An approximate global stationary axisymmetric solution of the Einstein equations

2004/07/05 by J. Martin-Martin, A. Molina, Martin-Martin, J. +3
Mathematics · Physics and Astronomy · #Algebraic and Geometric Analysis #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/0407016

12 pages, LaTeX, conference done at Spanish Relativity Meeting (Alicante, Spain, 2003). A few minor errata have been corrected. A formula for pressure is also added

openalex publication_date 2004/07/05 · arxiv created 2004/08/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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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