Highly accurate calculation of rotating neutron stars: Detailed description of the numerical methods

Details Highly accurate calculation of rotating neutron stars: Detailed description of the numerical methods Highly accurate calculation of rotating neutron stars: Detailed description of the numerical methods

2003-01-10

arxiv.org/abs/astro-ph/0301173v2

Astron.Astrophys.405:711,2003

Astronomy and Astrophysics

Astrophysics

22 pages, 4 figures, 9 tables, version accepted by A&A

Scientific paper

10.1051/0004-6361:20030618

We give a detailed description of the recently developed multi-domain spectral method for constructing highly accurate general-relativistic models of rapidly rotating stars. For both "ordinary" and "critical" configurations, it is exhibited by means of representative examples, how the accuracy improves as the order of the approximation increases. Apart from homogeneous fluid bodies, we also discuss models of polytropic and strange stars.

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