Understanding de Sitter Space: FRW or Hyperboloid?

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SUMMARY

The discussion focuses on understanding de Sitter space, specifically its representation as either a hyperboloid in Minkowski space or as an FRW cosmology with the scale factor a(t) = exp(Ht). Participants clarify that the confusion arises from the coordinate transformation between these two representations. The de Sitter metric can indeed be expressed as an FRW metric, but the choice of coordinates plays a crucial role in this interpretation. Key references include equations from Mukhanov's work, highlighting the mathematical nuances involved in these descriptions.

PREREQUISITES
  • Understanding of de Sitter space and its properties
  • Familiarity with FRW cosmology and scale factors
  • Knowledge of Minkowski space and hyperboloid geometry
  • Basic grasp of coordinate transformations in cosmology
NEXT STEPS
  • Study the mathematical foundations of de Sitter space in "Quantum Fluctuations in the Early Universe" by Mukhanov
  • Explore the implications of the FRW metric in cosmological models
  • Learn about coordinate transformations and their effects on cosmological metrics
  • Review the de Sitter metric forms in Wald's and Carroll's texts for deeper insights
USEFUL FOR

Cosmologists, theoretical physicists, and students of general relativity seeking to deepen their understanding of de Sitter space and its implications in cosmological models.

ramparts
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Hey all - I'm trying to get a better qualitative understanding of de Sitter space, and I'm a bit confused about the de Sitter universe. I've always seen it mathematically as a hyperboloid embedded in a higher-dimensional Minkowski space (with some annoying metric I've forgotten) but I've read (alright, fine, on Wikipedia :P) that a patch of de Sitter universe can be expressed as an FRW cosmology with a(t) = exp(Ht) - So... under that description, why is the de Sitter metric not just an FRW metric with that scale factor?
 
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I always did understand de Sitter space through its cosmological description - a flat, vacuum filled universe that undergoes exponential expansion (equivalently, constant Hubble parameter). What about this description is unsatisfactory?
 
Thanks George! Don't have my Wald or Carroll with me so I couldn't look it up...

The problem was that I was used to seeing the de Sitter metric in a form similar to eqn 1.94 in George's link, so I was a bit confused by the description of it as a FRW cosmology with a=exp(Ht). The coordinate transformation makes sense (or will, when I think about it some more :)).
 

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