Measuring displacements in Minkowski spacetime
Mortimer said:
But then again, this whole situation is purely academic anyway because a spacelike distance between events can only be demonstrated at velocities > c which is still considered an impossibility.
For your understanding, it is probably important to remember that the distance between events (i.e. ) in Minkowski space-time is just a "gadget" that happens to be invariant under a Lorentz transformation. It has no real physical meaning like for instance a distance in space or a timelapse on a clock. The math is merely a tool that helps making the correct calculations (just as complex numbers are for instance).
Mortimer said:
Any pair of events that are simultaneous in some reference frame have a spacelike separation, yes? FTL speeds are required for information transfer between such events
Yes. So there is no way that you can ever "see" or "measure" such a situation (note that I deliberately said "demonstrated", not "exist").
Well, depends on what you want to do with it, doesn't it? If i will never ever be able to come across the situation, what's the point in discussing it like it is real? It's like speculating about tachyons and so.
This may be helpful.
Here's a procedure to measure displacements in [Minkowski] spacetime using a clock, a light source, and detector. (This is the "radar method".)
Given two events, P and Q, what is the square-interval?
Consider an inertial observer meeting P.
One his worldline, there is
an event S when at a light ray can be sent to Q, and
an event R when that light ray's reflection is received from Q.
Let t_P, t_S, t_R be the times read off that observer's clock. (Obviously, t_R \geq t_S.)
According to this observer, the spatial-displacement from P to Q is
\Delta x_{Q\mbox{ from }P}=c(t_R-t_S)/2 ,
that is, half of the measured round-trip time multiplied by the speed of light.
According to this observer, the time-coordinate of the distant-event Q
is DEFINED by t_Q= (t_R+t_S)/2,
that is, the average of the send and receive clock-readings.
So,
according to this observer, the time-displacement from P to Q
is \Delta t_{Q\mbox{ from }P}=t_Q-t_P,
or
\Delta t_{Q\mbox{ from }P}=(t_R+t_S )/2 -t_P.
that is, the average of the send and receive clock-readings minus the clock-reading t_P.
The following quantity can tell us about the causal relationship of Q from P.
( t_R - t_P)(t_S - t_P).
If the events on this worldline happen in the sequence S-then-P-then-R,
then Q is
spacelike-related to P. This quantity is negative.
If the events on this worldline happen in the sequence P-then-S-then-R,
then Q is in the
timelike-future of P. This quantity is positive (since it's the product of two positive numbers).
If the events on this worldline happen in the sequence S-then-R-then-P,
then Q is in the
timelike-past of P. This quantity is positive (since it's the product of two negative numbers).
If any two events coincide, then that quantity is zero.
If it's S and P that coincide, then Q is in the
lightlike-future of P.
If it's R and P that coincide, then Q is in the
lightlike-past of P.
If S, R, and P coincide, then Q
coincides with P.
Now, consider any two inertial observers that meet P and
perform this procedure to make measurements of Q.
So, each observer will have a different set of send and receive events and
thus a different set of clock-readings for send and for receive.
According to special relativity, the quantity
c^2( t_{receive} - t_P)( t_{send} - t_P) is invariant.
Indeed,
<br />
\begin{align*}<br />
(c\Delta t_{Q\mbox{ from }P})^2-(\Delta x_{Q\mbox{ from }P})^2<br />
&=c^2\left(\frac{t_R+t_S}{2} -t_P\right)^2-\left(c\frac{t_R-t_S}{2} \right)^2\\<br />
&=c^2\left(\frac{(t_R-t_P)+(t_S-t_P)}{2}\right)^2-\left(c\frac{(t_R-t_P)-(t_S-t_P)}{2} \right)^2\\<br />
&=c^2\left( \left(\frac{(t_R-t_P)+(t_S-t_P)}{2}\right)^2-\left(\frac{(t_R-t_P)-(t_S-t_P)}{2} \right)^2\right) \\<br />
&=c^2\left( \frac{2(t_R-t_P)(t_S-t_P)}{4} - \frac{-2(t_R-t_P)(t_S-t_P)}{4} \right) \\<br />
&=c^2 (t_R-t_P)(t_S-t_P) \\<br />
\end{align*}<br />
(This calculation is simpler if we assume t_P=0.
To keep to the spirit of emphasizing the time-measurements, one should start at the bottom with (t_R-t_P)(t_S-t_P) and obtain the expression (c\Delta t)^2- \Delta x^2.)
So, to comment on the sections I quoted above,
there is a way to measure (with a physical setup) the separation of two spacelike-related events.