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Schwarzschild black hole

Schwarzschild black hole

Main features of a Schwarzschild black hole. Credit: N. Rumiano.


A Schwarzschild black hole is the simplest kind of black hole in theory but one that could never occur in the real universe. A Schwarschild black hole doesn't rotate (i.e. has zero angular momentum), has no electric charge, and exists in a spacetime with no other masses. It arises as an exact solution to Einstein's equations of general relativity worked out by Karl Schwarzschild in 1916.

 

There are three important features of a Schwarzschild black hole:

 

• A photon sphere 1.5 times bigger than the Schwarzschild radius

 

• An event horizon: effectively, the outer surface of the black hole; its distance from the singularity is the Schwarzschild radius

 

• A point singularity where space and time have infinite curvature

 

Compare with Kerr black hole and Reissner-Nordstrom black hole.