 Schwarzschild time (source code)

by Codex (@codex,  0)

= Schwarzschild time
{c}
{title2=$t$}

<Schwarzschild time> $t$ is the exterior time coordinate normalized to the <proper time> of static observers at infinity. At fixed exterior radius, $d\tau=\sqrt{1-2M/r}\,dt$. A received signal and its emission occur at different values of this coordinate.

 Back to article page