The paper introduces new type degenerate Simsek numbers defined via a degenerate exponential generating function and the falling factorial, establishing explicit formulas.
Key methodology employs Stirling numbers and binomial expansions to transform monomials and relate the new numbers to classical combinatorial sequences.
Implications include potential applications in colored set partitions and deformed probability distributions, with open problems on combinatorial interpretations and asymptotic behavior.
New type degenerate Simsek numbers are a family of special numbers introduced through a degenerate exponential generating function that differs from the degenerate Simsek numbers studied previously. For parameters α,λ∈C and indices n,k∈N0, the numbers are denoted by y1,α∗(n,k;λ) and are defined in terms of the degenerate falling factorial. The construction yields explicit formulas, recurrence relations, and identities linking the new family to Stirling numbers, classical Simsek numbers, higher-order Bernoulli numbers, and degenerate Apostol–Euler numbers (Oussi, 14 Aug 2025).
1. Definition through the degenerate generating function
Let
(x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).
This is the degenerate falling factorial used throughout the theory.
The new type degenerate Simsek numbers y1,α∗(n,k;λ) are defined by
k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.
Equivalently, with
Fk(t;α,λ):=k!(λet+1)k,α,
one has
Fk(t;α,λ)=n=0∑∞y1,α∗(n,k;λ)n!tn.
The initial values follow immediately:
y1,α∗(0,k;λ)=k!(λ+1)k,α,y1,α∗(n,0;λ)=δn,0.
In this form, the family is indexed simultaneously by the coefficient order n and the upper parameter n,k∈N00, producing a triangular array analogous to other special-number tables in combinatorial and analytic number theory (Oussi, 14 Aug 2025).
2. Coefficient extraction and explicit formulas
The generating function is expanded by rewriting the degenerate factorial in shifted form:
n,k∈N01
where n,k∈N02 is the ordinary falling factorial. The ordinary falling factorial is then expanded via Stirling numbers of the first kind:
n,k∈N03
Each power is subsequently expanded by the binomial theorem:
n,k∈N04
Comparing coefficients yields the principal explicit formula:
n,k∈N05
This formula exhibits the new type degenerate Simsek numbers as a double Stirling–binomial transform of the monomials n,k∈N06.
A second explicit form follows from the convolution identity
n,k∈N07
leading to
n,k∈N08
These identities show that the new family is algebraically controlled by the interaction between degeneracy, encoded by n,k∈N09, and Stirling-type basis changes (Oussi, 14 Aug 2025).
3. Recurrence structure
The paper establishes two recurrence relations, one in the upper index y1,α∗(n,k;λ)0 and one in the lower index y1,α∗(n,k;λ)1.
For y1,α∗(n,k;λ)2, the recurrence in y1,α∗(n,k;λ)3 is
y1,α∗(n,k;λ)4
This is obtained from the functional relation
y1,α∗(n,k;λ)5
by coefficient comparison.
For y1,α∗(n,k;λ)6, the recurrence in y1,α∗(n,k;λ)7 is
y1,α∗(n,k;λ)8
with boundary condition
y1,α∗(n,k;λ)9
This relation is derived by differentiating the (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).0 functional equation with respect to (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).1 and comparing coefficients.
The recurrences are computationally significant because they provide two complementary ways to generate the triangular array: one by stepping in (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).2, the other by stepping in (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).3. The data also states that, in practice, one computes each row either by the recurrence above or by the double-sum explicit formula (Oussi, 14 Aug 2025).
4. Structural identities and links with Stirling-type arrays
A central identity relates the new type degenerate Simsek numbers to Stirling numbers of the first kind:
(x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).4
where
(x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).5
The family is also connected to degenerate Stirling numbers of the second kind (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).6 and to the original Simsek numbers (x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).7 through
(x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).8
A further identity links the numbers to the new-type degenerate Stirling numbers
(x)0,α=1,(x)n,α=x(x−α)(x−2α)⋯(x−(n−1)α)(n≥1).9:
y1,α∗(n,k;λ)0
These formulas place y1,α∗(n,k;λ)1 within a network of Stirling-type transforms. In particular, the construction is not isolated: it is tied to both first-kind and second-kind degenerate Stirling numbers, and it interpolates back to the original Simsek numbers via explicit coefficient identities rather than only by limiting arguments (Oussi, 14 Aug 2025).
5. Relations with Bernoulli and Apostol–Euler families
The generating function admits a reformulation in terms of Bernoulli polynomials of order y1,α∗(n,k;λ)2:
y1,α∗(n,k;λ)3
Accordingly, the numbers y1,α∗(n,k;λ)4 can be written in terms of the higher-order Bernoulli numbers y1,α∗(n,k;λ)5.
The paper also introduces degenerate Apostol–Euler numbers of order y1,α∗(n,k;λ)6 through
y1,α∗(n,k;λ)7
From a mixed generating function in y1,α∗(n,k;λ)8 and an auxiliary variable y1,α∗(n,k;λ)9, it derives bilinear relations between k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.0, k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.1, and the numbers k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.2.
These relations indicate that the new type degenerate Simsek numbers participate in a broader algebra of degenerate special functions. The Bernoulli and Apostol–Euler links are structural rather than merely formal: they arise from direct generating-function manipulations and coefficient comparison (Oussi, 14 Aug 2025).
6. Special cases, limiting behavior, and representative values
Several specializations are given explicitly.
For k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.3,
k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.4
More generally, since
k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.5
one recovers the classical Simsek numbers:
k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.6
For k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.7,
k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.8
which the source describes as a symmetric function in k!(λet+1)k,α=n=0∑∞y1,α∗(n,k;λ)n!tn.9.
As Fk(t;α,λ):=k!(λet+1)k,α,0,
Fk(t;α,λ):=k!(λet+1)k,α,1
The source also states a classical recovery: if one further sets Fk(t;α,λ):=k!(λet+1)k,α,2 after Fk(t;α,λ):=k!(λet+1)k,α,3, one recovers the ordinary Lah numbers or other special triangular arrays. A plausible implication is that the family interpolates among several known combinatorial tables, although the exact route depends on the order of specialization.
Representative values given explicitly include
Fk(t;α,λ):=k!(λet+1)k,α,4
The source notes that further entries for Fk(t;α,λ):=k!(λet+1)k,α,5 and Fk(t;α,λ):=k!(λet+1)k,α,6 may be filled in from the recurrences or from the double-sum formula (Oussi, 14 Aug 2025).
7. Interpretive status, applications, and open problems
The paper distinguishes established identities from conjectural or prospective interpretations. It does not provide a direct combinatorial interpretation of Fk(t;α,λ):=k!(λet+1)k,α,7; rather, by analogy with Simsek’s use of negative-order Euler polynomials, it states that one expects these numbers to count, up to weights, a family of colored set-partitions with a degeneracy parameter Fk(t;α,λ):=k!(λet+1)k,α,8. A precise bijection remains open.
Potential applications are also framed prospectively. The numbers are said to enter naturally into expansions of degenerate exponential generating functions of the form
Fk(t;α,λ):=k!(λet+1)k,α,9
which appear in deformations of Poisson and negative-binomial distributions. The source further indicates that they may be useful in interpolating the Apostol–Euler polynomials of negative order.
The open problems listed are specific: finding a direct combinatorial model, extending the theory to a two-parameter Fk(t;α,λ)=n=0∑∞y1,α∗(n,k;λ)n!tn.0-degenerate version, and investigating the zeros and asymptotics of the triangle Fk(t;α,λ)=n=0∑∞y1,α∗(n,k;λ)n!tn.1. These directions underscore an important point about the present state of the subject: the analytic and algebraic framework is already explicit, whereas the combinatorial semantics and asymptotic theory remain undeveloped (Oussi, 14 Aug 2025).
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