Geometry of Inflationary Universe?

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SUMMARY

The discussion centers on the Geometry of the Inflationary Universe, emphasizing that our Observable Universe is a small segment of the total universe formed during the Big Bang. It posits that while the observable universe appears flat, the entire universe may resemble a balloon's shape. The conversation explores the implications of different observers having unique observable universes due to the finite speed of light and the universe's finite age, leading to a homogeneous and isotropic universe despite varying perspectives.

PREREQUISITES
  • Understanding of Inflation Theory
  • Familiarity with the concept of the Observable Universe
  • Knowledge of light cones and their implications in cosmology
  • Basic grasp of homogeneity and isotropy in the universe
NEXT STEPS
  • Research the implications of Inflation Theory on cosmic structure formation
  • Explore the concept of light cones in relation to different observers in cosmology
  • Study the principles of homogeneity and isotropy in the context of the universe
  • Investigate the potential shapes of the universe beyond the observable limits
USEFUL FOR

Astronomers, cosmologists, and physics enthusiasts interested in the structure and geometry of the universe, as well as those exploring the implications of Inflation Theory on observable phenomena.

Octavianus
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According to the Inflation Theory our Observable Universe is but a small part of the total universe created in the Big Bang.
Our observable universe appears to be flat (just like Earth at sea level may appear flat), while the total universe may be shaped like a balloon.
If we assume our observable universe was at one specific area in the pre-inflation universe, and other areas are now other universes no longer in causal contact with our universe, what lies between the universes?
Is there a uniform distribution of mass in the total universe, with each universe just being defined by how far one can observe in any direction? So our observable universe is slightly different from the observable universe of any sentient beings in the Andromeda galaxy?
Or is the observable universes like a galaxies or galaxy clusters, with vast expanses of empty space between them?
 
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Octavianus, the observable universe just represents all that an observer can see, his light cone. Since light has a finite speed, and the universe is of finite age, you can only see so much. Different observers obviously have different observable universes, it is purely dependent on where you are located and how long the universe has existed. So, the universe is homogeneous and isotropic, regardless of your observable universe.
 

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