De Sitter space, basic questions

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SUMMARY

The discussion centers on the properties of de Sitter space and its various coordinate charts, particularly in relation to the cosmological constant (Λ). For Λ > 0, the solutions for k = -1, 0, and 1 describe the same spacetime, while for Λ < 0, the geometry is classified as anti-de Sitter space. The scale factor's dynamics depend on the chosen coordinate chart, with the "comoving" chart being significant for observers in a dark energy-dominated universe. The geometry of de Sitter space cannot be simply categorized as open, closed, or flat, as these properties pertain to spacelike slices rather than the entire spacetime.

PREREQUISITES
  • Understanding of cosmological constants and their implications in general relativity.
  • Familiarity with coordinate transformations in spacetime geometry.
  • Knowledge of Friedmann equations and their role in cosmological models.
  • Basic concepts of homogeneous and isotropic universes.
NEXT STEPS
  • Study the properties of anti-de Sitter space and its applications in theoretical physics.
  • Explore the Friedmann equations in detail, focusing on dark energy models.
  • Investigate the implications of different coordinate charts on the dynamics of cosmological models.
  • Learn about the concept of comoving observers and their significance in cosmology.
USEFUL FOR

The discussion is beneficial for theoretical physicists, cosmologists, and students of general relativity who are interested in the dynamics of spacetime and the implications of dark energy in the universe.

  • #31
binbagsss said:
Since the different ##k## values correspond to a different space-like slicing - coordinate chart - can you conclude that the observers have relative motion as different coordinate charts give a rise to different relative velocities?

In de Sitter spacetime, observers at rest in one of the three charts are not at rest in the other two. That's all you need to conclude that observers at rest in each of the charts are in relative motion.
 
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  • #32
PeterDonis said:
In de Sitter spacetime, observers at rest in one of the three charts are not at rest in the other two. .
But how do we know this?
Or do you have any references stating it, thanks
 
  • #33
binbagsss said:
how do we know this?

By looking at how worldlines that are at rest in one chart transform into the other charts.
 
  • #34
PeterDonis said:
By looking at how worldlines that are at rest in one chart transform into the other charts.
PeterDonis said:
There are solutions where the "comoving" observers see k=1, solutions where they see k=-1, and solutions where they see k=0. It just happens that the solution that (as far as we can tell) describes our actual universe is the one in which comoving observers see k=0.

Do you know of any sources that state certain compositions and then the corresponding curvature/coordinate chart ? (for the obsevers that view the universe as isotropic and homoenous). Thanks.
 
  • #35
binbagsss said:
Do you know of any sources that state certain compositions

I don't know what you mean by "compositions". Many references discuss the FRW charts for all three values of k and the corresponding curvature components. For example, Carroll's lecture notes, IIRC, go into this.
 
  • #36
PeterDonis said:
I don't know what you mean by "compositions". Many references discuss the FRW charts for all three values of k and the corresponding curvature components. For example, Carroll's lecture notes, IIRC, go into this.
Apologies I meant different distributions of the matte/radiation/ dark-energy.
 
  • #37
binbagsss said:
I meant different distributions of the matte/radiation/ dark-energy.

Carroll's notes discuss this too, at least with respect to the most basic cases--ordinary non-relativistic matter, radiation, and dark energy.
 
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  • #38
Another very good reference for the same topic is "V.Mukhanov : Physical foundations of Cosmology", §1.3.6. On pp.33-34 is actually a very simple and intuitive solution giving the results described by binbagss in his initial message.

http://www.astro.caltech.edu/~george/ay21/readings/Mukhanov_PhysFoundCosm.pdf

I would like to thank binbagss for his very good questions and especially PeterDonis for his detailed and clear explanations!
 
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