Integration of Ricci Scalar Over Surface

In summary, the integration of the Ricci scalar over a surface applies in general, but on non-compact surfaces, it may fail to converge. This can be seen in the example of hyperbolic space. To prove the formula, there are different approaches such as considering order-of-limits or compacification with a point or curve at infinity. In the non-compact case where the integral converges, the total curvature can be less than 2π multiplied by the Euler characteristic of the surface. For a compact manifold with boundary, the total geodesic curvature of the bounding curve must be added to the integral. The flat plane is an example of a surface with zero total curvature but Euler characteristic of 1.
  • #1
darida
37
1
Does this integration of Ricci scalar over surface apply in general or just for compact surfaces?

∫RdS = χ(g)

where χ(g) is Euler characteristic.
And could anybody give me some good references to prove the formula?
 
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  • #2
On a non-compact surface, the integral might fail to converge. Take hyperbolic space, for example.
 
  • #3
This might still be true when the integral converges though ?
 
  • #4
I'm not sure.

Another way to look at this is an order-of-limits issue. Consider a modified integral for computing the Euler number of manifolds-with-boundary. This integral will contain a boundary term (sorry, I don't remember what it looks like). Then you can take any non-compact surface, and just cut a piece out of it, adding a boundary and making the integral finite. Perform the integral first, and then take the limit as the boundary goes to infinity.

I think this will give you an Euler number of 1 for the infinite plane. It is homologous to the disk, and boundaries add 1 to the Euler number.
 
  • #5
For a non compact surface, I was more thinking of compacification with a point/curve at infinity and hopefully making use of R=0 at infinity... But you're right the boundary term can make this whole business tricky.
 
  • #6
In the non-compact case where the integral does converge, the total curvature can be less than 2πχ(S).

The flat plane has zero total curvature 0 but has Euler characteristic 1.

For a compact manifold with boundary one needs to add on the total geodesic curvature of the bounding curve.
 
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Related to Integration of Ricci Scalar Over Surface

1. What is the Ricci scalar?

The Ricci scalar, denoted as R, is a mathematical quantity that describes the curvature of a space. It is an essential component of the Einstein field equations, which describe the relationship between the curvature of space and the distribution of matter and energy in the universe.

2. What does it mean to integrate the Ricci scalar over a surface?

Integrating the Ricci scalar over a surface means calculating the total curvature of that surface. This is done by taking small sections of the surface and adding up their individual curvatures. The result is a single value that represents the overall curvature of the entire surface.

3. Why is it important to integrate the Ricci scalar over a surface?

Integrating the Ricci scalar over a surface is important because it allows us to understand the overall curvature of a space. This information is crucial in many areas of physics, such as general relativity and cosmology, where the curvature of space plays a significant role in the behavior of matter and energy.

4. How is the integration of the Ricci scalar related to the concept of manifolds?

The integration of the Ricci scalar over a surface is closely related to the concept of manifolds. Manifolds are mathematical objects that describe the curvature and topology of a space. By integrating the Ricci scalar over a manifold, we can determine the total curvature of that space and understand its geometry.

5. What are the applications of integrating the Ricci scalar over a surface?

The integration of the Ricci scalar has many applications in physics and mathematics. It is used in the study of general relativity, cosmology, and differential geometry, among others. It also plays a crucial role in understanding the behavior of matter and energy in curved spaces, such as black holes and the universe as a whole.

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