Ricci scalar and curveture of FRW metric

In summary, the conversation discusses the homogeneity and isotropy of the universe, described by the FRW metric with a constant curvature parameter, k. However, the Ricci scalar, obtained from the Einstein equation, is a function of time, leading to the Friedman equation. This raises confusion about the constant curvature of the universe. The distinction between spatial and spacetime curvature is explained, with the former being constant in the FRW model and the latter varying with time. The conversation also mentions the work of Kolb on the early universe and the interpretation of "constant curvature" in cosmological models.
  • #1
sadegh4137
72
0
hi

we know that our universe is homogenous and isotropic in large scale.
the metric describe these conditions is FRW metric.
In FRW, we have constant,k, that represent the surveture of space.
it can be 1,0,-1.
but the the Einstan Eq, Ricci scalar is obtained as function of time! and this leads to Frideman Eq.
I sonfuse about this. the curveture of universe is constant or not!
 
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  • #2
sadegh4137 said:
hi

we know that our universe is homogenous and isotropic in large scale.
the metric describe these conditions is FRW metric.
In FRW, we have constant,k, that represent the surveture of space.
it can be 1,0,-1.
but the the Einstan Eq, Ricci scalar is obtained as function of time! and this leads to Frideman Eq.
I sonfuse about this. the curveture of universe is constant or not!
You must make a distinction between the curvature of the spatial three dimensional hypersurface, that has constant curvature in the FRW universe, and the 4-dimensional spacetime curvature that doesn't have constant curvature in that model.
 
  • #3
yes i know
in The early universe is written by kolb in chapter 3
auther stayed that Ricci tensor in the special space is 6k/a(t)
I can't understand this!
 
  • #4
"Constant curvature" means that the curvature of a space section is the same everywhere, i.e. independent of x,y,z. At a given instant, it's the same everywhere, like a sphere. In cosmological models the curvature of the space section varies with time.
 
  • #5


I can understand your confusion regarding the Ricci scalar and the curvature of the FRW metric. Let me explain it in simpler terms. The FRW metric is a mathematical representation of the homogeneity and isotropy of our universe on a large scale. This metric has a constant, represented by the letter 'k', which determines the curvature of space. This constant can take on values of 1, 0, or -1.

Now, the Einstein equations are a set of equations that describe the relationship between the curvature of space and the energy and matter present in the universe. The Ricci scalar is a mathematical quantity that is derived from these equations and is used to measure the curvature of space at a specific point in time.

It is important to note that the curvature of space is not constant, it can change over time. This is why the Ricci scalar is a function of time in the FRW metric. The Friedman equation, which is derived from the Einstein equations, relates the curvature of space to the energy and matter present in the universe.

In summary, the curvature of the universe is not constant, but it is described by a constant in the FRW metric. The Ricci scalar is a function of time and is used to measure the curvature of space at a specific point in time. I hope this helps clarify your confusion.
 

1. What is the Ricci scalar and curvature of FRW metric?

The Ricci scalar and curvature of FRW metric are mathematical quantities used to describe the geometry of the universe in the context of the Friedmann-Robertson-Walker (FRW) metric. The Ricci scalar is a measure of the intrinsic curvature of a space, while the curvature of FRW metric describes the overall shape of the universe.

2. How do the Ricci scalar and curvature of FRW metric relate to the expansion of the universe?

The Ricci scalar and curvature of FRW metric are closely related to the expansion of the universe. As the universe expands, the curvature decreases, and the Ricci scalar becomes more negative. This is due to the fact that the expansion of the universe stretches the space, making it less curved.

3. What is the significance of the Ricci scalar and curvature of FRW metric in cosmology?

The Ricci scalar and curvature of FRW metric are crucial in understanding the universe on a large scale. They help us to determine the overall geometry of the universe and how it has evolved over time. Additionally, they play a significant role in various cosmological models and theories.

4. How does the value of the Ricci scalar and curvature of FRW metric affect the fate of the universe?

The value of the Ricci scalar and curvature of FRW metric can affect the fate of the universe. If the curvature is positive, the universe will eventually collapse in a "Big Crunch." If the curvature is negative, the universe will continue to expand indefinitely. The value of the Ricci scalar also plays a role in determining the rate of expansion and the overall fate of the universe.

5. Can the Ricci scalar and curvature of FRW metric be measured?

Yes, the Ricci scalar and curvature of FRW metric can be measured using various cosmological observations and experiments. For example, the cosmic microwave background radiation provides valuable data that can be used to determine the curvature of the universe. Additionally, the gravitational lensing effect can also be used to measure the curvature of spacetime.

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