Part of universe mapped by coordinates

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SUMMARY

The discussion centers on the mapping of coordinates in a positively curved universe, specifically the radial coordinate r, which ranges from 0 to 1. Participants debate whether this range indicates a local map or if it reflects the full radius of the manifold, normalized to r_max = 1. The conversation references the Robertson-Walker metric as described in Kolb & Turner, highlighting that only half of the sphere may be mapped. The implications of coordinate choices on the line element as r approaches one are also examined.

PREREQUISITES
  • Understanding of positively curved universes and their properties
  • Familiarity with the Robertson-Walker metric
  • Knowledge of differential geometry concepts, particularly diffeomorphism
  • Basic comprehension of spherical coordinates and their applications
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  • Study the implications of the Robertson-Walker metric in cosmology
  • Explore the concept of diffeomorphism in the context of curved manifolds
  • Investigate the geometry of 3-spheres and their coordinate systems
  • Learn about the effects of coordinate normalization in general relativity
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Cosmologists, theoretical physicists, and students of general relativity who are interested in the geometric properties of the universe and the implications of coordinate systems in cosmological models.

bloby
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I read in a positively curved universe the radial r coordinate ranges from 0 to 1. Is it just a local map?
 
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bloby said:
I read in a positively curved universe the radial r coordinate ranges from 0 to 1. Is it just a local map?
Why do you suggest that it's a local map? Because the value of r ranges only from 0 to 1? Sounds to me like r is ranging over the full radius of the manifold, and is simply normalized so that r_max = 1. However, without context or more detail, I can't be of any more help.
 
bapowell said:
However, without context or more detail, I can't be of any more help.

In Kolb&Turner and in my cours the coordinates of a point on a 3-sphere are the projection on an hyperplane (the equatorial plane if on a 2-sphere). They construct the Robertson-Walker metric for positive curvature this way. But then only one half of the sphere is mapped, isn't it? The huge value the line element takes when r tends to one or R(you are right it's normalized r) is simply the consequence of the choice of coordinates? (Forgive me for my bad english)((If you live on the North, to name a point, of a 2-sphere you can map each points by an angle and a length (->r*pi) or even a comoving length (r/R*pi) but these are not the usual coordinates, aren't they?))

I suggest that it's a local map because I read a constant positive curvature means the universe is "only" diffeomorphic to a 3-sphere.
 

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