Abstract
We establish a new identity for generalized hypergeometric functions and apply it for first- and second-kind Gauss summation formulas to obtain some new summation formulas. The presented identity indeed extends some results of the recent published paper (Some summation theorems for generalized hypergeometric functions, Axioms, 7 (2018), Article 38).
Keywords:
generalized hypergeometric functions; Gauss and confluent hypergeometric functions; summation theorems of hypergeometric functions MSC:
33C20; 33C05; 65B10
1. Introduction
Let and denote the sets of real and complex numbers and z be a complex variable. For real or complex parameters a and b, the generalized binomial coefficient
in which
denotes the well-known gamma function for , can be reduced to the particular case
where denotes the Pochhammer symbol [1] given by
By referring to the symbol (1), the generalized hypergeometric functions [2]
are indeed a Taylor series expansion for a function, say f, as with for which the ratio of successive terms can be written as
According to the ratio test [3,4], the series (2) is convergent for any . In fact, it converges in for , converges everywhere for and converges nowhere () for . Moreover, for it absolutely converges for if the condition
holds and is conditionally convergent for and if and is finally divergent for and if .
There are two important cases of the series (2) arising in many physics problems [5,6]. The first case (convergent in ) is the Gauss hypergeometric function
with the integral representation
Replacing in (3) directly leads to the well-known Gauss identity
The second case, which converges everywhere, is the Kummer confluent hypergeometric function
with the integral representation
In this paper, we explicitly obtain the simplified form of the hypergeometric series
when are two natural numbers and .
2. A New Identity for Generalized Hypergeometric Functions
In [7], two particular cases of (6) for and were considered and other cases have been left as open problems. In this section, we wish to consider those open problems and solve them for any arbitrary value of m. For this purpose, since
relation (6) is simplified as
It is clear in (7) that
To evaluate , we can directly use Chu-Vandermonde identity, which is a special case of Gauss identity (4), i.e.,
Now if in (9), and , we have
Hence, replacing (10) in gives
It is important to note in the second equality of (11) that for any . Therefore, the lower index is starting from instead of . Now since
relation (11) is simplified as
Finally, by noting the identity
the main result of this paper is obtained as follows.
Main Theorem.If are two natural numbers so that , then
where and .
3. Some Special Cases of the Main Theorem
Essentially whenever a generalized hypergeometric series can be summed in terms of gamma functions, the result will be important as only a few such summation theorems are available in the literature. In this sense, the classical summation theorems such as Kummer and Gauss for , Dixon, Watson, Whipple and Pfaff-Saalschutz for , Whipple for , Dougall for and Dougall for are well known [1,10]. In this section, we consider some special cases of the above main theorem to obtain new hypergeometric summation formulas.
Special case 1. Note that if , the first equality of (13) reads as
Hence, the main theorem is simplified as
which is a known result in the literature [10] (p. 439).
Special case 2. For , relation (13) gives and the main theorem therefore reads (for ) as
For instance, we have [7]
As a very particular case, replacing and in the above relation yields
Special case 3. For , the main theorem is simplified as
For instance, by referring to the special case 1, we have [7,10]
Special case 4. For and , the main theorem is simplified as
in which we have used the relation . For instance, by referring to the special case 1, we have [7,10]
Special case 5. For and , the main theorem is simplified as
As a particular case and by noting the first kind of Gauss formula (4), if is replaced in (15) then we get
Therefore, we get
As a numerical example for the result (16), we have
It is clear that the right-hand side of this equality can be easily computed and therefore the infinite series in the left-hand side has been evaluated.
Author Contributions
Both authors have contributed the same amout in all sections.
Funding
The work of the first author has been supported by the Alexander von Humboldt Foundation under the grant number: Ref 3.4-IRN-1128637-GF-E.
Conflicts of Interest
The authors declare no conflict of interest.
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