Schwarzschild radius

The Schwarzschild radius or the gravitational radius is a physical parameter in the Schwarzschild solution to Einstein's field equations that corresponds to the radius defining the event horizon of a Schwarzschild black hole. It is a characteristic radius associated with any quantity of mass. The Schwarzschild radius was named after the German astronomer Karl Schwarzschild, who calculated this exact solution for the theory of general relativity in 1916.

The Schwarzschild radius is given as $r_{\text{s}}={\frac {2GM}{c^{2}}},$ where G is the gravitational constant, M is the object mass, and c is the speed of light.^{[note 1]}^[1]^[2]

Cite error: There are <ref group=note> tags on this page, but the references will not show without a {{reflist|group=note}} template (see the help page).

^ Kutner, Marc (2003). Astronomy: A Physical Perspective. Cambridge University Press. p. 148. ISBN 9780521529273.
^ Guidry, Mike (3 January 2019). Modern General Relativity: Black Holes, Gravitational Waves, and Cosmology. Cambridge University Press. p. 92. ISBN 978-1-107-19789-3.

[2] Kutner, Marc (2003). Astronomy: A Physical Perspective. Cambridge University Press. p. 148. ISBN 9780521529273.

[3] Guidry, Mike (3 January 2019). Modern General Relativity: Black Holes, Gravitational Waves, and Cosmology. Cambridge University Press. p. 92. ISBN 978-1-107-19789-3.

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