DaveC426913 said:
Well, OK, you've linked to your own posts. Do you have any references that aren't you?
Let's get this out of the way by putting up the math, this is not the first time you are making innuendos I do know what I am talking about.
Let's take a pair of stationary test observers R2 and R3 in a Schwarzschild solution with a Schwarzschild radius of R.
Do you agree that the ruler distance between them is:
<br />
\rho = R \left( \sqrt {3}\sqrt {2}-\sqrt {2}+\ln \left( -\sqrt {3}+\sqrt {3}<br />
\sqrt {2}-\sqrt {2}+2 \right) \right) <br />
If so do you agree that the radar distance T in coordinate time between them is:
<br />
T = R+R\ln \left( 2 \right)<br />
And that the radar distance in proper time for R2 is:
<br />
\tau_{R2} = 1/2\, \left( R+R\ln \left( 2 \right) \right) \sqrt {2}<br />
And for R3:
<br />
\tau_{R3} = 1/3\, \left( R+R\ln \left( 2 \right) \right) \sqrt {6}<br />
With me so far or anything wrong with the math?
From this you can calculate the (average) speed of light, if you do this you will find that both the coordinate speed and the speed from r2 to r3 (r2 < r3) in proper time is always < c. Only the speed from r3 to r2 in proper time is > c.
Agreed? No? Where do I make a mistake?
For you reference if we value the R2 and R3 values we can chart it, here is a 2D plot.
Below is a plot of light speeds between pairs of static observers (o1, o2) separated a fixed ruler distance of 1 with the radar distance as measured by a clock at observer o1. In the plot you can see the ruler distance (which is 1 for each pair) divided by the radar distance, this ratio is larger for pairs closer to the EH.
[PLAIN]http://img169.imageshack.us/img169/4331/slowdownoflight.gif
And here is a 3D plot:
[PLAIN]http://img717.imageshack.us/img717/2414/001lightspeed3d.gif
Any mistakes?
If not, could you please stop making innuendos I am wrong?