How to contract the christoffel symbol

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    Christoffel Symbol
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SUMMARY

The discussion focuses on contracting the Christoffel symbols, specifically the expression ##\Gamma^\sigma_{\sigma\mu}##. Participants emphasize the importance of showing intermediate steps to identify errors in calculations. The correct approach involves using the relationship ##g_{\sigma\nu}g^{\sigma\nu}=\delta_\sigma^{~~\sigma}=n##, where ##n## is the dimension of the manifold. A recommended method for progressing is to expand the expression ##\Gamma^\sigma_{\sigma\mu}=\partial_\mu (\ln\sqrt{g})## and to transform to a diagonal metric coordinate system for clarity.

PREREQUISITES
  • Understanding of Christoffel symbols in differential geometry
  • Familiarity with metric tensors and their properties
  • Knowledge of index notation and tensor contraction
  • Basic concepts of manifold dimensions
NEXT STEPS
  • Study the derivation of the Christoffel symbols from the metric tensor
  • Learn about tensor contraction techniques in differential geometry
  • Explore the implications of transforming to a diagonal metric coordinate system
  • Investigate the relationship between the determinant of the metric and the Christoffel symbols
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Mathematicians, physicists, and students studying general relativity or differential geometry who need to understand the manipulation and contraction of Christoffel symbols.

TimeRip496
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http://www.thephysicsforum.com/vlatex/pics/92_db3a451c7d105432675bef473582556e.png

Anyone can help me? I am really stuck at here.
 
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TimeRip496 said:
http://www.thephysicsforum.com/vlatex/pics/92_db3a451c7d105432675bef473582556e.png

Anyone can help me? I am really stuck at here.
Well, you should at least show your work so far, and exactly where you get "stuck". I.e., like in the homework forums.
 
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You might start with writing out how the Christoffel symbols are defined, and then contracting the two indices to see what you get.
 
strangerep said:
Well, you should at least show your work so far, and exactly where you get "stuck". I.e., like in the homework forums.
I get (0.5)(d/dxμ)(gσv)(gσv) . I don't even know to get that ln.

Sorry for my untidiness as I am still new to this.
 
If you don't show your intermediate steps, we can't really tell where you went wrong. By the way ##g_{\sigma\nu}g^{\sigma\nu}=\delta_\sigma^{~~\sigma}=n## where ##n## is the dimension of the manifold. So you definitely went wrong somewhere as your expression is the derivative of a constant so will equal 0.
 
Matterwave said:
If you don't show your intermediate steps, we can't really tell where you went wrong. By the way ##g_{\sigma\nu}g^{\sigma\nu}=\delta_\sigma^{~~\sigma}=n## where ##n## is the dimension of the manifold. So you definitely went wrong somewhere as your expression is the derivative of a constant so will equal 0.
IMG_20150125_142314-1.jpg

I did that by cancelling out the indices.
 
Ok, but your final result ##\Gamma^\sigma_{\sigma\mu}=\frac{1}{2}g^{\sigma\nu}\partial_\mu g_{\sigma\nu}## is very different than the one you wrote in post #4.

You are pretty close to the answer. Perhaps the easiest way to move forward now is to expand the original statement ##\Gamma^\sigma_{\sigma\mu}=\partial_\mu (\ln\sqrt{g})## out to see what that looks like in terms of components ##g_{\mu\nu}## (it will be pretty hard to reverse-engineer this I think). The easiest way to work out the equation in the OP is to transform to a coordinate system in which the metric is diagonal (which can always be done), work out the derivatives in terms of components of the metric in that coordinate system, and then produce an equation which will work in any coordinate system. :)
 
Matterwave said:
Ok, but your final result ##\Gamma^\sigma_{\sigma\mu}=\frac{1}{2}g^{\sigma\nu}\partial_\mu g_{\sigma\nu}## is very different than the one you wrote in post #4.

You are pretty close to the answer. Perhaps the easiest way to move forward now is to expand the original statement ##\Gamma^\sigma_{\sigma\mu}=\partial_\mu (\ln\sqrt{g})## out to see what that looks like in terms of components ##g_{\mu\nu}## (it will be pretty hard to reverse-engineer this I think). The easiest way to work out the equation in the OP is to transform to a coordinate system in which the metric is diagonal (which can always be done), work out the derivatives in terms of components of the metric in that coordinate system, and then produce an equation which will work in any coordinate system. :)
Thanks! I did finally manage to contract it. However, I have difficulty contracting Γσμμ. Is contracting it going to give us the same formula as shown above? I search online but I can't find any contraction of that christoffel symbol given above.
 
TimeRip496 said:
Thanks! I did finally manage to contract it. However, I have difficulty contracting Γσμμ. Is contracting it going to give us the same formula as shown above? I search online but I can't find any contraction of that christoffel symbol given above.

You can't "contract" two indices which are both lower indices. You can only contract one upper index with a lower index. So what you want to look for is actually ##g^{\mu\nu}\Gamma^\rho_{\mu\nu}##. Try writing that out and seeing what it turns out to be.
 

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