This paper is available on arxiv under CC 4.0 license.
Authors:
(1) A. V. Kuzin, Sternberg Astronomical Institute, Moscow, Russia and E-mail: alv.kuzin@gmail.com.
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Model of Disk and Neutron Star
The Solution for the Induced Field
4. THE SOLUTION FOR THE INDUCED FIELD
where A, C may be found easily from boundary conditions.
The problem for u may be solved in the following way. First, we solve the Sturm-Liouville problem with corresponding boundary conditions:
Eigenfunctions of (27) are combinations of Bessel functions of the first and second kind:
while the eigenvalues are roots of the equation:
