Geometry of Inflationary Universe?

In summary, according to the Inflation Theory, the observable universe is just a small part of the total universe created in the Big Bang. The observable universe may appear flat, while the total universe may have a balloon-like shape. It is believed that there are other universes beyond our observable universe, and they are no longer in causal contact with us. The distribution of mass in the total universe is assumed to be uniform, and each universe is defined by the observer's ability to see in any direction. This means that our observable universe may be different from the observable universe of other sentient beings in other galaxies. The observable universes are like galaxies or galaxy clusters with vast empty spaces between them. The universe is considered to be homogeneous and isotropic
  • #1
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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  • #2
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.
 

What is the "Geometry of Inflationary Universe?"

The "Geometry of Inflationary Universe" refers to the shape or structure of the universe during the inflationary period, which is a hypothetical rapid expansion that occurred in the early stages of the universe.

What evidence supports the existence of an inflationary period?

Several pieces of evidence support the idea of an inflationary period, including the uniformity of the cosmic microwave background radiation, the flatness of the universe, and the lack of certain predicted relics from the Big Bang.

How does the geometry of the universe affect its expansion?

The geometry of the universe plays a crucial role in determining its expansion rate. If the universe has a positive curvature, it will eventually stop expanding and collapse in a "Big Crunch." If it has a negative curvature, it will continue to expand forever. A flat universe, however, will continue to expand at a decreasing rate.

What is the relationship between the geometry of the universe and the amount of matter in it?

The geometry of the universe is closely linked to the amount of matter it contains. A higher density of matter leads to a positive curvature, while a lower density results in a negative curvature. This is known as the critical density of the universe.

How does the geometry of the universe affect the formation and distribution of galaxies?

The geometry of the universe has a significant impact on the formation and distribution of galaxies. If the universe has a positive curvature, galaxies will be clustered together in a closed space. A negative curvature would result in a more spread out distribution, while a flat universe would have a more uniform distribution of galaxies.

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