Mentz114 said:
In flat spacetime, radar distance is exactly the coordinate distance. I have demonstrated that both transform by the Bondi k-factor.
I don't know what you mean by "coordinate distance." Please compare it to my meaning of "spatial distance" between two events, in my last post.
Did you see my remark about the sign convention in the LT ( post#148) ? I hope that clears up your previous misunderstanding.
Mentz114 said:
\sqrt{\frac{1+\beta}{1-\beta}}+\sqrt{\frac{1-\beta }{1+\beta}}= 2 \gamma
The left hand side is symmetric in β. Changing its sign will not change the rhs which is always 2γ.
Your math is correct. I was confused. γ will always be positive, and the left-hand-side will always be positive so long as -1<β<1, so my "smart" question was a red herring. However, my "stupid" questions are still pertinent. :) Namely, our conversation up to that point had been about spatial distance, and non-reflected signals. Suddenly we changed to radar-distance, and reflected signals.
Which is fine, of course, but that is why I was so confused. Why did we suddenly switch topics?
The sign convention for the LT - if two observers are separating then the relative velocity is +beta. If they are approaching the relative velocity is -beta.
I disagree with you. Here's the problem. If you have two sources, S1 in front of the observer, and S2 behind the observer, And your observer is going toward S1, then Obs and S1 are approaching, and O and S2 is separating. By your logic, you would have to do TWO DIFFERENT Lorentz Transformations.
Contrast this with what I've said.
(From
http://www.spoonfedrelativity.com/pages/Number-of-Wavelengths-Is-Not-Invariant.php
In both of the equations below, (x,t) represent the coordinates of events in some <i>initial</i>, or source's reference frame, and (x',t') represent the coordinates of events in some <i>final</i>, or observer's reference frame.
\begin{pmatrix} x'\\ c t' \end{pmatrix}=\begin{pmatrix} \gamma & -\gamma\beta_{obs} \\ -\gamma\beta_{obs} & \gamma \end{pmatrix} \begin{pmatrix} x\\ ct \end{pmatrix}
In this equation β<sub>obs</sub> is the velocity of the observer in the "current" reference frame. You can also write this equation as
\begin{pmatrix} x'\\ c t' \end{pmatrix}=\begin{pmatrix} \gamma & \gamma\beta_{src} \\ \gamma\beta_{src} & \gamma \end{pmatrix} \begin{pmatrix} x\\ ct \end{pmatrix}
In this equation β<sub>src</sub> is the velocity of the source in the observer's reference frame.
This is true in both frames. Doing an LT can't make converging obervers begin to separate. My calculation is for positive beta ( separating) and gets the right result.
I'm not saying converging observers separate. I'm saying a particular pair of events along the world-line of the source, and the world-line of the observer separate. The intersection of the past-light-cone of the observer, with the world-line of the object the observer is moving toward. i.e. the image of the object in the observer's reference frame.
If two observers are located at the same point at the same time, and both are observing the same event, the one moving toward the event will see the image farther away, and the one moving away from the event will see the image closer.
Again, if you have doubt of this, I refer you to
http://www.spoonfedrelativity.com/pages/SR-Starter-Questions.php,