A perfect-fluid spacetime for a slightly deformed mass
classification
🌀 gr-qc
keywords
deformedmassaccountapproximatedeformationdescribedistributioneinstein
read the original abstract
We present approximate exterior and interior solutions of Einstein's equations which describe the gravitational field of a static deformed mass distribution. The deformation of the source is taken into account up to the first order in the quadrupole.
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.