yuiop said:
One point of view is that the lower end of the cylinder will stop rotating when it arrives at the event horizon, but will this halt in rotation be transmitted up the cylinder so that our stationary observer outside the event horizon sees the upper part of the cylinder stop rotating? I think not.
I think you're correct that no signal can be transmitted up the cylinder if the lower end is at (or below) the horizon, since any signal sent from the lower end of the cylinder upward is limited to the speed of light, and signals emitted radially outward at the horizon traveling at the speed of light stay at the horizon forever--they never get to any larger radius.
However, I don't agree that the "point of view" that says the cylinder will stop rotating when it arrives at the horizon is correct. The "hovering" viewpoint, which you describe further on in your post (in the quote I'll give below), does not cover the horizon, because the coordinate system on which it is based, exterior Schwarzschild coordinates, becomes singular there. To analyze what happens at the horizon you have to switch to a viewpoint that covers it, such as the viewpoint of an infalling observer (e.g., Painleve coordinates), and from such a viewpoint, the cylinder does *not* stop rotating at the horizon. See below.
yuiop said:
Mechanical forces are transmitted up the cylinder at the speed of sound in the cylinder material while the lower parts are (locally) approaching the speed of light.
This is more or less the "hovering" viewpoint of what I stated above, that signals emitted outward at the horizon never get to any larger radius--so as one gets closer and closer to the horizon, it takes longer and longer for signals to get out, approaching the limit of "infinitely long" at the horizon itself. (We can idealize the cylinder as having the maximum possible stiffness allowed by relativity, so that the speed of sound in the cylinder equals the speed of light; this allows us to assume that mechanical forces are transmitted at the speed of light in the cylinder, but no faster.)
yuiop said:
Secondly, as far as the stationary observer is concerned, it takes an infinite amount of his local time for the lower end of the cylinder to fall the short distance from r=2.020202M to r=2M. The top of the cylinder will arrive at his location long before the lower part reaches the event horizon from his point of view and the cylinder will appear to be subject to extreme length contraction. So it seems we are unable to use the long rotating cylinder to "probe" what is happening at the event horizon. Any thoughts?
This is true, but again, it does *not* imply that the cylinder stops rotating at the horizon; it only implies that the "hovering" viewpoint can't cover the horizon. From the viewpoint of an infalling observer riding alongside the cylinder and free-falling with it across the horizon, the cylinder keeps rotating at the same rate the whole time; in fact, the infalling observer does *not* see the "time dilation" effect that the hovering observer sees--both ends of the cylinder are always rotating at the same rate as far as the infalling observer is concerned. (Note that this involves another unstated assumption: that tidal gravity can be neglected over the length of the cylinder, which means the black hole has to have a large enough mass for tidal gravity to be negligible over the range of radial coordinates that are covered by the cylinder at any instant of the cylinder's proper time. If tidal effects can't be neglected, they will either stretch the cylinder or cause internal stresses in it, both of which may change how it behaves.)