Sbratman said:
If the acceleration due to gravity is velocity dependent at some point, that would solve the problem. But note that one doesn't need a black hole to cause acceleration past C (using the Newtonian force law, and the weak equivalence principle, which obviously must fail somehow, but I don't know how.) In one of my other posts I mentioned what would happen if one had a neutron star massive enough to have an escape velocity of, say, .999c. It's easy to come up with scenarios that cause a velocity > c. (see my post that mentions the "oh my god particle," that famous proton going ridiculously near the speed of light)
I have found a reference that shows gravity IS velocity dependent here:
http://www.mathpages.com/rr/s6-07/6-07.htm
They give the velocity dependent gravitational acceleration equation for a particle falling from infinity as:
a = \frac{-GM}{r^2}\left(1-\frac{2GM}{rc^2}\right)\left(3\left(1-\frac{2GM}{rc^2}\right)\left(1-\frac{V^2}{c^2}\right)-2\right)
where V^2/c^2 is the initial downward velocity of the particle at infinity. For a photon, V/c=1 at infinity and the equation reduces to:
a = \frac{2GM}{r^2}\left(1-\frac{2GM}{rc^2}\right)
Note that the equation for the acceleration of a falling photon is always positive for r>2GM/c^2 meaning that a falling photon is decelerated all the way from infinity to the event horizon starting with a velocity of c and finishing with a coordinate velocity of zero. This is consistent with the velocity of a falling photon derived directly from the Schwarzschild metric:
c' = \frac{dr}{dt} = c\left(1-\frac{2GM}{rc^2}\right)
As can be seen from this diagram http://www.mathpages.com/rr/s6-07/6-07_files/image017.gif the greater the initial velocity the greater the deceleration of gravity acting on it bringing it to zero velocity in coordinate terms (or c in local terms) at the event horizon. The velocity never exceeds c locally no matter how fast the intial velocity. This is due to a antigravity effect that is not often mentioned. Mathpages makes this antigravity effect clear in this quote:
" Notice that the value of
(d2r/dt2) / (-m/r2)
is negative in the range from r = 2m to r = 6m/(1 + 4m/R), where d2r/dt2 changes from negative to positive.
This signifies that the acceleration (in terms of the r and t coordinates)
is actually outward in this range."
and in this quote too:
"This shows that
the acceleration d2r/dt2 in terms of the Schwarzschild coordinates r and t for a particle moving radially with ultimate speed V (either toward or away from the gravitating mass)
is outward at all radii greater than 2m for all ultimate speeds greater than 0.577 times the speed of light. For light-like paths (V = 1), the magnitude of the acceleration approaches twice the magnitude of the Newtonian acceleration –
and is outward instead of inward. The reason for this outward acceleration with respect to Schwarzschild coordinates is that the speed of light (in terms of these coordinates) is greater at greater radial distances from the mass.
Mentz114 said:
SBratman, Kev,
thinking of gravity as 'accelerating' anything in GR is straining the analogy. It is space-time geometry and not force that causes the changes in motion. We don't observe things reaching the speed of light because it is barred by the geometry. If you try to account for this with Newtonian F=Ma thinking - you'll go mad.
By accelerating I mean that the velocity is increasing over time or the distance traveled per unit time is increasing. In this context it is not important whether the cause of the acceleration is gravity or geometry. If a person jumps off a high tower the situation can be explained by the person being stationary and the tower and the Earth attached to it that is actually accelerating upwards to meet him (as can be proven by an accelerometer) or you could say he is being accelerated downward by gravity (ridiculous, I know

) or you could say he is simply moving along a geodesic. Either way you know it is going to hurt. The point is that a the velocity of a falling object (whether caused by gravity or geometry) is not always increasing as it falls towards a gravitational mass. If you look very carefully at the graphs on the Mathpages page you will see that an object shot outwards from a radius of less than 2Rs can increase it velocity as it moves AWAY from the gravitational mass and only start slowing down when the radius exceeds 3Rs.
Mentz114 said:
Kev:
One can see from the geodesic equation that coordinate acceleration is proportional to velocity2, and the factor that connects them is a Christoffel symbol ( affine connection).
M
Mathpages obtains the parameter K from the affine parameter on this page
http://www.mathpages.com/rr/s6-04/6-04.htm and uses the parameter K interpreted as:
K=\sqrt{1-V^2/c^2}
or
K=\frac{1}{\sqrt{1-2GM/(Rc^2)}}
that he uses in the equations used on the page I discussed above
http://www.mathpages.com/rr/s6-07/6-07.htm