Unifying Curvatures with Riemann Tensor

In summary, the Riemann Tensor symbols can be used to unify the definitions of curvatures for both curves and surfaces. For surfaces, R_{1,2,1,2} corresponds to the Gaussian curvature, while R_{1,1,1,1}=0. This is because R_{i,j,k,l} measures the curvature of a manifold, while k_1 and k_2 are the main curvatures of a curve. Additionally, the Gaussian curvature of a 1-D curve can be calculated by embedding it in a higher dimensional manifold and using the Gauss-Codazzi equation.
  • #1
bchui
42
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I always wonder how the definitions of curvatures of curves and surfaces be unified by the Riemann Tensor symbols.
For surfaces, I know R_{1,2,1,2} corresponds to the Gaussian curvature of a surface. How come R_{1,1,1,1}=0 and not corresponds to the curvature of a curve in \RE^2 or in \Re^3 ?:confused:
 
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  • #2
Recall that:

[tex]R_{ijkl}=\dfrac{\partial \Gamma_{ijl}}{\partial u^k}- \dfrac{\partial \Gamma_{ijk}}{\partial u^l}+\Gamma^h_{ik}\Gamma_{jhl}-\Gamma^h_{il}\Gamma_{jhk}[/tex]

So that:

[tex]R_{1111}=\dfrac{\partial \Gamma_{111}}{\partial u^1}-\dfrac{\partial \Gamma_{111}}{\partial u^1}+\Gamma^h_{11}\Gamma_{1h1}-\Gamma^h_{11}\Gamma_{1h1}\\
=0[/tex]

For any finite dimensional Riemannian manifold. Moreover, we can still calculate the Gaussian curvature, [tex]K[/tex] for a 1-D curve via

[tex]K=-\dfrac{R_{1212}}{\text{det}g}[/tex]

by first viewing the curve as an embedding in a higher dimesional manifold, in particular [tex]\mathbb{R}^2[/tex] or higher--which is possible via the Nash-Kuiper theorem--allowing the appropriate number of terms to appear in the calculation.

There you have it!
 
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  • #3
How about the curvature of a curve on the plane?
Applying Gauss-Codazzi equation and we have [tex]R_{1,1,1,1}=0[/tex] and the Gaussian curvature of the plane [tex]\Re^2[/tex] is also zero!
The difference is that the curvatures of curves are the "main curvatures" [tex]k_1,k_2[/tex] while the "curvature tensors" [tex]R_{i,j,k,l}[/tex] has something to do with the Gaussian curvatures [tex]K=k_1k_2[/tex]
 

FAQ: Unifying Curvatures with Riemann Tensor

1. What is the Riemann Tensor and how does it relate to unifying curvatures?

The Riemann Tensor, also known as the Riemann Curvature Tensor, is a mathematical object used to describe the curvature of a space. It is a fundamental concept in differential geometry and plays a crucial role in Einstein's theory of general relativity. The Riemann Tensor is used to unify different types of curvatures, such as the Gaussian curvature and mean curvature, into a single mathematical framework.

2. How is the Riemann Tensor calculated?

The Riemann Tensor is calculated using the Christoffel symbols, which are derived from the metric tensor. The metric tensor describes the geometry of a space, and the Christoffel symbols are used to calculate the derivatives of the metric tensor. These derivatives are then used to calculate the components of the Riemann Tensor, which describes the curvature of the space at each point.

3. What is the significance of unifying curvatures with the Riemann Tensor?

By unifying different types of curvatures with the Riemann Tensor, we can better understand the geometry of a space and how it is affected by matter and energy. This has important implications in the study of gravity and the behavior of objects in space, as well as in other fields such as cosmology and astrophysics.

4. Can the Riemann Tensor be applied to any type of space?

Yes, the Riemann Tensor can be applied to any type of space, whether it is flat, curved, or even higher-dimensional. It is a fundamental concept in differential geometry and has applications in various fields, such as physics, mathematics, and engineering.

5. How is the Riemann Tensor used in Einstein's theory of general relativity?

In general relativity, the Riemann Tensor is used to describe the curvature of spacetime and how it is affected by the presence of matter and energy. This allows us to understand the behavior of gravity and the motion of objects in the universe. The Riemann Tensor is a key component of Einstein's field equations, which relate the curvature of spacetime to the distribution of matter and energy.

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