References in periodicals archive ?
Valiente Kroon have developed a method based on properties of the Kerr solution, a time-independent solution to the equations of General Relativity.
By looking at the region outside the black hole we have shown how to ascertain how much a dynamical black hole differs from the Kerr solution.
The Kerr solution, in Boyer-Lindquist coordinates and relativistic units is,
By (47) the correct expression for the Kerr solution (31) is,