Choice of scaling function for Penrose diagrams

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Discussion Overview

The discussion revolves around the choice of scaling functions for Penrose diagrams, exploring the implications of using the tangent function versus other potential transformations. Participants examine the theoretical underpinnings, visual representations, and the mathematical properties of these functions within the context of general relativity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that the standard definition of coordinates on Penrose diagrams involves the tangent function, questioning its desirability and whether alternatives like f=\tan^3 or f(x)=-x/[(x-1)(x+1)] could be equally valid.
  • One participant suggests that the tangent function arises naturally from cylindrical embedding, referencing a specific section of a paper for further clarification.
  • Another participant acknowledges the visual appeal of using the tangent function based on the cylindrical embedding but posits that its use may be arbitrary aside from that visual context.
  • It is pointed out that once a parametrization using sine and cosine is established, the tangent function emerges from projecting higher dimensions down to four dimensions.
  • Some participants express skepticism about the physical significance of the five-dimensional embedding, comparing it to the use of complex numbers in quantum mechanics, which, while extrinsic, can reveal significant relationships.
  • One participant highlights that there is some freedom in choosing the function, referencing specific notes that clarify the conditions under which the derivative of the inverse function must behave for large values.

Areas of Agreement / Disagreement

Participants express differing views on the necessity and implications of using the tangent function for Penrose diagrams, with some arguing for its natural emergence from certain mathematical frameworks while others suggest that alternatives could be equally valid. The discussion remains unresolved regarding the ultimate significance of the choice of scaling function.

Contextual Notes

Participants note that the choice of scaling function must satisfy specific mathematical conditions, such as the behavior of the derivative of the inverse function for large values, but the implications of these conditions are not fully agreed upon.

bcrowell
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The standard definition of coordinates on Penrose diagrams seems to be something like [itex]\tan(u\pm v)=x\pm t[/itex]. This is what Wikipedia gives, and Hawking and Ellis also give a transformation involving a tangent function, although I haven't checked whether the factors of 2, etc. agree. Neither source comments on why a tangent function is used. It's clear that if the transformation is going to be of the form [itex]f(u\pm v)=x\pm t[/itex], then f has to be a homeomorphism from a finite, open interval of the reals onto the whole real line. But it seems to me that we could just as well have used [itex]f=\tan^3[/itex], or [itex]f(x)=-x/[(x-1)(x+1)][/itex]. Is there anything about the tangent function that makes it especially desirable? Any transformation of the form [itex]f(u\pm v)=x\pm t[/itex] will preserve the shape of light-cones, since it sends curves x-t=const to curves u-v=const, and similarly for x+t and u+v. I believe that f=tan makes particles at rest have world-lines that look like hyperbolas, but is there some special reason that a hyperbola is a desirable result? World-lines of moving particles are funky S-shapes.
 
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Tangent function comes in naturally from the cylindrical embedding. See e.g. Section 4 of http://arxiv.org/abs/1008.4703" .
 
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arkajad said:
Tangent function comes in naturally from the cylindrical embedding. See e.g. Section 4 of http://arxiv.org/abs/1008.4703" .

Ah, thanks for the reference. I think I see the idea. You can make the static Einstein universe by tiling a cylinder with Penrose diagrams, so then it becomes natural to use the angle on the cylinder as a coordinate. So if I'm understanding correctly, the use of f=tan is visually compelling based on that visualized embedding, but is otherwise completely arbitrary. Does that sound right?
 
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Not quite. Once you parametrize [tex]v^2+w^2=1[/tex] by sin and cos functions, which is rather natural, then tan comes automatically by projecting from 5 to 4 dimensions.

P.S. Of course for the graphical diagram purpose only - you can take whatever suits you.
 
arkajad said:
Not quite. Once you parametrize [tex]v^2+w^2=1[/tex] by sin and cos functions, which is rather natural, then tan comes automatically by projecting from 5 to 4 dimensions.

P.S. Of course for the graphical diagram purpose only - you can take whatever suits you.
Hmm...but isn't the embedding in 5 dimensions purely extrinsic and without observable physical significance?
 
bcrowell said:
Hmm...but isn't the embedding in 5 dimensions purely extrinsic and without observable physical significance?

You can say that complex numbers in quantum mechanics are also purely extrinsic and without observable physical significance. After all you can work only with real numbers! But, working with complex numbers helps you to discover a lot of relations which do have physical significance. The same may be the case with embeddings in 5 or 6 dimensions.
 
atyy said:
There's probably some freedom of choice. Maybe try 3.2.1 and 3.2.2 of Winitzki's notes?

http://sites.google.com/site/winitzki/index/topics-in-general-relativity

Aha! That's exactly what I needed! On p. 77, he explains why f is basically arbitrary, but does need to satisfy the condition that the derivative of f-1 is proportional to x^-2 for large x. (What I'm referring to as f-1 would be his f.)

Thanks, atyy!
 

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