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Spacetime curvature can be a little bewildering
for most of us. It is an intimidating subject and just when we had a good look
at the "rubber sheet analogy" and start thinking, "OK, I get
it", someone tells us that it's less than half the story.
The reason is that the rubber sheet with its mass in the middle is static in
time, so it visualizes only spatial curvature. In a way it is just a snapshot
of spacetime at one given moment, so we need a movie of the rubber sheet at
successive times. This is possible, but the scale of the time axis soon becomes
problematic and it is very difficult to see the spacetime curvature
anyway.
There is a way of viewing spacetime curvature, by sacrificing one spatial
dimension and use it for a time dimension, so that we have one space, one time
and one 'hyper-space' dimension. Just like for the rubber sheet, hyperspace is
a fictitious dimension, so that space can have somewhere to curve into. The
other (up) dimension is now propertime, the reading of a clock sitting on the 'local
time' curve. To make things more palatable, math will be relegated to the
endnotes… 

The central bullet represents a point mass (black hole) M at the origin of
Schwarzschild spacetime and rs is the Schwarzschild radius of
the black hole. The top curve looks like 'curved time' and the bottom curve
looks like 'curved space', but actually, the bottom curve is just a projection
of the top curve (spacetime) onto the space-hyperspace plane.
At the point of interest (ro), which is distance r from
the origin, two tangents are drawn and they intersect at a point cc, on
the space-hyperspace plane. This point is the essence of it all - it is the
center of spacetime curvature and the distance ro to cc
(R) is the radius of spacetime curvature at the point ro.(1)
Now the interesting thing is that if we let time move on (by an increment dt)
and let the vector R rotate around the curvature center cc, the
centripetal acceleration at the point ro is exactly equal to
the proper gravitational acceleration at that point.(2) This gives some confidence that the curve
really represent spacetime curvature, albeit with only one space
dimension.
I will post a few more pointers for simplifying the Schwarzschild metric later, but in the meantime, questions are welcome.
Jorrie
(1)
Actually, it is just a tangent vector to the top (spacetime)
curve that intersects the space-hyperspace plane. The vector length is not
difficult to obtain: R = -(1-rs/r)0.5 r2c2/GM.
(3)
(2)
In relativity one must specify a bit more precisely: proper
acceleration is the reading on a static accelerometer, held at constant r
by some means, e.g. a rocket. In geometric units (which we have to use in order
to use the geometry of the situation), the accelerometer will 'move upwards' a
distance cdt in a time interval dt. The centripetal acceleration
will equal the velocity squared (c2) divided by the vector
length (R), so effectively a = -GM/(r2(1-rs/r)0.5). This is just Newton's gravity (-GM/r2)
increased by a factor 1/(1-rs/r)0.5.
(3)
The equations for the two curves are obtained from the
Schwarzschild metric: dtau2 = (1-rs/r) dt2
- dr2/(1-rs/r), simplified for when there is
no tangential movement. With the values and the derivatives against r
(slopes) of each curve at ro, the point of intersection (cc)
and the length R is just geometry/algebra. When there is tangential movement,
the situation becomes more complex, but still manageable. 
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