Position of Particle in Special Relativity (A vs B)

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Discussion Overview

The discussion revolves around the application of Lorentz transformations in Special Relativity, specifically focusing on the position of a particle in two reference frames, A and B, moving relative to each other. Participants explore how to derive the position function of a particle in one frame based on its position in another frame, while addressing units and the implications of different speed values.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant presents the position of a particle in frame B as ##x' = f(t') = 3t'## and seeks to find the corresponding position function in frame A.
  • Another participant questions the units being used, noting that in natural units where ##c = 1##, the given function implies a speed exceeding the speed of light.
  • A participant clarifies they are using classical units where ##c = 3 \times 10^8 \text{ m/s}## and discusses the implications for speed in the primed frame.
  • One response suggests that the velocity addition law can be used to derive the position function in frame A without needing the full Lorentz transformation.
  • Another participant mentions that transforming from ##x' = f(t')## to ##x = f(t)## can be complex due to the differences in coordinates, but transforming using proper time ##\tau## simplifies the calculation.

Areas of Agreement / Disagreement

Participants express differing views on the complexity of transformations and the appropriateness of using proper time versus coordinate time. There is no consensus on the best approach to derive the position function in frame A.

Contextual Notes

Participants note that the transformation process involves multiple variables and assumptions about speed and units, which may affect the outcomes of their calculations. The discussion highlights the challenges in applying Lorentz transformations and the nuances of different reference frames.

adosar
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Recently I have come into Special Relativity and specifically Lorentz transformation. Let's assume two frames A and B moving relative with speed ##v##. The position of a particle moving with respect to B is given by ##x′=f(t′)=3t′##. What is the function of position ##x=f(t)## of the particle for the observer A? Thanks in advance. As I said before I am new to Special Relativity.
 
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adosar said:
The position of a particle moving with respect to B is given by ##x′=f(t′)=3t′##.

What units are you using? In the natural units of relativity, where ##c = 1##, the worldline ##x' = 3 t'## is impossible; it would mean that the particle would be moving at 3 times the speed of light.
 
PeterDonis said:
What units are you using? In the natural units of relativity, where ##c = 1##, the worldline ##x' = 3 t'## is impossible; it would mean that the particle would be moving at 3 times the speed of light.
Thanks for the reply. I am using the "classical" units where c=3*10^8 m/s. I was just trying to figure out if given a position function for one (A) reference frame we can deduce another position function for another reference frame (B) moving relative with A.
 
adosar said:
I am using the "classical" units where c=3*10^8 m/s.

So that means ##x' = 3 t'## implies a speed in the primed frame of 3 m/s? Ok, good.

adosar said:
was just trying to figure out if given a position function for one (A) reference frame we can deduce another position function for another reference frame (B) moving relative with A.

Yes, we can, but for the simple function you give, you don't need the full Lorentz transformation to figure it out. You just need the velocity addition law: in the unprimed frame, the function will be ##x = w t## where

$$
w = \frac{v + 3}{1 + \frac{3 v}{c^2}}
$$
 
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adosar said:
Recently I have come into Special Relativity and specifically Lorentz transformation. Let's assume two frames A and B moving relative with speed ##v##. The position of a particle moving with respect to B is given by ##x′=f(t′)=3t′##. What is the function of position ##x=f(t)## of the particle for the observer A? Thanks in advance. As I said before I am new to Special Relativity.
This is just straight algebra. You have ##x’=f(t’)## so just substitute ##x’=\gamma\ (x-vt)## and ##t’=\gamma\ (t-vx/c^2)##. Then solve for ##x=g(t)##
 
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PeterDonis said:
So that means ##x' = 3 t'## implies a speed in the primed frame of 3 m/s? Ok, good.
Yes, we can, but for the simple function you give, you don't need the full Lorentz transformation to figure it out. You just need the velocity addition law: in the unprimed frame, the function will be ##x = w t## where

$$
w = \frac{v + 3}{1 + \frac{3 v}{c^2}}
$$
Thanks so much. I was trying to figure it out through position and time transformations.
 
adosar said:
Thanks so much. I was trying to figure it out through position and time transformations.
That's how you derive the velocity transformation, so it ought to have worked.
 
Just a comment. The transformation of x' = f(t') into x = f(t) winds up to be rather ugly. t and t' are different coordinates, due to the relativity. Thus, as other posters have mentioned, one needs to transform both x' and t'. The transformation x' = f(##\tau##) into x = f(##\tau##) is much simpler. Here ##\tau## denotes proper time. Because ##\tau## is a world scalar, it doesn't need to be transformed, thus one only needs to use the Lorentz transform to transform x' to x, making it a significantly easier calculation.

Sometimes you do want to express things in terms of coordinate time t rather than proper time ##\tau##, but it's often worth looking at the alternative.
 
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