Choice of scaling function for Penrose diagrams

In summary, the standard definition of coordinates on Penrose diagrams involves a tangent function, which is also used in the transformation given by Wikipedia, Hawking and Ellis. However, it is not explained why the tangent function is specifically used. It is necessary for the transformation to be a homeomorphism from a finite, open interval of the reals onto the whole real line. Other functions such as f=tan^3 or f(x)=-x/[(x-1)(x+1)] could also be used. The tangent function is visually compelling due to its use in the cylindrical embedding, but it is otherwise arbitrary. The embedding in 5 or 6 dimensions may not have observable physical significance, but it can help in understanding the
  • #1
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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  • #2
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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  • #3
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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  • #4
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.
 
  • #5
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?
 
  • #7
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.
 
  • #8
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!
 

Related to Choice of scaling function for Penrose diagrams

1. What is a scaling function in Penrose diagrams?

A scaling function in Penrose diagrams is a mathematical function used to transform the coordinates of a spacetime diagram in order to better visualize the structure and properties of the spacetime. It is commonly used in the study of black holes and other astronomical phenomena.

2. How is the scaling function chosen for a Penrose diagram?

The choice of scaling function for a Penrose diagram depends on the specific properties and features of the spacetime being studied. It is often chosen based on mathematical convenience and the desired visualization of the spacetime's structure.

3. What are the different types of scaling functions used in Penrose diagrams?

Some common types of scaling functions used in Penrose diagrams include logarithmic, power-law, and hyperbolic functions. Each type of function has its own advantages and is chosen based on the specific needs of the analysis.

4. How do scaling functions affect the interpretation of a Penrose diagram?

Scaling functions play a crucial role in the interpretation of a Penrose diagram. They can change the apparent shape and structure of the diagram, making certain features more prominent or obscuring others. The choice of scaling function can also affect how different regions of the spacetime are represented in the diagram.

5. Can the choice of scaling function affect the conclusions drawn from a Penrose diagram?

Yes, the choice of scaling function can have a significant impact on the conclusions drawn from a Penrose diagram. It can affect the visibility and interpretation of important features and can also alter the perceived relationships between different regions of the spacetime. Therefore, it is important to carefully consider the choice of scaling function when analyzing a Penrose diagram.

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