An approximate global stationary axisymmetric solution of the Einstein equations
General Relativity and Quantum Cosmology
2007-05-23 v2
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.
Cite
@article{arxiv.gr-qc/0407016,
title = {An approximate global stationary axisymmetric solution of the Einstein equations},
author = {J. Martin-Martin and A. Molina and E. Ruiz},
journal= {arXiv preprint arXiv:gr-qc/0407016},
year = {2007}
}
Comments
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