Spacetime distance and ruler-measured length on an XT chart

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KDP
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spacetime.png

With reference to the above diagram, we can see that if we used a ruler to measure the segments on the XT chart and added up all the segment lengths, that this ruler measured length is longer for the craft on the right which experiences the least elapsed proper time. Now unlike the regular spacetime distance (as correctly depicted in the picture) this XT chart ruler length is not invariant and different inertial observers will disagree on its length. However, from a quick check using a few examples in different reference frames, it seems that if one ruler measured chart path is longer than another in a given reference frame, then all observers will agree on which object has the longer XT chart ruler measured distance (Is there a formal name for this measurement?). Is it possible to show that this always the case or are there counter examples?

Just to be clear, I am talking about using the normal Pythagoras method of using $$ \sqrt{T^2 + X^2} $$ to calculate the segment lengths instead of the normal method of using$$\sqrt{T^2-X^2}$$ to calculate the spacetime distance segments.
 
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KDP said:
However, from a quick check using a few examples in different reference frames, it seems that if one ruler measured chart path is longer than another in a given reference frame, then all observers will agree on which object has the longer XT chart ruler measured distance
Consider two paths starting at the origin and ending at ##t=t_1##, ##x=\pm x_1##. The interval along each is ##t_1^2-x_1^2##, but the Euclidean length of either line drawn on the Minkowski diagram can be made longer while the other one is made shorter by a boost opposite directions. So this is a counter example to the claim that all frames agree which worldline has a longer Euclidean representation.
 
  • #3
Lets call the two paths, A and B and take the case where the first observer sees the two paths as equal and the second observer sees path A as shorter than path B. This is the outward trip. Now if they turn around so that they both return to x=0 at time t1*2, then the return path of A will be longer than that of B and by symmetry the round trip Euclidean lengths of the trips will be equal for the second observer (or any other observer) if they both return to the origin at the same time.
 
  • #4
The implication of that is tthat you have a restriction not present in your OP, that you are only considering pairs of paths that travel from one common event to another. Is that what you intended?
 
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  • #5
Ibix said:
The implication of that is that you have a restriction not present in your OP, that you are only considering pairs of paths that travel from one common event to another. Is that what you intended?
You are right. That is what I intended. Sorry for not making that clear.
 
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  • #6
KDP said:
However, from a quick check using a few examples in different reference frames, it seems that if one ruler measured chart path is longer than another in a given reference frame, then all observers will agree on which object has the longer XT chart ruler measured distance (Is there a formal name for this measurement?). Is it possible to show that this always the case or are there counter examples?

Counter-example (see screenshot):
PF-Euclid.png

Alice moves ##E_0## -> ##E_1##-> ##E_3##.
Bob moves ##E_0## -> ##E_2##-> ##E_3##.
 
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  • #7
Hi Sagittarius. You are right. I checked your figures. There are counter examples. Thanks for clearing that up.
 
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1. What is spacetime distance and how is it measured on an XT chart?

Spacetime distance is the measurement of the distance between two events in the fabric of spacetime. It is measured on an XT chart by using the coordinates of the events on the x-axis (representing space) and the t-axis (representing time) and calculating the distance between them using the Pythagorean theorem.

2. How do you calculate spacetime distance on an XT chart?

To calculate spacetime distance on an XT chart, you can use the formula D = √(Δx² + Δt²), where D is the spacetime distance, Δx is the difference in x-coordinates, and Δt is the difference in t-coordinates. This is based on the Pythagorean theorem, where the hypotenuse of a right triangle is equal to the square root of the sum of the squares of the other two sides.

3. What is the significance of ruler-measured length on an XT chart?

Ruler-measured length on an XT chart represents the distance between two events in space only. It does not take into account the time dimension. This is in contrast to spacetime distance, which considers both space and time. Ruler-measured length can be useful for measuring distances in everyday life, but for understanding the effects of relativity, spacetime distance is a more accurate measurement.

4. How does spacetime distance change in different reference frames?

Spacetime distance is relative and can change in different reference frames. This is due to the effects of time dilation and length contraction, which occur at high speeds or in strong gravitational fields. In these cases, the distance between two events may appear different depending on the observer's point of view.

5. Can spacetime distance be negative on an XT chart?

No, spacetime distance cannot be negative on an XT chart. This is because both space and time are positive quantities and the Pythagorean theorem only yields positive values. A negative value would indicate imaginary or complex numbers, which are not applicable in this context.

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