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Fractional Integration - Printable Version +- Tetration Forum (https://tetrationforum.org) +-- Forum: Tetration and Related Topics (https://tetrationforum.org/forumdisplay.php?fid=1) +--- Forum: Mathematical and General Discussion (https://tetrationforum.org/forumdisplay.php?fid=3) +--- Thread: Fractional Integration (/showthread.php?tid=1700) Pages:
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RE: Fractional Integration - tommy1729 - 02/09/2023 (02/09/2023, 08:09 AM)Caleb Wrote:(02/08/2023, 06:03 AM)JmsNxn Wrote: These are questions I have asked myself for 12 years There is no unique bijective association with a sequence and a function that solves all matters. You could ask it under conditions and arrive at uniqueness conditions such as Carlsons theorem or other theorems. Or you could ask the function to be entire. Or to have a certain integral transform like a Bernstein function. But it is like interpolation , there is no unique function. And hence no unique analytic continuation because it depends on what type of function you associate. And there is no unique fractional integral or integration constant for the same reasons. In general we use properties like the y the derivative of exp(x) is exp(x) and from there we can define fractional integration. Series expansion and distributive property are then key. Your questions appear to me to be too general to give a full or better answer. But maybe I missed something in your questions ? Regards tommy1729 RE: Fractional Integration - JmsNxn - 02/10/2023 Hey, Caleb; both of your solutions are unintegrable. And there is no interpolation for \(\frac{1}{n!}\). What happens is very different. For \(A(z)\) to be a FRactional Calculus interpolation of \(a_n\); it must be that: \[ A(z) = \frac{d^z}{dw^z}\Big{|}_{w=0} \sum_{n=0}^\infty a_n \frac{w^n}{n!}\\ \] End of story; where in this space, the bounds are pretty much \(A(z)\) is holomorphic for at least \(\Re(z) \ge 0\) and satisfies \(A(z) = O(e^{\rho |\Re(z)| + \tau|\Im(z)|})\) for \(0 \le \tau < \pi/2\). The reason, you find the \(1/n!\) in this camp is a much more difficult idea. \[ \Gamma(z) = \sum_{n=0}^\infty \frac{(-1)^n}{n!(n+z)} + h(z)\\ \] Where \(h\) is entire. So the reason you are seeing these factorials, is because you are seeing them as residues of the Gamma function. Not because you are flipping the Gamma function on it's head. I should've added, because I made a mistake, that the integral is in the opposite sign (man I am making too many sign mistakes lately );\[ f(w) = \frac{1}{2\pi i} \int_{c-i\infty}^{c+i\infty} w^{-z}\Gamma(z) \frac{d^{-z}}{dw^{-z}}\Big{|}_{w=0} f(w)\,dz \] Whereupon: \[ f(w) = \sum_{n=0}^\infty f^{(n)}(0) \frac{(-w)^n}{n!}\\ \] The \(1/n!\) you are seeing are actually the RESIDUES of the Gamma function. Not the gamma function itself. If you want to instead write: \[ \Gamma(z)\frac{d^{-z}}{dw^{-z}}\Big{|}_{w=0} f(w) = B(-z)\\ \] Where \(c_n = \frac{f^{(n)}(0)(-1)^n}{n!}\): \[ B(-z) = \sum_{n=0}^\infty c_n\frac{(-1)^n}{(n+z)} + h(z)\\ \] Then the equation reads as: \[ f(w) = \frac{1}{2\pi i} \int_{c-i\infty}^{c+i\infty} w^{-z}B(-z)\,dz \] And lastly, but not least; we can write it as Ramanujan would; which inspired Carlson: \[ f(w) = \sum_{n=0}^\infty c_n (-w)^n\\ \] \[ \int_0^\infty f(w)w^{z-1}\,dw = \frac{\pi C(-z)}{\sin \pi z}\\ \] And: \[ f(w) = \frac{1}{2\pi i} \int_{c-i\infty}^{c+i\infty} w^{-z}\frac{\pi C(-z)}{\sin \pi z}\,dz\\ \] Where now, we solely ask that \(C(z) = O(e^{\rho|\Re(z)|+\kappa|\Im(z)|})\) but \(0 \le \kappa < \pi\), rather than the half. And \(C(n) = c_n\). A lot of what's going on under the hood; when nature chooses the Gamma function; is this operation. You find it with Bernoulli numbers, all the way to zeta functions... |