Stability of Reissner-Nordström Black Hole

Abstract

The singularity of the solutions obtained before in the teleparallel theory of gravitation is studied. Also the stability of these solutions is studied using the equations of geodesic deviation. The condition of stability is obtained. From this condition the stability of the Schwarzschild solution can be obtained.

Reissner-Nordström Uzay-zaman Geometrisinde Burgers modelleri için Şok ve Seyrelme Dalgalarının Yayılımı

“…Godunov semaları ile ilgili detaylar için Guinot [6], Leveque [12] ve Van Leer [14] kaynak gösterilebilir. Son olarak genel görelilik teorisi ve uzay-zaman geometrisi ile ilgili olarak da [1,11,13,15] referanslarına bakılabilir.…”

Singularity transition in a Yukawa-Reissner-Nordström spacetime

“…This configuration is a solution of Einstein-Maxwell field equations, corresponding to the gravitational field caused by a charged non-rotating mass [3]. An important aspect of this gravitational scenario is the absence of a single horizon by the presence of a double singularity [23][24][25]. In the tereparallel formalism [27][28][29] the description of such a spacetime is appropriate the use of tetrad fields.…”