Angle-Preserving Linear Transformations in 2D Space for Relativity

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SUMMARY

The discussion focuses on angle-preserving linear transformations in 2D space, specifically in the context of Lorentz transformations as presented in a minutephysics video. The key transformations identified are the Euclidean rotation for cases where \( T > 4 \), the Galilean boost for \( T = 4 \), and the Lorentz boost for \( T < 4 \). The user seeks clarification on why only these three transformations satisfy the properties of angle preservation and linearity in flat geometry, and requests a mathematical proof or argument to support this conclusion.

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  • Understanding of Lorentz transformations
  • Familiarity with spacetime diagrams
  • Knowledge of linear algebra, specifically matrix transformations
  • Concept of metric spaces in geometry
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  • Research the mathematical proof of angle-preserving transformations in flat geometry
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This discussion is beneficial for physicists, mathematicians, and students studying relativity, linear algebra, and geometric transformations, particularly those interested in the foundational aspects of spacetime and its mathematical representations.

Shirish
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I'm watching this minutephysics video on Lorentz transformations (part starting from 2:13 and ending at 4:10). In my spacetime diagram, my worldline will be along the ##ct## axis and the worldline of an observer moving relative to me will be at some angle w.r.t. the ##y## axis.

When we switch to the other observer's spacetime diagram, the observer's worldline will be along the ##y## axis and my worldline would flip over to the other side, but the angle between the worldlines would be preserved. Then the video goes on to mention three possibilities:

hHR59.png


The event at ##(2,4)## ends up getting mapped to ##(0,T)##, where ##T<4##, ##T=4## or ##T>4##. And it seems like the video is suggesting only one possible transformation for each case, giving a total of only three possible transformations. For an angle preserving transformation ##A##, given any two unit vectors ##u_1,u_2##, $$[u_1]^TM[u_2]=[u_1]^TA^TMA[u_2]\implies M=A^TMA$$ where ##M## is the metric we're assuming for the space. Seems like (though I'm not a 100% sure) the ##T>4## possibility corresponds to rotation (Euclidean, sure about this one), ##T=4## to Galilean boost (Galilean) and ##T<4## to Lorentz boost (Minkowski metric).

But why is it being suggested that only these three transformations (satisfying the angle preservation and linearity properties) are possible? Is it possible to find any other transformations than rotation for the case of ##T>4##, or other than Lorentz for ##T<4##, etc.? If not, can anyone direct me to a proof or explanation of why only three transformations are possible?

(Specifically a mathematical argument/proof of why Euclidean, Galilean and Lorentz must be the only linear angle-preserving transformations in flat geometry would be nice)
 
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He discusses on x-t diagram so rotation which includes y,z coordinate is a digression from his scenario. It has nothing to do with your T discussion. Inversion and displacement, neither.
Galilean transformation was revealed not to be a right one to describe nature.
 
Small edit to my original post since I'm not finding the option to directly edit: in the first 2 paragraphs, I miswrote ##ct## axis as ##y## axis.
 

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