User:Tohline/MathProjects/EigenvalueProblemN1
Find Analytic Solutions to an Eigenvalue Problem
|
|---|
| | Tiled Menu | Tables of Content | Banner Video | Tohline Home Page | |
Note from J. E. Tohline to Students with Good Mathematical Skills: This is one of a set of well-defined research problems that are being posed, in the context of this online H_Book, as challenges to young, applied mathematicians. The astronomy community's understanding of the Structure, Stability, and Dynamics of stars and galaxies would be strengthened if we had, in hand, a closed-form analytic solution to the problem being posed here. (A solution can be obtained numerically with relative ease, but here the challenge is to find a closed-form analytic solution.) As is true with most meaningful scientific research projects, it is not at all clear whether this problem has a solution. In my judgment, however, it seems plausible that a closed-form solution can be discovered and such a solution would be of sufficient interest to the astronomical community that it would likely be publishable in a professional astronomy or physics journal. At the very least, this project offers an opportunity for a graduate student, an undergraduate, or even a talented high-school student (perhaps in connection with a mathematics science fair project?) to hone her/his research skills in applied mathematics. Also, I would be thrilled to include a solution to this problem — along with full credit to the solution's author — as a chapter in this online H_Book. Having retired from LSU, I am not in a position to financially support or formally advise students who are in pursuit of a higher-education degree. I would nevertheless be interested in sharing my expertise — and, perhaps, developing a collaborative relationship — with individuals who are interested in pursuing an answer to the mathematical research problem that is being posed here.
The Challenge
Formally, this is an eigenvalue problem. Find one or more analytic expression(s) for the (eigen)function, <math>~\mathcal{G}_\sigma(x)</math> — and, simultaneously, the value of the (eigen)frequency, <math>~\sigma</math> — that satisfies the following 2nd-order, ordinary differential equation:
<math>
(x^2\sin x ) \frac{d^2\mathcal{G}_\sigma}{dx^2} + 2 \biggl[ x \sin x + x^2 \cos x \biggr] \frac{d\mathcal{G}_\sigma}{dx} +
\biggl[ \sigma^2 x^3 - 2\alpha ( \sin x - x\cos x ) \biggr] \mathcal{G}_\sigma = 0 \, ,
</math>
where, <math>~\alpha</math> is a constant.
Related Discussions
|
|
|---|
|
© 2014 - 2021 by Joel E. Tohline |