An Exact Interior Kerr Solution
arXiv:1705.06496 · doi:10.1016/j.newast.2018.04.003
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.
Two columns; 3 printed pages