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Surface gravity

The surface gravity κ of a Killing horizon is the acceleration, as exerted at infinity, needed to keep an object at the horizon. Mathematically, if ka is a suitably normalized Killing vector, then the surface gravity is defined by

k^a \nabla_a k^b = \kappa k^b,

where the equation is evaluated at the horizon. For a static and asymptotically flat spacetime, the normalization should be chosen so that k^a k_a \rightarrow -1 as r\rightarrow\infty, and so that \kappa \geq 0. For the Schwarzschild solution, we take ka to be the time translation Killing vector k^a\partial_a = \frac{\partial}{\partial t}, and more generally for the Kerr-Newman solution we take k^a\partial_a = \frac{\partial}{\partial t}+\Omega\frac{\partial}{\partial\phi}, the linear combination of the time translation and axisymmetry Killing vectors which is null at the horizon, where Ω is the angular velocity.

Examples

The Schwarzschild solution

The surface gravity for the Schwarzschild solution with mass M is

\kappa = \frac{1}{4M}.

The Kerr-Newman solution

The surface gravity for the Kerr-Newman solution is

\kappa = \frac{r_+-r_-}{2(r_+^2+a^2)} = \frac{\sqrt{M^2-Q^2-J^2/M^2}}{2M^2-Q^2+2M\sqrt{M^2-Q^2-J^2/M^2}},

where Q is the electric charge, J is the angular velocity, we define r_\pm := M \pm \sqrt{M^2-Q^2-J^2/M^2} to be the locations of the two horizons and a: = J / M.

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