tiny-tim said:
You are saying that the particle (or the geodesic) follows a future time direction, which
is the same as "there is no space direction to follow"!
Huh? All geodesics "follow a future time direction", unless I'm misunderstanding what you mean by that phrase. Put it this way, the geodesic extending from an event inside the horizon lies inside the future light cone of that event, just as would be true for geodesics outside the horizon; the point is that the light cones tip over as they get closer to the horizon, as depicted in the diagrams at the bottom of http://www.etsu.edu/physics/plntrm/relat/blackhl.htm which I have pointed to before.
tiny-tim said:
erm … if my head goes through the event horizon before my feet, then surely I
will hit the singularity head-first!
I would guess it's probably true that if you synchronize clocks at your head and feet using the usual SR technique when far from the hole, then fall in head-first, your head would indeed be crushed earlier according to the clock there. But I think this is sort of complicated by gravitational time dilation--if you were to synchronize a different pair of clocks at your feet and head using the same method after having let the first pair run for a while, I think you'd find that according to the newly-synchronized pair, the clock at your head would show less time than the one at your feet thanks to gravitational time dilation (the same would be true if you just stood on your head for a long time in a strong gravitational field--your head would age slower than your feet, in effect). It may be that if you synchronize a new pair of clocks at your head and feet very shortly before being crushed by the singularity, then the difference in time that each was showing at the instant of being crushed would be very small, and that the closer the new synchronization was to the moment of being crushed, the less the time difference.
Also, even if your feet and head are at some sense crushed at different times (one would have to specify a particular coordinate system for the falling observer to make sense of this), if you think in terms of Egan's description of the approaching the singularity being like the collapse of a hypercylindrical universe, then it may just be that the collapse seems asymmetrical in this coordinate system, with the region of space at your head having collapsed to zero radius in the two finite directions before the region of space at your feet has collapsed to zero radius in these directions. You'd still be hitting the singularity "future-first" in this picture.
tiny-tim said:
Sorry, but "enforced falling" is a fact.
Our job is to choose the mathematics or physics with which to describe that fact.
It's also a fact that according to GR, the future light cone of any event that happens inside the horizon contains only events which lie at a smaller Schwarzschild radius, none which lie at a greater one. I guess you can call this "enforced falling" if you so choose, but it seems like a counterintuitive description to me, since from the perspective of a locally inertial coordinate system surrounding that event, you can still go in any direction of any of the three spacelike dimensions.
tiny-tim said:
rab99 and I think that talking about
movement along a
time direction is confusing and against common-sense.
Who said anything about "movement along a time direction"? The observer inside the horizon has three space dimensions and one time dimension, and the worldline must be timelike as always (meaning that every point on the worldline lies in the past or future light cone of every other event on it). It's just that the light cones are tilted so that every point in the future light cone of some event inside the horizon will be at a smaller Schwarzschild radius than that event. And in Schwarzschild coordianates, the t-coordinate is a
space direction inside the event horizon, while the r-coordinate is now the new time dimension; this is just a property of Schwarzschild coordinates though, it is possible to find other coordinate systems where the same coordinate is used for time both inside and outside the horizon.
tiny-tim said:
I
would be happier with the following explanation:
Outside an event horizon, an object follows a time-like geodesic (in space-time). The time-like geodesics go in every space direction.
Inside an event horizon … it's the same … an object follows a time-like geodesic! Except that the time-like geodesics now do not go in every space direction, but are confined within a cone.

Outside or inside the event horizon, objects follow timelike geodesics. Outside or inside the horizon, if you pick some event, and then pick some 3D spacelike surface which lies within the 4D future light cone of that event (like the base of an ordinary 3D cone), then there are geodesics going from the original event to every point in that spacelike surface, which is what we mean by "geodesics go in every space direction". And
exactly the same thing is true inside the horizon--if you pick any 3D spacelike surface which lies within the future light cone of an event inside the horizon, then there are geodesics from that event to
any point within the surface (it is probably easier to visualize if you imagine a universe with only 2 space dimensions and one time, so light cones look like ordinary 3D cones and a spacelike surface would just be a flat 2D 'bottom' to a cone whose pointy end represents the event that this is the light cone for). So, it doesn't make any sense to argue that there are spatial directions which the falling observer can't go in. Such a notion would violate the equivalence principle, which says that in any local region of spacetime picked from a larger curved spacetime, it must be possible to find a locally inertial coordinate system in that region where a freefalling observer is at rest and the laws of physics work exactly the same as in SR. Since there are no restrictions on which spatial direction you can move in SR, it can't be true that you'd see such a restriction in GR.
tiny-tim said:
This uses the
same physics …
unlike saying "we must now move along time directions instead of space directions" … the physics is that movement is always along time-like directions, but those directions are arranged differently inside an event horizon compared with outside!
No, the Egan quote
does use the same physics. I suggest that you look at some actual GR textbooks and see what they have to say about the subject before making these confident but uniformed statements about what the theory predicts. For example, a tilting light-cone diagram almost identical to the one I keep linking to at the bottom of http://www.etsu.edu/physics/plntrm/relat/blackhl.htm can be found on p. 829 of the Misner-Thorne-Wheeler textbook
Gravitation, and on p. 823 they write of the problem with using Schwarzschild coordinates for events inside the horizon:
The most obvious pathology at r=2M is the reversal there of the roles of t and r as timelike and spacelike coordinates. In the region r > 2M, the t direction, \frac{\partial}{\partial t}, is timelike (g_{tt} < 0) and the r direction, \frac{\partial}{\partial r}, is spacelike (g_{rr} > 0); but in the region r < 2M, \frac{\partial}{\partial t} is spacelike (g_{tt} > 0) and \frac{\partial}{\partial r} is timelike (g_{rr} < 0).
What does it mean for r to "change in character from a spacelike coordinate to a timelike one"? The explorer in his jet-powered spaceship prior to arrival at r=2M always has the option to turn on his jets and change his motion from decreasing r (infall) to increasing r (escape). Quite the contrary is the situation when he has once allowed himself to fall inside r=2M. Then the further decrease of r represents the passage of time. No command that the traveler can give to his jet engine will turn back time. That unseen power of the world which drags everyone forward willy-nilly from age twenty to forty and from forty to eighty also drags the rocket in from time coordinate r=2M to the later value of the time coordinate r=0. No human act of will, no engine, no rocket, no force (see exercise 31.3) can make time stand still. As surely as cells die, as surely as the traveler's watch ticks away "the unforgiving minutes," with equal certainty, and with never one halt along the way, r drops from 2M to 0.
Likewise, on p. 3-20 of Taylor and Wheeler's
Exploring Black Holes: Introduction to General Relativity they write:
Inside there is an interchange of the character of the t-coordinate and the r-coordinate. For an r-coordinate less than the Schwarzschild radius 2M, the curvature factor (1 - 2M/r) in the Schwarzschild metric becomes negative. In consequence, the signs reverse between the radial part and the time part of the metric, making the dt^2 term negative and the dr^2 term positive. Space and time themselves do not interchange roles. Coordinates do. The t-coordinate changes in character from a timelike coordinate to a spacelike coordinate. Similarly, the r-coordinate changes in character from a spacelike coordinate to a timelike one.