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J.F. said:Yes, they mean the all points accelerated with constant and equal proper acceleration by law
x(t,s)=s+\frac{c^{2}}{w}\sqrt{1+(wt/c)^{2}}-
-\frac{c^{2}}{w}
0{\leq}s{\leq} L
Ok, they are essentially using the same formula used by Baez in "The Relativistic Rocket Equations" See http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
I quote from Baez:
"First of all we need to be clear what we mean by continuous acceleration at 1g. The acceleration of the rocket must be measured at any given instant in a non-accelerating frame of reference traveling at the same instantaneous speed as the rocket (see relativity FAQ on accelerating clocks). This acceleration will be denoted by a. The proper time as measured by the crew of the rocket (i.e. how much they age) will be denoted by T, and the time as measured in the non-accelerating frame of reference in which they started (e.g. Earth) will be denoted by t. We assume that the stars are essentially at rest in this frame. The distance covered as measured in this frame of reference will be denoted by d and the final speed v. The time dilation or length contraction factor at any instant is the gamma factor γ."
His formula is d = (c2/a) (sqrt[1 + (at/c)2] - 1).
Say we have two rockets initially at rest in frame S. We take one rocket r1 to be at the origin of frame S (x=0) and the other rocket r2 is at x = L. Both accelerate with constant and equal proper acceleration (a) in the x direction. At time t as measured in the frame S they will be a distance d2-d1 apart
= [L + (c2/a) (sqrt[1 + (at/c)2] - 1)] - [((c2/a) (sqrt[1 + (at/c)2] - 1)]
= L.
An observer in an inertial frame that is momentarily comoving with accelerating rockets, measures them to be a distance L/sqrt(1-(v/c)^2), which is of course greater than their initial separation.
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