Sure. Bellow the event horizon. Considering the fact that the interior Kerr solution is known to be unstable, and even if it was stable, making use of something located below the event horizon is problematic, this is absolutely useless. What you want are closed curves that pass through an arbitrary point in asymptotically flat space, and you do not get such CTCs with Kerr metric or any other metric known to be stable.
But yes, this is why my first thought was to Kerr metric. Taking the r² slightly
greater than zero allows for a closed space-like curve with all the same properties. So a FTL ship should be capable to keep station at constant t above Cauchy surface. Again, assuming the interior region is stable.
Now, the question is how far we can raise r and still have a closed curve that's traversable by FTL. After all, there are limits to how far we can push Alcubierre Drive. In flat space-time, I can still take a t = constant curve which will have positive ds². But you can't follow that with Alcubierre Drive. You can only push it so far past null curve with finite energy.
I have a feeling event horizon might still end up being a hard cutoff for that and I'd have to come up with something more creative, but I really should just bite the bullet and work this out properly.
George Jones said:
How can a ship move from a timelike curve to a spacelike curve?
By changing parameters in the Alcubierre Metric, presumably via adjusting energy densities required to generate such metric. Assuming we are still talking about an Alcubierre Drive, of course. If you have some other FTL method in mind,
you'd have to tell me how it's done. But in either case, if we are saying that a FTL ship is possible, ability to move from a time-like trajectory to a space-like one is part of what it has to be capable of.P.S. Yeah, for r >> r
s Kerr looks like rotating Schwarzschild, so there is definitely nothing to gain there. If there is going to be anything interesting about FTL near a Kerr black hole, it's going to be in the Ergosphere.