Should the 'time' axis of a Minkowski diagram be time's imaginary unit?

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Discussion Overview

The discussion revolves around the use of the imaginary unit in the time coordinate of Minkowski diagrams, particularly the ##\mathrm{i} c t## convention. Participants explore its implications for special relativity (SR) and general relativity (GR), as well as the potential confusion it may cause in understanding spacetime metrics. The conversation includes theoretical considerations, mathematical reasoning, and differing perspectives on the appropriateness of this convention.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • Some participants argue that the ##\mathrm{i} c t## convention can make the metric appear Euclidean, but this is merely a matter of preference and does not change the underlying physics.
  • Others strongly discourage the use of the ##\mathrm{i} c t## convention, suggesting it complicates understanding, especially in the context of general relativity where it is said to no longer be applicable.
  • A participant mentions that the choice of using imaginary time can lead to confusion and that it may not be fundamental, as indicated by sources like Taylor's "Space-time Physics".
  • Some contributions highlight that using the ##\mathrm{i} c t## convention can lead to sign errors in general relativity, suggesting that it may introduce unnecessary complications.
  • There are discussions about the mathematical implications of using imaginary time and real space coordinates, with references to the complex plane and its established rules.
  • Participants note that the ##\mathrm{i} c t## convention is often abandoned in favor of more rigorous formulations as one moves to general coordinate systems in GR.

Areas of Agreement / Disagreement

Participants express differing views on the utility and appropriateness of the ##\mathrm{i} c t## convention. While some see it as a useful tool for certain contexts, others argue it leads to confusion and is ultimately not fundamental, particularly in general relativity. The discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Limitations include the dependence on the choice of coordinate systems and the potential for confusion arising from the use of imaginary numbers in physical interpretations. The discussion also highlights the transition from special to general relativity and the implications for the use of the ##\mathrm{i} c t## convention.

jk22
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Since the metric is euclidean in coordinates ##(ict,x)## it can be drawn in a plane, but if the metric is ##diag(1,-1)##, can both axis still be drawn in a plane ?
 
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You can draw anything two-dimensional in a plane. You do not even need a metric at all. What is going to differ is that the interpretation of the physical distance between points on your drawing is going to be irrelevant.
 
I strongly discourage the use of the ##\mathrm{i} c t## convention in relativity. It's maybe a bit inconvenient first to introduce the Minkowski-pseudometric coefficients ##\eta_{\mu \nu}## and to deal with upper and lower indices for vector and tensor components, but it pays off. At the end at latest when it comes to general relativity the ##\mathrm{i} c t## convention doesn't make any sense anymore!
 
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vanhees71 said:
I strongly discourage the use of the ##\mathrm{i} c t## convention in relativity. It's maybe a bit inconvenient first to introduce the Minkowski-pseudometric coefficients ##\eta_{\mu \nu}## and to deal with upper and lower indices for vector and tensor components, but it pays off. At the end at latest when it comes to general relativity the ##\mathrm{i} c t## convention doesn't make any sense anymore!

The ict notation is necessary to confuse people. If students cannot deal with confusing notation, they won't be able to become good theoretical physicists! :oldbiggrin: http://www.staff.science.uu.nl/~hooft101/lectures/genrel_2013.pdf
 
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Hm, ok. The logical conclusion from 't Hooft's many words about his awkward decision to do SRT with the infamous ##\mathrm{i} c t## convention and GRT in the more appropriate real-time formalism is that sign errors are unavoidable in GR. Well, then you have to live with that o0).
 
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Well the i comes too from taking squares when formulating the invariance of speed of light ##x=ct\Leftrightarrow x'=A(x,t) ct'##, whereas taking plus minus for the A function treats cases separately and has free parameters (unwanted ?), but squaring leads to bilinear forms but also implies the price to pay as a singularity (BTW why is it not called the speed of light catastrophe ?) and imaginary numbers.
 
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jk22 said:
i comes too from taking squares when formulating the invariance of speed of light ##′x=ct\Leftrightarrow x'=A(x,t) ct'##, whereas taking plus minus for the A function treats cases separately and has free parameters (unwanted ?), but squaring leads to bilinear forms but also implies the price to pay as a singularity (BTW why is it not called the speed of light catastrophe ?) and imaginary numbers.

None of this makes sense. It appears that you do not understand either the rationale for, or the limitations of, the ##ict## convention.

In special relativity, the choice of whether to multiply the ##t## coordinate by ##i## to make the metric look Euclidean (notice I said "look" Euclidean, not "be" Euclidean) is a matter of preference and convention. For some purposes the ##ict## convention can be useful, which is why you sometimes see it in the literature.

However, you can't change the actual physics by changing conventions; the actual, physical spacetime still has timelike, null, and spacelike intervals, and Lorentz transformations still act differently on the three different kinds of intervals (or vectors in a more rigorous formulation) even if you obfuscate that fact by making the metric look Euclidean.

As @vanhees71 points out, once you move to general relativity, the ##ict## convention no longer works; this is its most important limitation, and the reason why GR textbooks will tell you that you have to unlearn it. (MTW, for example, has a clear explanation of the issue.)
 
PeterDonis said:
As @vanhees71 points out, once you move to general relativity, the ict convention no longer works
I would say it is sufficient to start writing down SR in general coordinate systems to make it no longer work.
 
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I think it was Taylor, in "Space-time physics" who has a chapter heading entitled "Farewell to ict". The takeaway from this should be that one should expect to abandon "ict" at some point, that it's not fundamental.

I haven't verified that I got the source of the "farewell" quote right, this is from memory. But eventually, the ict convention is no longer used, it stops working. Basically, "ict" is a fudge that can delay the need for the introduction of a metric tensor if one uses cartesian coordinates in flat space-time. Cartesian coordinates do not exist in curved space-times, and even in flat space-times one may wish to use other coordinate systems. Using anything other than cartesian coordinates makes the "ict" fudge stop working.
 
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pervect said:
I think it was Taylor, in "Space-time physics" who has a chapter heading entitled "Farewell to ict".
It might be there, but it is definitely in MTW... not a full chapter, just a few short paragraphs in a named section.
 
  • #11
jk22 said:
Since the metric is euclidean in coordinates (ict,x)(ict,x)(ict,x) it can be drawn in a plane, but if the metric is diag(1,−1)diag(1,−1)diag(1,-1), can both axis still be drawn in a plane ?

I would show another disadvantage to use imaginary time and real space coordinate.
In mathematics we know Gauss plane or complex plane z=x+iy the rules of which include
|z|=\sqrt{x^2+y^2}
z^*=x-iy
do not result our ##c^2t^2-x^2## or ##x^2-y^2##. To avoid unnecessary confusion it would be better to keep imaginary component for use in Gauss plane that is very useful in all the field of physics.
 
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  • #12
Just to add: if you write down spacetime intervals for solutions which are not static, (or app,y general coordinate transfo's to static solutions) you can end up wit loose factors of i due to cross terms between time and space
 
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