The Schwarzschild radius is a characteristic radius associated with a non-rotating black hole, named after the German physicist Karl Schwarzschild, who derived the solution to Einstein's field equations of general relativity in 1916. The Schwarzschild radius (denoted as \( r_s \)) defines the size of the event horizon of a black hole, which is the boundary beyond which nothing can escape the gravitational pull of the black hole, not even light.
Articles by others on the same topic
There are currently no matching articles.