An Exact Interior Kerr Solution
General Relativity and Quantum Cosmology
2018-05-16 v1
Abstract
We present a simple exact solution for the interior of a rotating star. The interpretation of the stress energy tensor as that of a fluid requires the existence of a high viscosity, which is quite expected for a rotating fluid. In spite of the negative stresses, energy conditions are in fact all satisfied.
Cite
@article{arxiv.1705.06496,
title = {An Exact Interior Kerr Solution},
author = {Aravind P Ravi and Narayan Banerjee},
journal= {arXiv preprint arXiv:1705.06496},
year = {2018}
}
Comments
Two columns; 3 printed pages