Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University
ApJ, 777-60 (2013)
We derive a family of post-Newtonian (PN) Dedekind ellipsoids to first order. They describe non-axially symmetric,
homogeneous, and rotating figures of equilibrium. The sequence of the Newtonian Dedekind ellipsoids allows for
an axially symmetric limit in which a uniformly rotating Maclaurin spheroid is recovered. However, the approach
taken by Chandrasekhar & Elbert to find the PN Dedekind ellipsoids excludes such a limit. In a previous work,
we considered an extension to their work that permits a limit of 1 PN Maclaurin ellipsoids. Here we further detail
the sequence and demonstrate that a choice of parameters exists with which the singularity formerly found by
Chandrasekhar & Elbert along the sequence of PN Dedekind ellipsoids is removed.
gravitation – relativistic processes – stars: general – stars: kinematics and dynamics – stars: neutron
@article{UTF529,
author = {Gurlebeck, N. and Petroff, D.},
title = {{A GENERALIZED FAMILY OF POST-NEWTONIAN DEDEKIND ELLIPSOIDS}},
journal = {ApJ},
pages = {777-60},
year = {2013},
doi = {10.1088/0004-637X/777/1/60},
}