An approximate global stationary axisymmetric solution of the Einstein equations
classification
🌀 gr-qc
keywords
approximateaxisymmetriceinsteinequationsglobalsolutionstationaryangular
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.