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This paper presents an intuitive derivation of the Kerr metric using an orthogonal metric ansatz with ellipsoidal symmetry, aiming to simplify the understanding of its derivation for students. The authors compare the Kerr metric to the Schwarzschild solution, highlighting key differences and proposing a method to derive the Kerr solution by maintaining the symmetry of the ellipsoidal space-time. The paper concludes with a system of equations that can be solved to obtain the desired metric for a rotating bod

Author

Eloan França

Language

EN