The deformed figures of the Dedekind ellipsoids in the post-Newtonian approximation to general relativity - Corrections and amplifications

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Ellipsoids, Newton Theory, Relativity, Velocity Distribution, Boundary Value Problems, Gravitational Fields, Harmonic Oscillation, Linear Equations, Pressure Distribution

Scientific paper

Two errors in the analysis of an earlier paper on the same subject are corrected. It is found that as a consequence of the corrections, the solution to the post-Newtonian equations (appropriate to determining the deformed figures of the Dedekind ellipsoid) now diverges at a point where the axes of the ellipsoid are in the ratios 1:0.3370:0.2850. In addition, the fourth-harmonic oscillations of the Dedekind ellipsoid are considered. It is found that it becomes dynamically unstable when its axes are in the ratios 1:0.3121:0.2680.

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