How can we derive the event horizon from a metric dependant on $(t,x,y,z)$? I've seen the Schwarzschild solution and the Kerr solution, but both of these are given in $(t,r,θ,φ)$. I tried converting them from $x,y,z$ to $r$ (keeping $θ$ and $φ$ constant along with $t$)
The problem is I can't use the same method as with Kerr and/or Schwarzschild because the $g_{xx}=g_{yy}=g_{zz}$ is still $(1+M/2r)^4$ which only goes to infinity at $r=0$ (there is no incoherence in the coordinates like in the Schwarzschild solution)... And I can't use the sign and say from that point on is timelike and before it, it's spacelike, so the light cone is tilted towards the interior when r<(event horizon).
There is no sign to change, the term it is in the fourth power. I just don't know where to begin I suppose, everywhere I've searched the only mathematical definitions of the event horizon I could find are those two and they don't seem to apply here.
I just need a point to begin.