Deriving length contraction using spacetime

  • #1
Kaguro
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Homework Statement
Derive time dilation and length contraction using invariance of spacetime interval.
Relevant Equations
##ds^2 = dx^2+dy^2+dz^2 - c^2 dt^2##
Deriving time dilation was easy:

Imagine two events in frame O' at the same location.
##ds^2 = -c^2 dt'^2##

The same viewed in O frame is:
##ds^2 = dx^2+dy^2 + dz^2 - c^2 dt^2##
##\Rightarrow dx^2+dy^2 + dz^2 - c^2 dt^2 = -c^2 dt'^2##
##\Rightarrow (\frac{dx}{dt})^2+(\frac{dy}{dt})^2+ (\frac{dz}{dt})^2 - c^2 = -c^2(\frac{dt'}{dt})^2##

But since these events are at the same location in O', the dx, dy, dz is hence the amount by which O' moves in O in time dt.
Therefore,
##v^2 -c^2 = -c^2 (\frac{dt'}{dt})^2##
##\Rightarrow (\frac{dt'}{dt})^2 = 1-\frac{v^2}{c^2}##
##\Rightarrow (\frac{dt'}{dt}) = \sqrt{1-\frac{v^2}{c^2}}##
##\Rightarrow dt = \gamma dt'##




But for length contraction

I choose two events in O which are simultaneous. So dt=0
##ds^2 = dx^2+dy^2 + dz^2 = dx'^2 + dy'^2 + dz'^2 - c^2 dt'^2##
Here I can not equate any of these with the amount by which O' moves in O.

Please help.

P.S.: Why has the website become so weird ? The preview button is shifted and works differently, and I am asked to "submit homework statement" and "relevant equations" twice...
 

Answers and Replies

  • #2
anuttarasammyak
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I did it as attached.

2021-04-17 13.40.43.jpg
 
Last edited:
  • #3
PeroK
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Homework Statement:: Derive time dilation and length contraction using invariance of spacetime interval.
Relevant Equations:: ##ds^2 = dx^2+dy^2+dz^2 - c^2 dt^2##

Deriving time dilation was easy:

Imagine two events in frame O' at the same location.
##ds^2 = -c^2 dt'^2##

The same viewed in O frame is:
##ds^2 = dx^2+dy^2 + dz^2 - c^2 dt^2##
##\Rightarrow dx^2+dy^2 + dz^2 - c^2 dt^2 = -c^2 dt'^2##
##\Rightarrow (\frac{dx}{dt})^2+(\frac{dy}{dt})^2+ (\frac{dz}{dt})^2 - c^2 = -c^2(\frac{dt'}{dt})^2##

But since these events are at the same location in O', the dx, dy, dz is hence the amount by which O' moves in O in time dt.
Therefore,
##v^2 -c^2 = -c^2 (\frac{dt'}{dt})^2##
##\Rightarrow (\frac{dt'}{dt})^2 = 1-\frac{v^2}{c^2}##
##\Rightarrow (\frac{dt'}{dt}) = \sqrt{1-\frac{v^2}{c^2}}##
##\Rightarrow dt = \gamma dt'##




But for length contraction

I choose two events in O which are simultaneous. So dt=0
##ds^2 = dx^2+dy^2 + dz^2 = dx'^2 + dy'^2 + dz'^2 - c^2 dt'^2##
Here I can not equate any of these with the amount by which O' moves in O.

Please help.

P.S.: Why has the website become so weird ? The preview button is shifted and works differently, and I am asked to "submit homework statement" and "relevant equations" twice...
I suggest you take an object of proper length ##L## and describe the spacetime coordinates of each end in a second frame where the object is moving with constant velocity ##\vec v##.
 
  • #4
PeroK
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PS you can also use this idea to give a much simpler derivation of time dilation. You start with a clock in its rest frame having the coordinates: ##(t', 0, 0, 0)## and in other frame coordinates ##(t, v_xt, v_yt, v_zt)##.

Note: if the object does not pass through the spacetime origin, then we have coordinates ##(t', x'_0, y'_0, z'_0)## and ##(t, x_0 + v_xt, y_0 + v_yt, z_0 + v_zt)## and it all works out just as well.
 
  • #6
Kaguro
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57
PS you can also use this idea to give a much simpler derivation of time dilation. You start with a clock in its rest frame having the coordinates: ##(t', 0, 0, 0)## and in other frame coordinates ##(t, v_xt, v_yt, v_zt)##.

Note: if the object does not pass through the spacetime origin, then we have coordinates ##(t', x'_0, y'_0, z'_0)## and ##(t, x_0 + v_xt, y_0 + v_yt, z_0 + v_zt)## and it all works out just as well.
Wouldn't that be just plain derivation using Lorentz Transformations ?
 
  • #7
Kaguro
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I have a related question, if someone asks me to prove length contraction using four vectors, would that be similar to what I originally asked in this thread?
 
  • #8
PeroK
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Wouldn't that be just plain derivation using Lorentz Transformations ?
Not if you use the invariance rather than the explicit LT.
 
  • #9
Kaguro
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Okay..
Can you recommend me a good place/book which illustrates the use of 4-vectors to derive everything we have derived using LTs? Focusing heavily on applications of four vectors.
 
  • #10
PeroK
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Wouldn't that be just plain derivation using Lorentz Transformations ?
Let me show you what I mean.

We have two events described in two different reference frames by the coordinates:
$$(t'_0, 0, 0, 0), (t'_1, 0, 0, 0)$$ and $$(t_0, x_0, y_0, z_0), (t_1, x_0 + v_xt_1, y_0 + v_yt_1, z_0 + v_zt_1)$$
Instead of using the LT and the explicit relationship between these coordinates, we can use only the invariance of the spacetime interval, to give: $$(\Delta s')^2 = (\Delta s)^2$$ $$\Rightarrow \ -c^2(\Delta t')^2 = -c^2(\Delta t)^2 + (v_x^2 + v_y^2 + v_z^2)(\Delta t)^2 = -c^2(\Delta t)^2 + v^2(\Delta t)^2 = -c^2(1 - \frac{v^2}{c^2})(\Delta t)^2$$ And we can get the time dilation formula.
 
  • #11
PeroK
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Okay..
Can you recommend me a good place/book which illustrates the use of 4-vectors to derive everything we have derived using LTs? Focusing heavily on applications of four vectors.
Most textbooks on SR should present four-vectors in all their glory. Although they may wait until you are studying the energy-momentum of particle collisions.

A critical point is that all four-vectors transform according to the Lorentz Transformation. E.g. for boosts in the x-direction: $$A'^t = \gamma(A^t - \frac v c A^x), \ A'^x = \gamma(A^x - \frac v c A^t), \ A'^y = A^y, A'^z = A^z$$ And you can check that ##(ct, x, y, z)## is a four-vector, for example.
 
  • #12
Kaguro
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Let me show you what I mean.

We have two events described in two different reference frames by the coordinates:
$$(t'_0, 0, 0, 0), (t'_1, 0, 0, 0)$$ and $$(t_0, x_0, y_0, z_0), (t_1, x_0 + v_xt_1, y_0 + v_yt_1, z_0 + v_zt_1)$$
Instead of using the LT and the explicit relationship between these coordinates, we can use only the invariance of the spacetime interval, to give: $$(\Delta s')^2 = (\Delta s)^2$$ $$\Rightarrow \ -c^2(\Delta t')^2 = -c^2(\Delta t)^2 + (v_x^2 + v_y^2 + v_z^2)(\Delta t)^2 = -c^2(\Delta t)^2 + v^2(\Delta t)^2 = -c^2(1 - \frac{v^2}{c^2})(\Delta t)^2$$ And we can get the time dilation formula.
Okay! So I could also say this in this way: Since (ct,x,y,z) is a four vector so I can say that the coordinates of the clock is also a four vector and its norm should remain invariant under different frames. And this is exactly the invariance of the spacetime interval.
 
  • #13
PeroK
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Okay! So I could also say this in this way: Since (ct,x,y,z) is a four vector so I can say that the coordinates of the clock is also a four vector and its norm should remain invariant under different frames. And this is exactly the invariance of the spacetime interval.
To be precise, I should have said that ##(ct, x, y, z)## are the components of a four-vector.

An important point is that there is an invariant quantity associated with every four-vector: $$A^2 = -c^2(A^t)^2 + (A^x)^2 + (A^y)^2 + (A^z)^2$$ The proof of invariance follows in the same way as the proof that the spacetime interval is invariant - by using the LT directly.

The other point is that the proper time shown on a clock is a measure of this invariant spacetime interval along the worldline of the clock.

And, of course, the invariant quantity associated with the energy-momentum four-vector of a particle is its mass. This is where SR pulls everything together - mass, energy & momentum - in a way that is not even hinted at in classical mechanics.
 
  • #14
Kaguro
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My book defines four-vectors as quantities with four components that transform via LTs under a change of frame.

The other point is that the proper time shown on a clock is a measure of this invariant spacetime interval along the worldline of the clock.
Yes! :biggrin:

So the invariant quantity associated with position four vector is spacetime interval,
The invariant quantity associated with velocity four vector is speed of light,
The invariant quantity associated with energy-momentum four vector is rest mass energy!(hence mass)

Cool!
 

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