Invariance of spacetime interval

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Discussion Overview

The discussion centers around the invariance of the spacetime interval as derived from Lorentz transformations. Participants explore various methods of proving this invariance, including algebraic manipulations and matrix representations, while addressing challenges in calculations and visualizations.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant expresses difficulty in proving the invariance of the spacetime interval, noting the emergence of extra terms during their calculations.
  • Another participant suggests that sharing the entire calculation would help identify where the errors might be occurring.
  • Several participants provide alternative approaches, including working in units where c=1 and using specific substitutions into the spacetime interval equation.
  • One participant mentions the importance of the (1-β²) factor in their calculations, indicating a realization of a missing component in their earlier work.
  • Another participant discusses the advantages of using matrix notation for proving invariance, while acknowledging that basic algebra might be simpler for those less familiar with matrices.
  • There is a suggestion that learning special relativity alongside matrix algebra could be more efficient than learning special relativity alone.

Areas of Agreement / Disagreement

Participants do not reach a consensus on a single method for proving the invariance of the spacetime interval, as multiple approaches and perspectives are presented. Some participants agree on the utility of matrix methods, while others prefer traditional algebraic techniques.

Contextual Notes

Some participants express limitations in their mathematical skills, particularly in LaTeX formatting and matrix operations, which may affect their ability to fully engage with the discussion. Additionally, there are unresolved aspects regarding the specific calculations and transformations involved in proving invariance.

motoroller
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I've tried proving the invariance of the spacetime interval from Lorentz transformations 3 times now, but every time I end up with two extra terms that don't cancel! Could I have some help?
 
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I'm trying to visualize your calculations via my paranormal abilities, but somehow I fail.
 
haushofer said:
I'm trying to visualize your calculations via my paranormal abilities, but somehow I fail.


My LaTeX isn't so good, but substituting:

x'=\gamma(x+vt)
t'=\gamma(t+\frac{vx}{c^2})

into
(x')^2+(y')^2+(z')^2-c^2(t')^2

trying to get
x^2+y^2+z^2-c^2t^2

i.e. invariant interval
 
Yes you told us that in your first post in words. What you need to show us is your entire calculation, otherwise we cannot possibly know where you went wrong or what these 'extra' terms are.

Hint: It will become a lot more obvious if you work in units where c=1.
 
Last edited:
motoroller said:
My LaTeX isn't so good, but substituting:

x'=\gamma(x+vt)
t'=\gamma(t+\frac{vx}{c^2})

into
(x')^2+(y')^2+(z')^2-c^2(t')^2

trying to get
x^2+y^2+z^2-c^2t^2

i.e. invariant interval

Ok, we try to show that

<br /> ds^2 = dx^2 - dt^2 = dx&#039;^2 - dt&#039;^2<br />

With your transformation rules, write down

<br /> dt&#039; = \frac{\partial t&#039;}{\partial x}dx + \frac{\partial t&#039;}{\partial t}dt<br />

and a same expression for dx'. Now calculate the interval ds^2 in these primed coordinates. The cross terms cancel because of the minus sign in the interval, and you can check that

<br /> \gamma^2 v^2 - \gamma^2 = 1<br />

This should give that

<br /> ds^2 = ds&#039;^2<br />


That's all there is :)
 
Did you manage to do the calculation?
 
haushofer said:
Did you manage to do the calculation?

Yes - thanks, it was the (1-\beta^2) factor I was missing when re-arranging
 
Try this - straight from the Lorentz transformation equations:

x' = \gamma(x - vt) and x = \gamma(x' + vt')

x'/x = (x - vt)/(x' + vt') or x2 - xvt = x'2 - x'vt'
----------------------------------------------------------------------
t' = \gamma(t - xv/c2) and t = \gamma(t' + x'v/c2)

t'/t = (t - xv/c2)/(t' - x'v/c2) or t2 - xvt/c2 = t'2 + x'vt'/c2.

mulitply this last equation by c2: c2t2 - xvt = c2t'2 + x'vt'

now subtract this last equation from the above equation above the dotted line and you get:

x2 - c2t2 = x'2 - c2t'2

or, the other way:

c2t2 - x2 = c2t'2 - x'2

This establishes the hyperbolic relationship between time and distance. Again, this is the space interval or time interval (depending on which is positive).

This is as simple an algebraic derivation of this that you can get.
 
  • #10
All of these things get easier when you're used to working with matrices. We want to prove that (x-y)^T\eta(x-y) is invariant, i.e. that it's equal to (\Lambda(x-y))^T\eta\Lambda(x-y). So we stare at it for two seconds and realize that the equality follows immediately from the definition of a Lorentz transformation and a trivial fact about the transpose of a product.

I have said before that I think you can learn SR and matrices in less time than you can learn just SR, and I still think that's right.
 
  • #11
Fredrik said:
All of these things get easier when you're used to working with matrices. We want to prove that (x-y)^T\eta(x-y) is invariant, i.e. that it's equal to (\Lambda(x-y))^T\eta\Lambda(x-y). So we stare at it for two seconds and realize that the equality follows immediately from the definition of a Lorentz transformation and a trivial fact about the transpose of a product.

I have said before that I think you can learn SR and matrices in less time than you can learn just SR, and I still think that's right.

True, but this requires the acquisition of a working knowledge of matrix algebra. I did learn a lot of that years ago but have lost my working knowledge of this long ago and have no current knowledge of matrix operations. Thus, using the basic algebra is a little simpler for me. To wit, I don't even know what (\Lambda(x-y))^T\eta\Lambda(x-y) means yet I can still derive the basic hyperbolic relationship between t and x without it.

Of course in more complex matters, one must use the matrix notation and operations to get somewhere.
 

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