Highly accurate calculation of rotating neutron stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages, submitted to Astronomy & Astrophysics

Scientific paper

10.1051/0004-6361:20011643

A new spectral code for constructing general-relativistic models of rapidly rotating stars with an unprecedented accuracy is presented. As a first application, we reexamine uniformly rotating homogeneous stars and compare our results with those obtained by several previous codes. Moreover, representative relativistic examples corresponding to highly flattened rotating bodies are given.

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