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2.4 Answer to the Unsolved Puzzle

What is wrong with treating c as infinity? Negligence of the relative power of c and n to asymptotic infinity drives an incorrect conclusion in (2.17), that all of the weighting factor {{w}_{i}} is one, and thus \underset{n\to \infty }{\mathop{\lim }}\,\sum\limits_{i=1}^{n}{{{w}_{i}}{{\beta }_{i}}} approaches infinity. As (2.14) indicates, for any given value of c, we can always find a larger number N that makes {w}_{N+j}, where j\in {{\mathbb{Z}}^{+}_{0}}, approach 0. By taking a derivative, we know that the integrand function {{x}^{N}}\exp(-x) has the maximum value at x=N. Thus, the integral value at \left[ 0,c \right] as a ratio of the same integral value at the overall domain \left[ 0,\infty \right] will approach 0 if c\ll N. This means, {w}_{i} cannot always be one because N will eventually overpower c in creating the weighting factor.

This conclusion explains why the infinite series based on the Taylor series (1.2) or Kummer's confluent hypergeometric function (1.4) was not widely recognized as a solution to the gamma integral. Employing the "h" factorization method, we can actually establish the identity between "h" and the gamma function, with an understanding that the infinite upper limit c should be regarded as a finite number. Once we realize the finite property of c, we are on firm ground to understand the "h" factorization method presented in (2.2) as a general solution to the gamma integral.

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