Short-cut method of solution of geodesic equations for Schwarzchild black hole
Jean-Alain Marck; Jean-Alain Marck; Département d'Astrophysique Relativiste et de Cosmologie (UPR 176 du CNRS), Observatoire de Paris - section de Meudon, F-92195 Meudon Cédex, France
Журнал:
Classical and Quantum Gravity
Дата:
1996-03-01
Аннотация:
It is shown how the use of the Kerr - Schild coordinate system can greatly simplify the formulation of the geodesic equation of the Schwarzschild solution. An application of this formulation to the numerical computation of the aspect of a non-rotating black hole is presented. The generalization to the case of the Kerr solution is also presented. 0470B, 9760L
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