Spatial potential of a weakly compressed elliptical disk
- Authors: Kondratyev B.P.1,2
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Affiliations:
- Sternberg Astronomical Institute
- Pulkovo Astronomical Observatory
- Issue: Vol 61, No 7 (2016)
- Pages: 1097-1100
- Section: Short Communications
- URL: https://journal-vniispk.ru/1063-7842/article/view/197626
- DOI: https://doi.org/10.1134/S1063784216070161
- ID: 197626
Cite item
Abstract
The problem of expanding spatial potential in terms of eccentricity e accurate to e2 has been formulated and solved for a homogeneous gravitating (or charged with static electric charge) elliptical disk. An original method that makes it possible to obtain the desired result using the superposition of a perturbation layer and a circular disk has been developed. The potential of such a layer has been derived. The first term of the expansion of the potential (zero power of parameter e) coincides with the potential of a homogeneous circular disk and the coefficient of the first power of the parameter e is zero. The main term of the expansion of the potential proportional to e2 is analytically derived. The resulting expression makes it possible to determine the potential in the entire space, including the inner region of the disk.
About the authors
B. P. Kondratyev
Sternberg Astronomical Institute; Pulkovo Astronomical Observatory
Author for correspondence.
Email: work@boris-kondratyev.ru
Russian Federation, Universitetskii pr. 13, Moscow, 119991; Pulkovskoe sh. 65/1, St. Petersburg, 196140
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