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An approximate global stationary axisymmetric solution of the Einstein equations

J. Martin-Martin·A. Molina·E. Ruiz
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Abstract

In this work we present an approximate solution of the Einstein equations describing a global model for the gravitational field generated by a bounded, self-gravitating stationary and axisymmetric body rotating rigidly with constant angular velocity.

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J. Martin-Martin, A. Molina, E. Ruiz. 2004-08-30. An approximate global stationary axisymmetric solution of the Einstein equations. https://arxiv.org/abs/gr-qc/0407016

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