The Reissner-Nordström metric describes the geometry of spacetime around a charged, non-rotating black hole. It extends the static Schwarzschild solution by incorporating electric charge, allowing it to model the effects of electromagnetic fields in addition to gravitational forces. The metric is characterized by two parameters: the mass of the black hole and its electric charge .
Mathematically, the Reissner-Nordström metric is expressed in Schwarzschild coordinates as:
where
This solution reveals important features such as the presence of two event horizons for charged black holes, known as the outer and inner horizons, which are critical for understanding the black hole's thermodynamic properties and stability. The Reissner-Nordström metric is fundamental in the study of black hole thermodynamics, particularly in the context of charged black holes' entropy and Hawking radiation.
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