Submitted:
16 January 2026
Posted:
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:
factorials
; binomial coefficients
; combinatorial numbers
; non-classical hypergeometric orthogonal polynomials
; non-classical second-order hypergeometric linear DEs
MSC: 05A10; 33C45; 34B30
1. Introduction
Usually, the factorial of a positive integer, denoted by, is defined as the product of all positive integers less than or equal to n: . 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 implies division by zero, and also due to the fact that the usual binomial coefficient 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 , where 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:
It is quite clear that multiplying each integer on the RHS of (1) by the constant is equivalent to multiplying the LHS of (1) by:
Putting in (2) yields
Using the notation to rewrite (3) in the following compact form
As we can see, the relation (4) is, in fact, a special case of
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
Multiplying the two sides of (6) by to get
From (4) and (7), we arrive at the result: in general
Definition 1: We call a factorial number any expression of the form
Result 1: From (1), (4) and (5) we get
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
Replacing with on both sides of (10) to get:
Taking into account Eq.(4) and definition (1), the expression (11) becomes:
Again, replacing with on both sides of (10) yields:
Result 2: From (12) and (13), we get
Finally, replacing and with and , respectively, on both sides of (10) to obtain:
Result 3: Comparing (10) and (15) yields:
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 . 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.
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 of degree n inand :
where x, y are real or complex with n, k∈ℕ and the coefficients are the generalized binomial coefficients (generalized combinatorial numbers). In this sense, where {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 , we make use of (13), (15), and (17) to define the following polynomials:
First, we begin with (18), which can be written in explicit form as follows:
The first few P-polynomials
Derivative formulae for P-polynomial
mth -order partial derivative of w.r.t ,,and, respectively.
where , are the falling factorials and , are the rising factorials.
Characteristic values
Parity
Property
Now, supposing that is fixed by putting and , we get, after substitution in (20), the polynomial of order and degree n in :
The polynomial (26) satisfies the second-order self-adjoint ODE
, for the interesting special case when and , where
4. Non-Classical Hypergeometric Orthogonal Polynomials
The well-known sets of orthogonal polynomials (OPs) such as Jacobi polynomials , Laguerre polynomials [14,15,16], Hermite polynomials , and Bessel polynomials , 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.:
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 thatis fixed, we let and. After substitution in (19), we get:
Replacing with the rising factorial , . We obtain
Where
4.2. Properties of p-polynomials
Characteristic values
p-monomial
We obtain the -monomial for the interesting special case when , that is which satisfies the non-classical second-order hypergeometric linear ODE:
Orthogonality
Now we prove the orthogonality of -polynomials w.r.t the weight function (42) on the interval
(0, ∞). That is to say, we will get if . To this end, let us rewrite Eq.(36) in the following self-adjoint form:
Then by Eq. (45), we get
Multiply (46) by and integrate from to to obtain
Integrating the first integral by parts we get
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 on the interval such that, may be expanded in a series of p-polynomials. More precisely, let us prove that if
this implies
To achieve this, we multiply the series (59) by and integrate from to . Taking into account the previous result, namely the expression (57), we get
For the case when , we have
By taking into account (57), we can derive the expected formula (60) from the above expression.
Illustrative example: Let be a continuous function on the interval such that . Our aim is to find the expansion of in a series of p-polynomials for the interesting case when, i.e., . First, note that , where with and , is the falling factorial, therefore, after substitution in (35), we obtain:
The few first-polynomials for
We have according to (59)
It is clear from the explicit expression of , that is, we should have . Consequently, the above expression becomes
Using the formula (60) to get the following values for the coefficients:,, , . Finally, after substitution, we obtain the requested expansion:
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 , and a is real or complex with n∈ℕ. Therefore, after substitution, the p-polynomials (35) and their ODE (36) become
The first fewp-polynomials for
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
Since both polynomials (63) and (i) have not the same explicit expressions for the recurrence relations and derivative formulae, respectively:
And
This implies, among other things, that they have not the same generating function. Consequently, the polynomials 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 and through the reverse polynomials , which can be easily deduced from (63):
The first few-polynomials
As we can see from (65) and (67), the polynomialsare arranged in descending power order of z while the polynomialsare 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
−polynomials. We now proceed to show that there is actually some link betweenandthrough, which can be rewritten in the following form:
a simple comparison between (i) and (68) leads directly to the expression:
or equivalently
Expressions (69) and (70) mean that the polynomialsare expressible in terms of the polynomialsand vice versa. Moreover, the polynomialsare related to the Hermite ones through:
Because of this, the polynomialscan be arisen in the treatment of the quantum harmonic oscillator.
Associated φ-functions
In terms of the polynomials, we can define the associated φ-functions as:
Using Eq.(64), we get the following self-adjoint DE for φ-functions
Therefore, φ-functions are eigen-functions of a Sturm-Liouville system on the interval (0, ∞).
-polynomials
Now returning to the -polynomials (37), solutions of Eq.(36), and considering the same previous special case, i.e., when , we get after substitution in (37):
or equivalently
which are also solutions of Eq.(64).
The first six-polynomials
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:
where the μ-monomialsor equivalently satisfy Eq.(44).
Now, let us focus our attention exclusively on the κ-polynomials
which satisfy the DE
The first fewκ-polynomials
Generating function forκ-polynomials
Recurrence relation
Derivative formula
Weight function
Laguerre Eq.:
Hermite Eq.:
(iii)
Bessel Eq.
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 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:
such that the coefficients of and are quadratic and/or linear polynomials; and are, respectively, the bi-order and degree of the polynomial solutions of Eq.(29); the characteristic parameter depends on the polynomial's degree ‘n’ and is defined by
The weight function of polynomial solutions is given by
and satisfies the condition
where a and b are the end points of the interval of orthogonality of polynomial solutions and , are real or complex with 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 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 and implies that the sequences and correspond to a unique sequence of polynomial solutions of Eq.(29).
The -polynomials of bi-order and degree in are the highly anticipated ones that satisfy the non-classical second-order hypergeometric linear ODE:
Furthermore, the -polynomials defined by the following explicit formula
are also solutions of Eq.(36).
The first few-polynomials
Generating function forp-polynomials
Recurrence relation
Derivative formula
Weight function
The analogue of Rodrigues' formula
Since, according to (42), we have and with , thus the above expression becomes
In exactly the same way, we can multiply (47) by and integrate by parts from to to obtain
Finally, subtracting (49) from (48), we get the expected orthogonality condition
At present, let us evaluate the integral, that is, the integral (50) for the case when . First, we have
Combining (42) and (43) yields
From (51) and (52), we get
Integration by parts gives
The first term on the RHS is zero, hence by integrating several times by parts, we find
Since and for thus the above integral becomes
From (51) and (56), we obtain the expected expression
Finally, combining (50) and (57), we get
where and is the Kronecker delta defined as .
(77)
The analogue of Ridrogues' formula
(78
The polynomials (75) are related tofor α = ‒ a and β = ‒ n by the following relation:
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:
The analogue of Rodrigues' formula
Characteristic values
Some properties
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.
Then by (89) we have
where .
Now, we multiply (90) by and integrate from to to obtain
Integrating the first integral by parts we get:
By taking into account the explicit expression of the weight function (87), we have
with , thus the above expression becomes:
In exactly the same way we can multiply (91) by and integrate from to to find
Subtracting (93) from (92) and replacing the weight functionby its explicit expression (87) we get the very expected orthogonality condition:
Finally, let us evaluate the integral as follows. First, we have
Secondly, rewriting the generating function in its explicit form
Square and multiply both sides of (96) by the weight function (87) to obtain:
Now, let us focus our attention on the LHS of (97) which can also be written in terms of series as follows:
and after substitution, (97) becomes
with , .
Integrating (98) from z = 0 to z = ∞, we get after simplification
Since and , λ < 0, therefore (99) becomes:
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: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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