 Distorted Schwarzschild metric

The Distorted Schwarzschild metric is a solution to the Einstein field equations of general relativity that describes the spacetime geometry around a gravitating mass, particularly in scenarios where the symmetry of the Schwarzschild solution, which describes a perfect spherical non-rotating mass, is disrupted by some additional factors. This could include the effects of matter distribution, rotation, or other gravitational influences that cause deviations from the standard Schwarzschild solution.