Bianchi Models and Kantowski-Sachs

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In summary, Bianchi and Kantowski-Sachs models are both examples of homogeneous and isotropic universes with different symmetry groups. Bianchi models have a 3-parameter group, while Kantowski-Sachs has a 4-parameter group due to its additional symmetry axis. Both models have different types corresponding to different types of Lie algebras.
  • #1
utku
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What are main differencies between Bianchi models and Kantowski-Sachs models.
Can anyone give mathematical definition clearly and possibly simple form?
 
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Both Bianchi and Kantowski-Sachs cosmologies are homogeneous and isotropic. Hiomogeneous means that for each space section, there's a symmetry operation that maps any point P into any other point Q. Bianchi cosmologies are simply transitive, meaning that there's only one symmetry mapping P into Q. Consequently for Bianchi types the symmetry groups are 3-parameter groups. There are nine different types, corresponding to the nine different types of 3-parameter Lie algebras.
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Kantowski-Sachs
is an example of a homogeneous, isotropic universe with a symmetry group that is multiply transitive. It has a 4-parameter group: SO(3) x R, rotations on a sphere and translations along an axis.
 
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  • #3
Thanks for your reply.
I think you want to say homogeneous and anisotropic spaces.
 
  • #4
Thanks Bill_K,

Can you express more explicitly the term 3-parameters and 4-parameters groups please?

thanks.
 
  • #5
utku said:
I think you want to say homogeneous and anisotropic spaces.
Yes, I meant ANisotropic, in both places! :redface: Thanks!

utku said:
Can you express more explicitly the term 3-parameters and 4-parameters groups please?
The number of parameters in a group is the number of variables you need to specify to pick out a particular group element. For example the usual group of 3-d rotations acting on a sphere S - you can rotate the North pole P into any other point Q on the sphere, and you must give the latitude and longitude of Q - that's two parameters. But after doing that, you can still rotate through some angle ψ about Q, keeping Q fixed. That's a total of three parameters. And the group action on S is multiply transitive - since ψ can be anything, there are many group elements that map P into Q.

The space section of a Bianchi cosmology has a 3-parameter symmetry group, because you can map P into any other point Q, and this time Q needs three coordinates to label it - x, y, z for example. And there is no further symmetry, you can't rotate about Q due to the anisotropy. So the action is simply transitive.

The Kantowski-Sachs cosmology has one more parameter - there's a symmetry axis at each point, so you can hold Q fixed and rotate through angle ψ about this axis - making it multiply transitive.
 
  • #6
Thanks Bill_K,
Your answer is very usefull for me. I understood many of your reply :)
 

Related to Bianchi Models and Kantowski-Sachs

1. What are Bianchi models?

Bianchi models are a class of cosmological models in which the universe is homogeneous and anisotropic, meaning that it appears the same in all directions but not necessarily in the same way. These models are important in understanding the large-scale structure of the universe.

2. How do Bianchi models differ from the standard cosmological model?

The standard cosmological model, known as the Lambda-CDM model, assumes that the universe is both homogeneous and isotropic, meaning that it appears the same in all directions and in the same way. Bianchi models, on the other hand, allow for anisotropy, which can have significant effects on the evolution of the universe.

3. What is the Kantowski-Sachs metric?

The Kantowski-Sachs metric is a mathematical description of the spacetime geometry in Bianchi models. It is a special case of the more general Bianchi metric and is characterized by its anisotropic expansion rates in different directions.

4. What is the significance of the Kantowski-Sachs metric?

The Kantowski-Sachs metric is significant because it allows for anisotropic expansion, which can have important implications for the evolution of the universe. It also allows for more complex and realistic models than the standard cosmological model, which can help us better understand the behavior of the universe.

5. How do Bianchi models and Kantowski-Sachs metric relate to the observable universe?

Bianchi models and the Kantowski-Sachs metric are important tools for studying the large-scale structure of the universe. By comparing the predictions of these models to observations of the observable universe, we can better understand the evolution of the universe and its properties, such as the distribution of matter and energy.

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