Kapteyn series

Kapteyn series is a series expansion of analytic functions on a domain in terms of the Bessel function of the first kind. Kapteyn series are named after Willem Kapteyn, who first studied such series in 1893.[1][2] Let ${\displaystyle f}$ be a function analytic on the domain

${\displaystyle D_{a}=\left\{z\in \mathbb {C} :\Omega (z)=\left|{\frac {z\exp {\sqrt {1-z^{2}}}}{1+{\sqrt {1-z^{2}}}}}\right|\leq a\right\}}$

with ${\displaystyle a<1}$. Then ${\displaystyle f}$ can be expanded in the form

${\displaystyle f(z)=\alpha _{0}+2\sum _{n=1}^{\infty }\alpha _{n}J_{n}(nz)\quad (z\in D_{a}),}$

where

${\displaystyle \alpha _{n}={\frac {1}{2\pi i}}\oint \Theta _{n}(z)f(z)dz.}$

The path of the integration is the boundary of ${\displaystyle D_{a}}$. Here ${\displaystyle \Theta _{0}(z)=1/z}$, and for ${\displaystyle n>0}$, ${\displaystyle \Theta _{n}(z)}$ is defined by

${\displaystyle \Theta _{n}(z)={\frac {1}{4}}\sum _{k=0}^{\left[{\frac {n}{2}}\right]}{\frac {(n-2k)^{2}(n-k-1)!}{k!}}\left({\frac {nz}{2}}\right)^{2k-n}}$

Kapteyn's series are important in physical problems. Among other applications, the solution ${\displaystyle E}$ of Kepler's equation ${\displaystyle M=E-e\sin E}$ can be expressed via a Kapteyn series:[2][3]

${\displaystyle E=M+2\sum _{n=1}^{\infty }{\frac {\sin(nM)}{n}}J_{n}(ne).}$

Relation between the Taylor coefficients and the α_n coefficients of a function

Let us suppose that the Taylor series of ${\displaystyle f}$ reads as

${\displaystyle f(z)=\sum _{n=0}^{\infty }a_{n}z^{n}.}$

Then the ${\displaystyle \alpha _{n}}$ coefficients in the Kapteyn expansion of ${\displaystyle f}$ can be determined as follows.[4]: 571 

${\displaystyle {\begin{aligned}\alpha _{0}&=a_{0},\\\alpha _{n}&={\frac {1}{4}}\sum _{k=0}^{\left\lfloor {\frac {n}{2}}\right\rfloor }{\frac {(n-2k)^{2}(n-k-1)!}{k!(n/2)^{(n-2k+1)}}}a_{n-2k}\quad (n\geq 1).\end{aligned}}}$

Examples

The Kapteyn series of the powers of ${\displaystyle z}$ are found by Kapteyn himself:[1]: 103,  [4]: 565 

${\displaystyle \left({\frac {z}{2}}\right)^{n}=n^{2}\sum _{m=0}^{\infty }{\frac {(n+m-1)!}{(n+2m)^{n+1}\,m!}}J_{n+2m}\{(n+2m)z\}\quad (z\in D_{1}).}$

For ${\displaystyle n=1}$ it follows (see also [4]: 567 )

${\displaystyle z=2\sum _{k=0}^{\infty }{\frac {J_{2k+1}((2k+1)z)}{(2k+1)^{2}}},}$

and for ${\displaystyle n=2}$ [4]: 566 

${\displaystyle z^{2}=2\sum _{k=1}^{\infty }{\frac {J_{2k}(2kz)}{k^{2}}}.}$

Furthermore, inside the region ${\displaystyle D_{1}}$,[4]: 559 

${\displaystyle {\frac {1}{1-z}}=1+2\sum _{k=1}^{\infty }J_{k}(kz).}$

See also

• Schlömilch's series

References

1. Kapteyn, W. (1893). Recherches sur les functions de Fourier-Bessel. Ann. Sci. de l’École Norm. Sup., 3, 91-120.
2. Baricz, Árpád; Jankov Maširević, Dragana; Pogány, Tibor K. (2017). "Series of Bessel and Kummer-Type Functions". Lecture Notes in Mathematics. Cham: Springer International Publishing. doi:10.1007/978-3-319-74350-9. ISBN 978-3-319-74349-3. ISSN 0075-8434.
3. Borghi, Riccardo (2021). "Solving Kepler's equation via nonlinear sequence transformations". arXiv:2112.15154 [math.CA].
4. Watson, G. N. (2011-06-06). A treatise on the theory of Bessel functions (1944 ed.). Cambridge University Press. OL 22965724M.