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
,
where the equation is evaluated at the horizon. For a static and asymptotically flat spacetime, the normalization should be chosen so that
as
, and so that
. For the Schwarzschild solution, we take ka to be the time translation Killing vector
, and more generally for the Kerr-Newman solution we take
, 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
.
The Kerr-Newman solution
The surface gravity for the Kerr-Newman solution is
,
where Q is the electric charge, J is the angular velocity, we define
to be the locations of the two horizons and a: = J / M.