De Sitter space, basic questions

  • Context: Graduate 
  • Thread starter Thread starter binbagsss
  • Start date Start date
  • Tags Tags
    Space
Join the discussion
Ask a follow-up here, or get your own question answered by working scientists, mathematicians and engineers — people, not an autocomplete.
Real named experts · corrections over time · the nuance an AI answer skips
37 replies · 5K views
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.
 
Physics news on Phys.org
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
 
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.
 
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.
 
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.
 
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.
 
  • Like
Likes   Reactions: LoicM
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!
 
Last edited: