Hi, AlphaNumeric,
AlphaNumeric said:
You'd notice the view out your porthole/window looking pretty weird as the light bending effects become so powerful, but if you were falling in a windowless lift you'd not know when you passed the event horizon.
Agreed: observers falling freely into a black hole, or hovering outside a black hole, or otherwise using a rocket engine to manuever in a strong gravitational field, would experience various interesting optical effects. The simulations at http://casa.colorado.edu/~ajsh/schw.shtml are potentially a bit misleading in the present context, but serve to give some indication.
AlphaNumeric said:
If you were falling slow enough, you'd reach a point where your feet were inside the EH and your head not.
Consider the Schwarzschild vacuum solution. Speaking somewhat loosely, the "slowfall frame field" models the physical experience of infalling observers who fire their rocket engine radially inwards with just the right thrust to oppose the attraction of the hole, according to Newtonian theory, namely m/r^2, which of course is less than the corresponding quantity in gtr, namely m/r^2/\sqrt{1-2m/r}, with the result that these observers slowly fall radially inwards.
More precisely, in the ingoing Eddington chart
ds^2 = -(1-2m/r) \, du^2 + 2 \, du \, dr + r^2 \, \left( d\theta^2 + \sin(\theta)^2 d\phi^2,
-\infty < u < \infty, \; 0 < r < \infty, \; 0 < \theta < \pi, \; -\pi < \phi < \pi
consider the frame field
\vec{e}_0 = \partial_u - m/r \, \partial_r
\vec{e}_1 = \partial_u + \left( 1 - m/r \right) \, \partial_r
\vec{e}_2 = 1/r \, \partial_\theta, \; \vec{e}_3 = 1/r/\sin(\theta) \, \partial_\phi
Here the acceleration vector of the world lines (integral curves of the timelike unit vector \vec{X} = \vec{e}_0) is \nabla_{\vec{X}} \vec{X} = \frac{m}{r^2} \, \vec{e}_1. These world lines are given by u-u_0 = -r^2/2/m.
AlphaNumeric said:
Then you wouldn't be able to see your feet. From then on, your feet would be invisible, as would anything below your eyes.
Careful, that's not true as stated. I think you meant to say: "your view of your feet would be somewhat out of date". Likewise for electrical signals from that region of your body. Of course--- and this is rather the point--- this would be true in any region of any spacetime.
AlphaNumeric said:
all bodily functions would stop since blood wouldn't be able to go up from your heart to your head or nerve impulses. You'd die at the event horizon
You already know that nothing special happens locally at the event horizon, so you already know that this can't be quite right. But it is true that anyone falling sufficiently "slowly" in the sense of slowly decreasing Schwarzschild radial coordinate would have to be accelerating outward, and accelerating sufficiently hard can certainly break a human body, as in the example of a skydiver whose parachute fails catastrophically.
AlphaNumeric said:
your body's general shape would not be turn apart till you hit strong enough tidal forces.
I am not sure what you are thinking of here, but as MTW remark, the Coulomb form of the tidal tensor appears not only for static observers in the exterior, but also for freely and radially infalling observers--- and for the slowfall observers defined above. Specifically, wrt the above frame field, the expansion tensor (of our timelike congruence) is
\theta[\vec{X}]_{\hat{a} \hat{b}} = m/r^2 \, \rm{diag} \left( 1, \, -1, \, -1 \right)
and the tidal tensor is
E[\vec{X}]_{\hat{a} \hat{b}} = m/r^3 \, \rm{diag} \left( -2, \, 1, \, 1 \right)
(Hatted indices are often used to stress that components refer to a specific frame field, not the coordinate basis; see MTW.)
Chris Hillman