An explanation of the Newman-Janis Algorithm
S. P. Drake P. Szekeres
Abstract
After the original discovery of the Kerr metric, Newman and Janis showed that this solution could be ``derived'' by making an elementary complex transformation to the Schwarzschild solution. The same method was then used to obtain a new stationary axisymmetric solution to Einstein's field equations now known as the Kerr-newman metric, representing a rotating massive charged black hole. However no clear reason has ever been given as to why the Newman-Janis algorithm works, many physicist considering it to be an ad hoc procedure or ``fluke'' and not worthy of further investigation. Contrary to this belief this paper shows why the Newman-Janis algorithm is successful in obtaining the Kerr-Newman metric by removing some of the ambiguities present in the original derivation. Finally we show that the only perfect fluid generated by the Newman-Janis algorithm is the (vacuum) Kerr metric and that the only Petrov typed D solution to the Einstein-Maxwell equations is the Kerr-Newman metric.
Create a lesson
Related papers
Scale-Dependent Weak-Field Dynamics in Horndeski Theory: Galaxy Rotation Curves and Turnaround Scales
Hatice Özer
Mixed-Order Parity-Violating Corrections to Rotating Black Holes in Combined Scalar Gauss-Bonnet and Dynamical Chern-Simons Gravity
Abhishek Rout, Brett Altschul
On the Motion of a Point Electric Charge in the Field of Wu-Yang Monopoles in Bertotti-Robinson Spacetimes
Tekin Dereli, Yorgo Senikoglu
Particle dynamics in rotating charged Bumblebee black holes: An analytical correspondence with Kerr-Newman
Deyou Chen, Chuang Yang
A Unified AI Framework for Rapid and Accurate Waveform Generation of Compact Binary Coalescences
Mengfei Sun, Jin Li, Yuanhong Zhong et al.
Final state of superradiant instability in Einstein-Maxwell-dilaton black hole
Afsaneh Rahmani, Samaneh Oghbaiee