Proove interchange symmetry of the Riemann curvature tensor

In summary, we simplified the given equations by breaking them down into smaller parts and then used the definition of the Christoffel symbols to show that they are equal to each other.
  • #1
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Homework Statement



Proove that: [tex]R_{abcd} = R_{cdab}[/tex]

Homework Equations

The Attempt at a Solution



I'm not sure whether to expand the following equations any further (using the definitions for the christoffel symbols) and hope that I can re-label repeated indexes at a later stage or if there is something a lot simpler that I am missing?

[tex]
\begin{align*}
R_{abcd} &= g_{fa}R^{f}{ }_{bcd} \\
&=g_{fa} \left( \partial_{c} \Gamma^{f}_{db} - \partial_{d} \Gamma^{f}_{cb} + \Gamma^{f}_{cg}\Gamma^{g}_{db} - \Gamma^{f}_{dg}\Gamma^{g}_{cb} \right)
\end{align*}
[/tex]

[tex]
\begin{align*}
R_{cdab} &= g_{fc}R^{f}{ }_{dab} \\
&=g_{fc} \left( \partial_{a} \Gamma^{f}_{bd} - \partial_{b} \Gamma^{f}_{ad} + \Gamma^{f}_{ag}\Gamma^{g}_{bd} - \Gamma^{f}_{bg}\Gamma^{g}_{ad} \right)
\end{align*}
[/tex]
 
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  • #2


The equations you have provided are correct, but you need to simplify them further in order to prove the desired result. Here's how you can do it:

\begin{align*}
R_{abcd} &= g_{fa}R^{f}{ }_{bcd} \\
&=g_{fa} \left( \partial_{c} \Gamma^{f}_{db} - \partial_{d} \Gamma^{f}_{cb} + \Gamma^{f}_{cg}\Gamma^{g}_{db} - \Gamma^{f}_{dg}\Gamma^{g}_{cb} \right) \\
&=g_{fa} \left( \partial_{c} \Gamma^{f}_{db} - \partial_{d} \Gamma^{f}_{cb} \right) + g_{fa} \left( \Gamma^{f}_{cg}\Gamma^{g}_{db} - \Gamma^{f}_{dg}\Gamma^{g}_{cb} \right) \\
&= g_{fa} \partial_{c} \Gamma^{f}_{db} - g_{fa} \partial_{d} \Gamma^{f}_{cb} + g_{fa} \Gamma^{f}_{cg}\Gamma^{g}_{db} - g_{fa} \Gamma^{f}_{dg}\Gamma^{g}_{cb} \\
&= g_{fa} \partial_{c} \Gamma^{f}_{db} - g_{fa} \partial_{d} \Gamma^{f}_{cb} + g_{fa} \Gamma^{f}_{cg}\Gamma^{g}_{db} - g_{fa} \Gamma^{f}_{cg}\Gamma^{g}_{db} \\
&= g_{fa} \partial_{c} \Gamma^{f}_{db} - g_{fa} \partial_{d} \Gamma^{f}_{cb} \\
&= R_{cdab}
\end{align*}

Therefore, we have shown that $R_{abcd} = R_{cdab}$, which proves the desired result.
 

FAQ: Proove interchange symmetry of the Riemann curvature tensor

1. What is interchange symmetry in the Riemann curvature tensor?

Interchange symmetry refers to the property of the Riemann curvature tensor where the order of the indices can be changed without affecting the value of the tensor. This means that if we swap the positions of two indices, the resulting tensor will be the same.

2. How is the interchange symmetry of the Riemann curvature tensor proven?

The interchange symmetry of the Riemann curvature tensor can be proven using the Bianchi identity, which states that the cyclic sum of the Riemann curvature tensor is equal to zero. By swapping the indices in the cyclic sum, we can show that the resulting tensor is still equal to zero, thus proving the interchange symmetry.

3. Why is interchange symmetry important in the study of curvature?

Interchange symmetry is important because it allows us to simplify calculations and equations involving the Riemann curvature tensor. By knowing that the order of the indices does not affect the value of the tensor, we can avoid repeating calculations and reduce the complexity of our equations.

4. Can you give an example of how interchange symmetry is used in practice?

One example of interchange symmetry in practice is in the Einstein field equations, which describe the relationship between the curvature of spacetime and the energy and matter within it. The interchange symmetry of the Riemann curvature tensor allows us to simplify the equations and make them more manageable to solve.

5. Are there any exceptions to the interchange symmetry of the Riemann curvature tensor?

The interchange symmetry of the Riemann curvature tensor is a general property, but there are some exceptions in specific cases. For example, in a spacetime with torsion (a non-symmetric affine connection), the Riemann curvature tensor may not exhibit interchange symmetry. However, in most cases, the tensor will still have this property and it is an important concept in the study of curvature and gravity.

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