1 ) k n ! k ! n + k !
Again, replacing k with − k on both sides of (10) yields:
C n − k = ( − 1 ) k n ! k ! n + k !
Result 2: From (12) and (13), we get
C − n k = C n − k
Finally, replacing n and k with − n and − k , respectively, on both sides of (10) to obtain:
C − n − k = n ! k ! n − k !
Result 3: Comparing (10) and (15) yields:
C − n − k =     C n k
Definition 2: We call a combinatorial number any expression of the form (12), (13) and (15).
As we will see, the usual factorials of positive integers are, actually, a special case of Eq.(5), that is to say, when ε = 1 . Furthermore, the usual binomial coefficients are generalized to negative integers via the formulae (12), (13), and (15). To clarify all that, some usual factorials of positive integers, factorial numbers (factorials of negative integers), usual binomial coefficients and combinatorial numbers are, respectively, listed in Table 1 and Table 2.

3.1. Some Generalized Combinatorial Formulae

We deduce from definitions 1 and formulae (12), (13), and (15) the following interesting formulae which can be useful later.
C − n + k k = ( − 1 ) k ( n − k ) ! n ! k ! C − n − k C n − k = C n k C − n k = ( − 1 ) k ( n + k ) ! ( n − k ) ! C − n + k k · C − n − k = C − n + k k · C n k = ( − 1 ) k ( k ! ) 2 C − n − k · C n k = n ! k ! n − k ! 2 C − n k · C n − k = n ! k ! n + k ! 2 C − n − k · C − n k = C n k · C n − k = ( − 1 ) k n − k ! n + k ! n ! k ! 2

3.2. Application of the Generalized Combinatorial Numbers

The concept of generalized combinatorial numbers as a generalization of the usual binomial coefficients allows us to introduce a new kind of polynomials in which the generalized combinatorial numbers defined by formulae 12, 13, 15, and I-VI, play the role of coefficients. Let us begin with the polynomial H n   x − 1   ,   y − 1 of degree n in x − 1 and y − 1 :
H n   x − 1   ,   y − 1     = ∑ k = 0 n a n , k x n   − k y k
where x, y are real or complex with n, k∈ℕ and the coefficients a n ,   k are the generalized binomial coefficients (generalized combinatorial numbers). In this sense, a n ,   k ∈ C where C = {12, 13, 15, I, II, III, IV, V, VI} is the set of the generalized binomial coefficients defined by the formulae 12, 13, 15, and I-VI. Furthermore, in order to understand correctly the role and importance of a n , k , we make use of (13), (15), and (17) to define the following polynomials:
a n ,   k ∈ C | a n ,   k = C n − k ;   H n   x − 1   ,   y − 1     ≡ P n   x − 1   ,   y − 1 = ∑ k = 0 n C n − k 1 x n   − k y k
a n ,   k ∈ C | a n ,   k = C − n − k ;   H n   x − 1   ,   y − 1     ≡ Q n   x − 1   ,   y − 1 = ∑ k = 0 n C − n − k 1 x n   − k y k
First, we begin with (18), which can be written in explicit form as follows:
P n x − 1 , y − 1 = ∑ k = 0 n ( − 1 ) k n ! k ! n + k ! 1 x n − k 1 y k = 1 x n − n ! 1 ! n + 1 ! 1 x n − 1 1 y 1 + n ! 2 ! n + 2 ! 1 x n − 2 1 y 2 −   … + ( − 1 ) n 2 n ! 1 y n
The first few P-polynomials
P 0 x − 1 , y − 1 = 1 P 1 x − 1 , y − 1 = x − 1 − 1 2 y − 1 P 2 x − 1 , y − 1 = x − 2 − 1 3 x − 1 y − 1 + 1 24 y − 2
P 3 x − 1 , y − 1 = x − 3 − 1 4 x − 2 y − 1 + 1 40 x − 1 y − 2 − 1 720 y − 3 P 4 x − 1 , y − 1 = x − 4 − 1 5 x − 3 y − 1 + 1 60 x − 2 y − 2 − 1 1260 x − 1 y − 3 + 1 40320 y − 4 P 5 x − 1 , y − 1 = x − 5 − 1 6 x − 4 y − 1 + 1 84 x − 3 y − 2 − 1 2016 x − 2 y − 3 + 1 72576 x − 1 y − 4 − 1 39916800 y − 5
Derivative formulae for P-polynomial
mth -order partial derivative of P n   x − 1   ,   y − 1 w.r.t x − 1 , x , y − 1 and y , respectively.
x − 1 m ∂ m P n   ∂ x − 1 m     =   ∑ k = 0 n C n − k ( n   −   k ) ( m ) x n   − k y k
x m ∂ m P n   ∂ x m     = ( − 1 ) m   ∑ k = 0 n C n − k ( n   −   k ) ( m ) x n   − k y k
y − 1 m ∂ m P n   ∂ y − 1 m     =   ∑ k = 0 n C n − k   k ( m ) x n   − k y k
y m ∂ m P n   ∂ y m     = ( − 1 ) m   ∑ k = 0 n C n − k k ( m ) x n   − k y k
where ( n   −   k ) ( m ) , k ( m ) are the falling factorials and ( n   −   k ) ( m ) , k ( m ) are the rising factorials.
Characteristic values
P 0   x − 1   ,   y − 1   =   1   , P n   1   ,   1   =   ∑ k = 0 n C n − k   ,   P n   ∞   ,   ∞ = 1   ,   P n   x − 1 ,   y − 1   ( x , y ) → ( 0 , 0 ) =   ∞
Parity
P n   − x − 1 , − y − 1 =     ( − 1 ) n P n   x − 1 , y − 1
Property
Now, supposing that y is fixed by putting α = y − 1 and z = x − 1 , we get, after substitution in (20), the polynomial P n z , α ≡ P n α z of order α and degree n in z :
P n α z = ∑ k = 0 n C n − k α k z n − k = n ! z n n ! − α 1 1 ! n + 1 ! z n − 1 + α 2 2 ! n + 2 ! z n − 2   … + ( − 1 ) n α n n ! 2 n !
The polynomial (26) satisfies the second-order self-adjoint ODE
d d z z 2 d U d z − η U = z λ γ f n ( z , α )
, for the interesting special case when η = n ( n + 1 ) and γ = n , where
f n z , α = ∑ k = 0 n C k n α z k ,   C k n = ( − 1 ) k + 1 k ( 2 n − k + 1 ) k ! ( n + 1 ) ( k )

4. Non-Classical Hypergeometric Orthogonal Polynomials

The well-known sets of orthogonal polynomials (OPs) such as Jacobi polynomials J n ( α , β ) x n = 0 ∞ , Laguerre polynomials L n ( α ) x n = 0 ∞ [14,15,16], Hermite polynomials H n x n = 0 ∞ , and Bessel polynomials B n ( a ) x n = 0 ∞ , which include important special cases like Legendre polynomials, Chebyshev polynomials, and Gegenbauer polynomials, are typically referred to as classical (hypergeometric) OPs [17,18,19,20]. This is because they satisfy the four classical hypergeometric linear ODEs, namely:
Jacobi Eq.:
1 − x 2 y " + β − α − α + β + 2 x y ' + n n + α + β + 1 y = 0

4.1. π-Polynomials

Throughout the rest of this paper we concentrate exclusively on the derivation of π-polynomials and their differential equation, generating function, recurrence relation, derivative formula, weight function, Rodrigues' formula, characteristic values as well as their properties . But first, let us begin with their derivation as follows. Assuming that y is fixed, we let z = x − 1 and   λ = α + β = y − 1 . After substitution in (19), we get:
1 n ! Q n z , λ = ∑ k = 0 n λ k k ! n − k ! z n − k
Replacing λ k with the rising factorial λ ( k ) = λ λ + 1 λ + 2 … λ + k − 1 = Γ ( λ + k ) / Γ ( λ ) ,   λ ( 0 ) = 1 . We obtain
1 n ! Q n z , λ ≡ π n ( α , β ) z
Where
π n ( α , β ) z = ∑ k = 0 n λ ( k ) k ! n − k ! z n − k = 1 n ! ∑ k = 0 n C n k λ ( k ) z n − k   ,   λ = α + β

4.2. Properties of p-polynomials

Characteristic values
π 0 ( α , β ) z = 1 π n ( α , β ) 0 = λ ( n ) n ! = Γ ( λ + n ) n ! Γ ( λ ) π n ( α , β ) 1 = ∑ k = 0 n λ ( k ) k ! n − k ! = ∑ k = 0 n Γ ( λ + k ) k ! n − k ! Γ ( λ ) π n ( α , β ) − 1 = ∑ k = 0 n ( − 1 ) ( n − k ) λ ( k ) k ! n − k ! = ∑ k = 0 n ( − 1 ) ( n − k ) Γ ( λ + k ) k ! n − k ! Γ ( λ ) π n ( 1 / 2,1 / 2 ) 0 = 1 π n ( α , β ) 0 = λ ( n ) n ! = Γ ( λ + n ) n ! Γ ( λ ) π n ( α , β ) 1 = ∑ k = 0 n λ ( k ) k ! n − k ! = ∑ k = 0 n Γ ( λ + k ) k ! n − k ! Γ ( λ ) π n ( α , β ) − 1 = ∑ k = 0 n ( − 1 ) ( n − k ) λ ( k ) k ! n − k ! = ∑ k = 0 n ( − 1 ) ( n − k ) Γ ( λ + k ) k ! n − k ! Γ ( λ ) π n ( 1 / 2,1 / 2 ) 0 = 1 π n ( − 1 / 2 , − 1 / 2 ) 0 = 0 π n ( 1 / 2,1 / 2 ) 1 = ∑ k = 0 n 1 n − k ! π n ( − 1 / 2 , − 1 / 2 ) 1 = ∑ k = 0 n ( − 1 ) k n − k !
p-monomial
We obtain the π -monomial for the interesting special case when α = β = 0 , that is π n ( 0,0 ) z = z n n ! which satisfies the non-classical second-order hypergeometric linear ODE:
z u " − ( z + n − 1 ) u ' + n u = 0
Orthogonality
Now we prove the orthogonality of π -polynomials w.r.t the weight function (42) on the interval
(0, ∞). That is to say, we will get ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0 if m ≠ n . To this end, let us rewrite Eq.(36) in the following self-adjoint form:
d d z z ρ u ' + n ρ u = 0
Then by Eq. (45), we get
d d z z ρ π ' m ( α , β ) z + m ρ π m ( α , β ) z = 0
d d z z ρ π ' n ( α , β ) z + n ρ π n ( α , β ) z = 0
Multiply (46) by π n ( α , β ) z and integrate from   z = 0 to z = ∞ to obtain
∫ 0 ∞ d d z z ρ π ' m ( α , β ) z π n ( α , β ) z d z + m ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0
Integrating the first integral by parts we get
z ρ π ' m ( α , β ) z π n ( α , β ) z 0 ∞ − ∫ 0 ∞ z ρ π ' m α , β z π ' n α , β z d z + m ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0

4.3. Series of p-Polynomials

As a direct consequence of p-polynomials, we can refer to the series of p-polynomials.That is to say, any continuous function   f ( z ) on the interval ( 0 ,     ∞ ) such that   z < 1 , may be expanded in a series of p-polynomials. More precisely, let us prove that if
f z = ∑ n = 0 ∞ c n π n ( α , β ) z ,   z < 1
this implies
c n = n ! Γ ( 1 − λ ) ∫ 0 ∞ ρ π n ( α , β ) z f z d z ,   λ < 1
To achieve this, we multiply the series (59) by   ρ π m ( α , β ) z and integrate from z = 0 to z = ∞ . Taking into account the previous result, namely the expression (57), we get
∫ 0 ∞ ρ π m ( α , β ) z f z d z = ∑ n = 0 ∞ c n ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z
For the case when m = n , we have
∫ 0 ∞ ρ π n ( α , β ) z f z d z = c n ∫ 0 ∞ ρ π n ( α , β ) z 2 d z
By taking into account (57), we can derive the expected formula (60) from the above expression.
Illustrative example: Let f z = z 3 − 3 z 2 + z − 2 be a continuous function on the interval ( 0 ,   ∞ ) such that z < 1 . Our aim is to find the expansion of f ( z ) in a series of p-polynomials for the interesting case when   α = β = − n / 2 , i.e., λ = − n . First, note that ( − n ) ( k ) = ( − 1 ) k n ( k ) , where n ( k ) = n n − 1 n − 2 … n − k + 1 with n ( 0 ) = 1 and n n = n ! , is the falling factorial, therefore, after substitution in (35), we obtain:
π n ( − n / 2 , − n / 2 ) z = 1 n ! ∑ k = 0 n ( − 1 ) k C n k n ( k ) z n − k
The few first π -polynomials for α = β = − n / 2
π 0 ( 0,0 ) z = 1 π 1 ( − 1 / 2 , − 1 / 2 ) z = z − 1 π 2 ( − 1 , − 1 ) z = 1 2 ! z 2 − 4 z + 2 π 3 ( − 3 / 2 , − 3 / 2 ) z = 1 3 ! z 3 − 9 z 2 + 18 z − 6
π 4 ( − 2 , − 2 ) z = 1 4 ! z 4 − 16 z 3 + 72 z 2 − 96 z + 24 π 5 ( − 5 / 2 , − 5 / 2 ) z = 1 5 ! z 5 − 25 z 4 + 200 z 3 − 600 z 2 + 600 z − 120 π 6 ( − 3 , − 3 ) z = 1 6 ! z 6 − 36 z 5 + 450 z 4 − 2400 z 3 + 5400 z 2 − 4320 z + 720
We have according to (59)
f z = ∑ n = 0 ∞ c n π n ( − n / 2 , − n / 2 ) z = c 0 π 0 ( 0,0 ) z + c 1 π 1 ( − 1 / 2 , − 1 / 2 ) z + c 2 π 2 ( − 1 , − 1 ) z +
It is clear from the explicit expression of f ( z ) , that is, we should have c 4   =   c 5   =   c 6   =     ⋅ ⋅ ⋅     = 0 . Consequently, the above expression becomes
f z = ∑ n = 0 3 c n π n − n / 2 , − n / 2 z = c 0 π 0 ( 0,0 ) z + c 1 π 1 ( − 1 / 2 , − 1 / 2 ) z + c 2 π 2 ( − 1 , − 1 ) z + c 3 π 3 ( − 3 / 2 , − 3 / 2 ) z
Using the formula (60) to get the following values for the coefficients:   c 0 = − 1 ,   c 1 = 7 , c 2 = 12 , c 3 = 6 . Finally, after substitution, we obtain the requested expansion:
f ( z ) = − π 0 ( 0,0 ) z + 7 π 1 ( − 1 / 2 , − 1 / 2 ) z + 12 π 2 ( − 1 , − 1 ) z + 6 π 3 ( − 3 / 2 , − 3 / 2 ) z

4.4. Consequences of p-Polynomials

The consequences and applications of p-polynomials are generally related to the specialization of their bi-order (α,β). For instance, as a direct consequence of p-polynomials we can refer to the series of p-polynomials. It may be added that the p-polynomials and their reverse can be used in physics, particularly in non-relativistic and relativistic quantum mechanics, as we will see. With this aim, we shall now consider the following interesting special case, that is, when α = − a ,     β = − n , and a is real or complex with n∈ℕ. Therefore, after substitution, the p-polynomials (35) and their ODE (36) become
π n ( − a , − n ) z = ∑ k = 0 n ( − 1 ) k ( a + n ) ( k ) k ! n − k ! z n − k = ∑ k = 0 n ( − 1 ) k a + n k z n − k n − k !
z u " + 1 + a − z u ' + n u = 0
The first fewp-polynomials for α = − a ,     β = − n
  π 0 ( − a , 0 ) z = 1 π 1 ( − a , − 1 ) z = z − ( a + 1 ) ( 1 ) π 2 ( − a , − 2 ) z = z 2 2 − a + 2 1 z + ( a + 2 ) ( 2 ) 2 π 3 ( − a , − 3 ) z = z 3 6 − a + 3 1 2 z 2 + a + 3 2 2 z − ( a + 3 ) ( 3 ) 6
π 4 − a , − 4 z = z 4 24 − a + 4 1 6 z 3 + a + 4 2 4 z 2 − a + 4 3 6 z + a + 4 4 24 π 5 ( − a , − 5 ) z = z 5 120 − a + 5 1 24 z 4 + a + 5 2 12 z 3 − a + 5 3 12 z 2 + a + 5 4 24 − a + 5 5 120 π 6 ( − a , − 6 ) z = z 6 720 − a + 6 1 120 z 5 + a + 6 2 48 z 4 − a + 6 3 36 z 3 + a + 6 4 48 − a + 6 5 120 + a + 6 6 720
It is worthwhile to note that in spite of the fact that Eq.(64) is identical to the so-called Laguerre (generalized) equation([1]), the polynomials (63) are not strictly speaking identical to the alleged generalized (associated) Laguerre polynomials
L n ( a ) z = ∑ k = 0 n ( − 1 ) k a + n n − k z k k !
Since both polynomials (63) and (i) have not the same explicit expressions for the recurrence relations and derivative formulae, respectively:
( n + 1 ) π n + 1 ( − a , − n ) z = z − a π n − a , − n z − z π n − 1 ( − a , − n ) z ;   d d z π n ( − a , − n ) z = π n − 1 ( − a , − n ) z
And
( n + 1 ) L n + 1 ( a ) z = a + 2 n + 1 − z L n a z − ( a + n ) L n − 1 ( a ) z ;   d d z L n ( a ) z = − L n − 1 ( a + 1 ) z
This implies, among other things, that they have not the same generating function. Consequently, the polynomials π n ( − a , − n ) z can also be used in non-relativistic and relativistic QM, particularly, in the case of the Schrödinger equation, and Dirac equations for an electron in a Coulomb potential field. However, we can show that there is some link between π n ( − a , − n ) z and L n ( a ) z through the reverse polynomials π ¯ n ( − a , − n ) z , which can be easily deduced from (63):
π ¯ n ( − a , − n ) z = ∑ k = 0 n ( − 1 ) n − k a + n n − k z k k !
The first few π ¯ -polynomials
π ¯ 0 ( − a ,   0 ) z = 1 π ¯ 1 ( − a ,   − 1 ) z = −   ( a + 1 ) ( 1 ) + z π ¯ 2 ( − a ,   − 2 ) z = ( a   +   2 ) ( 2 ) 2 − ( a + 2 ) ( 1 ) z + z 2 2
π ¯ 3 ( − a ,   − 3 ) z = − ( a   +   3 ) ( 3 ) 6 + ( a   +   3 ) ( 2 ) 2 z − ( a   +   3 ) ( 1 ) 2 z 2 + z 3 6 π ¯ 4 ( − a ,   − 4 ) z = ( a   +   4 ) ( 4 ) 24 − ( a   +   4 ) ( 3 ) 6 z + ( a   +   4 ) ( 2 ) 4 z 2 − ( a   +   4 ) ( 1 ) 6 z 3 + z 4 24 π ¯ 5 ( − a ,   − 5 ) z = ( a   +   5 ) ( 5 ) 120 − ( a   +   5 ) ( 4 ) 24 z + ( a   +   5 ) ( 6 ) 12 z 2 − ( a   +   5 ) ( 1 ) 12 z 4 + z 4 24 + z 5 120 .
As we can see from (65) and (67), the polynomials π n ( − a , − n ) z are arranged in descending power order of z while the polynomials π ¯ n ( − a , − n ) z are arranged in ascending power order of z, and as the descending power order is more commonly used that is why (66) are called the ‘reverse’ polynomials or simply
π ¯ −polynomials. We now proceed to show that there is actually some link between π n ( − a , − n ) z and L n ( a ) z through π ¯ n ( − a , − n ) z , which can be rewritten in the following form:
π ¯ n ( − a , − n ) z =   ( − 1 ) n   ∑ k = 0 n ( − 1 ) k   a   +   n n   −   k     z k   k !
a simple comparison between (i) and (68) leads directly to the expression:
π ¯ n ( − a , − n ) z =   ( − 1 ) n   L n ( a ) ( z )
or equivalently
L n ( a ) ( z ) =   ( − 1 ) n   π ¯ n ( − a , − n ) z
Expressions (69) and (70) mean that the polynomials π ¯ n ( − a , − n ) z are expressible in terms of the polynomials L n ( a ) ( z ) and vice versa. Moreover, the polynomials π n ( − a , − n ) z are related to the Hermite ones through π ¯ n ( − a , − n ) z :
H 2 n ( z ) =   2 2 n   n   ! π ¯ n ( 1 / 2 , − n ) z 2
H 2 n   + 1 ( z ) =   2 2 n   + 1   n   ! z π ¯ n ( − 1 / 2 , − n ) z 2
Because of this, the polynomials π ¯ n ( − a , − n ) z can be arisen in the treatment of the quantum harmonic oscillator.
Associated φ-functions
In terms of the polynomials π n ( − a , − n ) z , we can define the associated φ-functions as:
ϕ n   ( z ,   a ) =   z a 2   e − z 2   π n ( − a , − n ) z
Using Eq.(64), we get the following self-adjoint DE for φ-functions
z ϕ ″ n   + ϕ ′ n +   2 n   +   a   +   1 2   −   z 4   −   a 2 4 z ϕ n = 0
Therefore, φ-functions are eigen-functions of a Sturm-Liouville system on the interval (0, ∞).
π ˜ -polynomials
Now returning to the π ˜ -polynomials (37), solutions of Eq.(36), and considering the same previous special case, i.e., when α = − a ,     β = − n , we get after substitution in (37):
π ˜ n ( − a , − n ) z =   ∑ k = 0 n   ( − 1 ) k     n ( k ) ( a   +   1 ) ( k )       z k k !
or equivalently
π ˜ n ( − a , − n ) z =     1 ( a   +   1 ) ( n )     ∑ k = 0 n   ( − 1 ) k     n ( k )   k !     ( a   +   n ) ( n   − k ) z k
which are also solutions of Eq.(64).
The first six π ˜ -polynomials
π ˜ 0 ( − a ,   0 ) z = 1 π ˜ 1 ( − a ,   − 1 ) z = 1 −   1 ( a + 1 ) ( 1 ) z π ˜ 2 ( − a ,   − 2 ) z = 1 −   2 ( a   +   1 ) ( 1 ) z +   1 ( a   +   1 ) ( 2 ) z 2

4.5. μ-Monomials and κ-Polynomials

In addition to the properties of p-polynomials (35) mentioned in the previous section, there is another specific property which is in fact a direct consequence of the explicit expression of p-polynomials which can also be written in the form of the product of μ-monomials in z and κ-polynomials in (z‒1) as follows:
π n ( α , β ) z =   ∑ k = 0 n   λ ( k ) k !   ( n   −   k ) !   z n   − k = z n   ∑ k = 0 n   λ ( k ) k !   ( n   −   k ) !   1 z k = μ n z κ n ( α , β ) z
where the μ-monomials μ n z = z n or equivalently μ n z = n   ! π n ( 0 , 0 ) z   satisfy Eq.(44).
Now, let us focus our attention exclusively on the κ-polynomials
κ n ( α , β ) z = ∑ k = 0 n   λ ( k ) k !   ( n   −   k ) !   1 z k ,   λ = α + β
which satisfy the DE
z 2 w ″   +     z ( n   − λ + 1 − z )   w ′ − n   λ   w = 0
The first fewκ-polynomials
  κ 0 ( α , β ) z =     1 κ 1 ( α , β ) z =   1     +     λ z − 1 κ 2 ( α , β ) z =   1 2     +     λ z − 1   +     λ ( 2 ) 2 z − 2 κ 3 ( α , β ) z = 1 6     +       λ 2 z − 1     +       λ ( 2 ) 2 z − 2 +       λ ( 3 ) 6 z − 3   κ 4 ( α , β ) z = 1 24     +     λ 6 z − 1   +     λ ( 2 ) 4 z − 2 +     λ ( 3 ) 6 z − 3 +     λ ( 4 ) 24   z − 4 κ 5 ( α , β ) z =   1 120 +     λ 24 z − 1     +     λ ( 2 ) 12 z − 2 +     λ ( 3 ) 12 z − 3   +     λ ( 4 ) 24 z − 4     +       λ ( 5 ) 120 z − 5 κ 6 ( α , β ) z =   1 720     +     λ 120 z − 1     +     λ ( 2 ) 48 z − 2 +     λ ( 3 ) 36 z − 3   +     λ ( 4 ) 48 z − 4     +       λ ( 5 ) 120 z − 5   +     λ ( 6 ) 720 z − 6     .
Generating function forκ-polynomials
    g ( z ,   t ,   α ,   β ) = 1 −     t z − λ e t ,   λ = α + β
Recurrence relation
    ( n + 1 ) κ n   + 1 ( α , β ) z = 1   +     λ   +   n z   κ n ( α , β ) z −     λ   z 2   κ n − 1 ( α , β ) z
Derivative formula
d κ n ( α , β ) z d z     =     1 z d κ n   − 1 ( α , β ) z d z   −   λ z 2 κ n   − 1 ( α , β ) z
Weight function
ρ ( z ,     α ,   β ,   n ) = z γ e − z ,   γ =   n   − λ − 1
Laguerre Eq.:
x y " + α + 1 − x y ' + n y = 0
Hermite Eq.:
y " + 2 x y ' + 2 n y = 0
(iii)
Bessel Eq.
x 2 y " + a x + b y ' − n n + a − 1 y = 0
Also, the classical OPs have the property that their derivatives form orthogonal systems.
In addition to the above-mentioned classical OPs, there is a new class of Ops π n ( α , β ) z n = 0 ∞ which do not belong to the classical sets of OPs. They are called non-classical (hypergeometric) OPs because, in addition to their property of orthogonality, they satisfy a non-classical second-order hypergeometric linear ODE of the form:
A z u " + B ( z , α , β , n ) u ' + μ n u = 0
such that the coefficients of u " and u ' are quadratic and/or linear polynomials; ( α , β   ) and n are, respectively, the bi-order and degree of the polynomial solutions of Eq.(29); the characteristic parameter μ n depends on the polynomial's degree ‘n’ and is defined by
μ n = − n n − 1 2 A " + B '
The weight function   ρ z , λ , n of polynomial solutions is given by
A ρ ' = B ρ
and satisfies the condition
lim z → a A ρ = lim z → b A ρ = 0
where a and b are the end points of the interval of orthogonality of polynomial solutions and z , λ are real or complex with λ = α + β and n∈ℕ.
As we can see, Eq.(29) is different from the second-order classical hypergeometric linear ODEs (i-iv) in that‒the coefficient of u ′ contains the positive integral parameter ‘n’ which is the degree of polynomial solutions of Eq.(29). Furthermore, the explicit presence of the polynomial's degree ‘n’ in the coefficients of u ′ and u implies that the sequences   B ( z , α , β , n ) n = 0 ∞ and μ n n = 0 ∞ correspond to a unique sequence π n ( α , β ) z n = 0 ∞ of polynomial solutions of Eq.(29).
The π -polynomials of bi-order ( α , β ) and degree n in z are the highly anticipated ones that satisfy the non-classical second-order hypergeometric linear ODE:
z u " − z + λ + n − 1 u ' + n u = 0 ,   λ = α + β
Furthermore, the π ~ -polynomials defined by the following explicit formula
π ~ n ( α , β ) z = ∑ k = 0 n n ( k ) k ! γ ( k ) z k ,   γ = λ + n − 1
are also solutions of Eq.(36).
The first few π -polynomials
π 0 ( α , β ) z = 1 π 1 ( α , β ) z = z + λ ( 1 ) π 2 ( α , β ) z = 1 2 ! z 2 + 2 λ ( 1 ) z + λ ( 2 ) π 3 ( α , β ) z = 1 3 ! z 3 + 3 λ ( 1 ) z 2 + 3 λ ( 2 ) z + λ ( 3 ) π 4 ( α , β ) z = 1 4 ! z 4 + 4 λ ( 1 ) z 3 + 6 λ ( 2 ) z 2 + 4 λ ( 3 ) z + λ ( 4 ) π 5 ( α , β ) z = 1 5 ! z 5 + 5 λ ( 1 ) z 4 + 10 λ ( 2 ) z 3 + 10 λ ( 3 ) z 2 + 5 λ ( 4 ) z + λ ( 5 ) π 6 ( α , β ) z = 1 6 ! z 6 + 6 λ ( 1 ) z 5 + 15 λ ( 2 ) z 4 + 20 λ ( 3 ) z 3 + 15 λ ( 4 ) z 2 + 6 λ ( 5 ) z + λ ( 6 )
Generating function forp-polynomials
g z , t , λ = e z t ( 1 − t ) λ ,   λ = ( α + β )
Recurrence relation
( n + 1 ) π n + 1 ( α , β ) z = z + + n π n α , β z − z π n − 1 ( α , β ) z
Derivative formula
d d z π n ( α , β ) z = π n − 1 ( α , β ) z
Weight function
ρ z , λ , n = z − ( λ + n ) e − z ,   λ = ( α + β )
The analogue of Rodrigues' formula
π n ( α , β ) z = ( − 1 ) n n ! z λ + n e z d n d z n z − λ e − z   ,   λ = ( α + β )
Since, according to (42), we have lim z   → 0 ( z ρ ) = lim z   → 0 ( z 1 − γ e − z ) = 0 and lim z   → ∞ ( z ρ ) = lim z   → ∞ ( z 1 − γ e − z ) = 0 with γ =     λ + n < 1 , thus the above expression becomes
− ∫ 0 ∞ z ρ π ' m α , β z π ' n α , β z d z + m ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0
In exactly the same way, we can multiply (47) by π m ( α ,   β ) z and integrate by parts from z = 0 to z = ∞ to obtain
− ∫ 0 ∞ z ρ π ' m α , β z π ' n α , β z d z + n ∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0
Finally, subtracting (49) from (48), we get the expected orthogonality condition
∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = 0 ,   m ≠ n
At present, let us evaluate the integral ∫ 0 ∞ ρ π n ( α , β ) z 2 d z , that is, the integral (50) for the case when m = n . First, we have
I n = ∫ 0 ∞ ρ π n ( α , β ) z 2 d z
Combining (42) and (43) yields
π n ( α , β ) z = ( − 1 ) n n ! ρ − 1 d n d z n z n ρ
From (51) and (52), we get
I n = ( − 1 ) n n ! ∫ 0 ∞ π n ( α , β ) z d n d z n z − λ e − z d z
Integration by parts gives
I n = ( − 1 ) n n ! π n ( α , β ) z d n − 1 d z n − 1 z − λ e − z 0 ∞ − ( − 1 ) n n ! ∫ 0 ∞ d d z π n ( α , β ) z d n − 1 d z n − 1 z − λ e − z d z
The first term on the RHS is zero, hence by integrating several times by parts, we find
I n = 1 n ! ∫ 0 ∞ z − λ e z d n d z n π n ( α , β ) z d z
Since d n d z n π n ( α , β ) z = 1 and ∫ 0 ∞ z − λ e z d z = Γ 1 − λ     for λ < 1 thus the above integral becomes
I n = Γ ( 1 − λ ) n !
From (51) and (56), we obtain the expected expression
I n = ∫ 0 ∞ ρ π n ( α , β ) z 2 d z = Γ ( 1 − λ ) n ! ,   λ = ( α + β ) < 1
Finally, combining (50) and (57), we get
∫ 0 ∞ ρ π m ( α , β ) z π n ( α , β ) z d z = δ m n Γ ( 1 − λ ) n !
where   λ = ( α + β ) < 1 and δ m n is the Kronecker delta defined as δ m n = 0   i f   m ≠ n 1   i f   m = n .
(77)
π ˜ 3 ( − a ,   − 3 ) z = 1 − 3 ( a   +   1 ) ( 1 ) z + 3 ( a   +   1 ) ( 2 ) z 2 − 1 ( a   +   1 ) ( 3 ) z 3 π ˜ 4 ( − a ,   − 4 ) z = 1 − 4 ( a   +   1 ) ( 1 ) z + 6 ( a   +   1 ) ( 2 ) z 2 − 4 ( a   +   1 ) ( 3 ) z 3 + 1 ( a   +   1 ) ( 4 ) z 4 π ˜ 5 ( − a ,   − 5 ) z = 1 − 5 ( a   +   1 ) ( 1 ) z + 10 ( a   +   1 ) ( 2 ) z 2 − 10 ( a   +   1 ) ( 3 ) z 3 + 5 ( a   +   1 ) ( 4 ) z 4 − 1 ( a   +   1 ) ( 5 ) z 5
The analogue of Ridrogues' formula
π ˜ n ( − a , − n ) z =     1 ( a   +   n   ) ( n )   z − a e z d n d z n z a + n e − z
(78
The polynomials (75) are related to π n ( − a , − n ) z for α = ‒ a and β = ‒ n by the following relation:
π n ( − a , − n ) z =     ( − 1 ) n   ( a   +   n   ) ( n ) n   !   π ˜ n ( − a , − n ) z
It may be added that the orthogonality property of the polynomials (75) is a direct consequence of the orthogonality of p-polynomials (35) and without difficulty can be shown to be of the form:
∫ 0 ∞ z a e − z       π ˜ m ( − a ,   − n ) z   π ˜ n ( − a ,   − n ) z d z = δ m n n   !   Γ ( a + 1 ) 2 Γ ( a + n + 1 )
The analogue of Rodrigues' formula
κ n ( α , β ) z = ( − 1 ) n n   ! z λ e z   d n d z n   z − λ e − z
Characteristic values
κ n ( α , β ) ∞ = κ n ( 0 , 0 ) z = 1 n   ! κ n ( α , β ) 0 = ∞ κ n ( α , β ) 1 = ∑ k = 0 n   λ ( k ) k !   ( n   −   k ) !     = ∑ k = 0 n   Γ ( λ +   k ) k !   ( n   −   k ) !   Γ ( λ ) κ n ( α , β ) − 1 = ∑ k = 0 n   ( − 1 ) k λ ( k ) k !   ( n   −   k ) !     = ∑ k = 0 n   ( − 1 ) k Γ ( λ +   k ) k !   ( n   −   k ) !   Γ ( λ )
Some properties
κ n ( α , β ) − z = ∑ k = 0 n   ( − 1 ) k λ ( k ) k !   ( n   −   k ) !   1 z k   ,         λ = α + β κ n ( − α , − β ) z = ∑ k = 0 n   ( − 1 ) k λ ( k ) k !   ( n   −   k ) !   1 z k   κ n ( − α , − β ) − z = ∑ k = 0 n   λ ( k ) k !   ( n   −   k ) !   1 z k   κ n ( − α , β ) z = ∑ k = 0 n   ( β −   α ) ( k ) k !   ( n   −   k ) !   1 z k   κ n ( α , − β ) z = ∑ k = 0 n   ( − 1 ) k ( β −   α ) ( k ) k !   ( n   −   k ) !   1 z k   κ n ( − α , β ) − z = ∑ k = 0 n   ( − 1 ) k ( β −   α ) ( k ) k !   ( n   −   k ) !   1 z k   κ n ( α , − β ) − z = ∑ k = 0 n   ( β −   α ) ( k ) k !   ( n   −   k ) !   1 z k  
Orthogonality
To show the orthogonality property of κ-polynomials on the interval (0, ∞) w.r.t the weight function (87) it suffices to follow the usual procedure. With this aim, let us first rewrite Eq.(82) in self-adjoint form.
d d z   z 2 ρ w ′     −   n   λ ρ w   =   0.
Then by (89) we have
d d z   z 2 ρ d κ m ( α , β ) z d z     −   m   λ ρ κ m ( α , β ) z =   0
d d z   z 2 ρ d κ n ( α , β ) z d z     −   n   λ ρ κ n ( α , β ) z =   0
where m     ≠     n   .
Now, we multiply (90) by κ n ( α , β ) z and integrate from z = 0 to z = ∞ to obtain
∫ 0 ∞ d d z   z 2 ρ d κ m ( α , β ) z d z κ n ( α , β ) z   d z   −   m   λ ∫ 0 ∞ ρ κ m ( α , β ) z   κ n ( α , β ) z   d z =   0
Integrating the first integral by parts we get:
z 2 ρ d κ m ( α , β ) z d z κ n ( α , β ) z 0 ∞   −   ∫ 0 ∞   z 2 ρ d κ m ( α , β ) z d z d κ n ( α , β ) z d z   d z   −   m   λ ∫ 0 ∞ ρ κ m ( α , β ) z   κ n ( α , β ) z   d z =   0
By taking into account the explicit expression of the weight function (87), we have
lim z   → 0   ( z γ + 2 e − z ) = lim z   → ∞   ( z γ + 2 e − z ) = 0 with γ > − 2 , thus the above expression becomes:
  ∫ 0 ∞   z 2 ρ d κ m ( α , β ) z d z d κ n ( α , β ) z d z   d z     +     m   λ ∫ 0 ∞ ρ κ m ( α , β ) z κ n ( α , β ) z =   0
In exactly the same way we can multiply (91) by κ m ( α , β ) z and integrate from z = 0 to z = ∞ to find
  ∫ 0 ∞   z 2 ρ d κ m ( α , β ) z d z d κ n ( α , β ) z d z   d z     +     n   λ ∫ 0 ∞ ρ κ m ( α , β ) z κ n ( α , β ) z =   0
Subtracting (93) from (92) and replacing the weight function ρ by its explicit expression (87) we get the very expected orthogonality condition:
∫ 0 ∞ z γ e − z κ m ( α , β ) z   κ n ( α , β ) z   d z = 0 ,   m ≠ n
Finally, let us evaluate the integral ∫ 0 ∞ ρ   κ n ( α , β ) z 2 d z as follows. First, we have
I n = ∫ 0 ∞ ρ   κ n ( α , β ) z 2 d z
Secondly, rewriting the generating function in its explicit form
e t   1 −     t z − λ = ∑ n   = 0 ∞ κ n ( α , β ) z   t n   ,           λ =   α + β .
Square and multiply both sides of (96) by the weight function (87) to obtain:
e 2 t   1 −     t z − 2 λ ρ = ∑ n   = 0 ∞ ρ   κ n ( α , β ) z 2 t 2 n   .
Now, let us focus our attention on the LHS of (97) which can also be written in terms of series as follows:
e 2 t   1 −     t z − 2 λ ρ = ∑ n   = 0 ∞ 2 n ( 2 λ ) ( n ) ( n   ! ) 2 t 2 n z n   ρ = ∑ n   = 0 ∞ 2 n ( 2 λ ) ( n ) ( n   ! ) 2   z −   ( λ + 1 )   e − z   t 2 n
and after substitution, (97) becomes
∑ n   = 0 ∞ z γ   e − z   κ n ( α , β ) z 2 t 2 n = ∑ n   = 0 ∞ 2 n ( 2 λ ) ( n ) ( n   ! ) 2   z −   ( λ + 1 )   e − z t 2 n
with γ = n − λ − 1 , λ =     α + β .
Integrating (98) from z = 0 to z = ∞, we get after simplification
∫ 0 ∞ z γ e − z   κ n ( α , β ) z 2 d z = 2 n ( 2 λ ) ( n ) ( n   ! ) 2 ∫ 0 ∞ z − ( λ + 1 )   e − z d z
Since ( 2 λ ) ( n )   =   Γ ( 2 λ   +   n ) / Γ ( 2 λ   ) and ∫ 0 ∞ z −   ( λ + 1 )   e − z d z =   Γ ( − λ   ) , λ < 0, therefore (99) becomes:
∫ 0 ∞ z γ e − z   κ n ( α , β ) z 2 d z = 2 n Γ ( 2 λ + n ) ( n   ! ) 2 Γ ( 2 λ ) Γ ( − λ )

5. Conclusion

In this paper, the usual factorials and binomial coefficients have been generalized and extended by means of the new concept of factorials and combinatorial numbers to the negative integers. Based on this generalization and extension, a new kind of polynomials has been proposed, which led directly to the non-classical hypergeometric orthogonal polynomials and the non-classical second-order hypergeometric linear DEs. Also the resulting polynomials can be used in non-relativistic and relativistic QM, particularly in the case of the Schrödinger equation and Dirac equations for an electron in a Coulomb potential field.
([1]) The so-called generalized Laguerre equation and polynomials have been wrongly attributed to the French mathematician Edmond Nicolas Laguerre (1834-1886) by Encyclopedia of Mathematics, Encyclopedic Dictionary of Mathematics, Wikipedia, Wolfram MathWorld, and also by many authors of mathematics textbooks and peer-reviewed research articles relating to the classical orthogonal polynomials. Laguerre had nothing to do with such a wrong attribution and the actual discoverer was the Russian mathematician Nikolay Yacovlevich Sonine (1849-1915), see Ref.[14]. ‒Laguerre true and authentic ODEs and polynomials: Laguerre published two seminal articles, respectively, in 1879 Ref.[15] in which he explicitly wrote the equation: x y ″   +   1 + x y ′   − n y = 0 and its polynomial solution; and in his second article published in 1885 Ref.[16] in which he explicitly wrote the equation: xy′′+(x +1−α )y′− ny = 0 and its polynomial solution. As we can see more clearly, the first Eq. is a special case of the second Eq. when α = 0 and both Eqs. are different from xy′′+(1− x)y′+ ny = 0 and xy′′+(α +1− x)y′+ ny = 0 , which are wrongly attributed to Laguerre

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