Still learning about tensors

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SUMMARY

The covariant derivative of the metric tensor \( g_{\alpha\beta} \) with respect to \( x^{\lambda} \) is always zero under the torsion-free condition applied to the affine connection on the tangent bundle. This is a fundamental aspect of general relativity, where the Christoffel symbols simplify the manipulation of the connection. The expression for the covariant derivative shows that it vanishes due to the symmetry of the metric tensor and the properties of the Levi-Civita connection. Understanding this concept is crucial for grasping the geometric framework of general relativity.

PREREQUISITES
  • Understanding of covariant derivatives in differential geometry
  • Familiarity with the metric tensor and its properties
  • Knowledge of Christoffel symbols and their role in general relativity
  • Basic grasp of tensor notation and manipulation
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  • Study the derivation of the Levi-Civita connection and its implications in general relativity
  • Explore the properties of symmetric tensors and their significance in physics
  • Learn about the relationship between the metric tensor and Christoffel symbols
  • Investigate examples of covariant derivatives for various metric tensors
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Students and professionals in physics, particularly those focusing on general relativity, differential geometry, and tensor calculus. This discussion is beneficial for anyone seeking to deepen their understanding of the mathematical foundations of spacetime and curvature.

  • #31
WannabeNewton said:
In any case, doing it on S^{2} is probably a good way of getting used to it.

You may have noticed that I have posted and deleted twice now. (and now I have edited again, for emphasis) I couldn't seem to get the notation right. But my main point was that if we define a parametric path on the surface of a sphere, (\theta(\lambda),\phi(\lambda))

and you are asked to calculate the length of a differential section of that path, \left \| \left (\frac{\mathrm{d \theta} }{\mathrm{d} \lambda},\frac{\mathrm{d} \phi }{\mathrm{d} \lambda} \right )| \right \| =\sqrt {r^2 \frac{d \theta}{d\lambda}+ r^2 \sin^2(\theta)\frac{d \phi}{d\lambda}}
you need to take into account the unit vectors; (i.e. the scale factors) how long a differential change in theta or phi actually is in the three-dimensional space.

However, if you are just asked for the differential of that path

\frac{\mathrm{d} \vec s }{\mathrm{d} \lambda}=\left (\frac{\mathrm{d \theta} }{\mathrm{d} \lambda},\frac{\mathrm{d} \phi }{\mathrm{d} \lambda} \right )

you don't need to take into account how long the unit vectors are in the theta direction or phi direction, because the coordinates of the path already take that into account.

In particular, \frac{\mathrm{d} \vec s}{\mathrm{d} r},\frac{\mathrm{d} \vec s}{\mathrm{d} \theta}, \, \mathrm{and}\, \frac{\mathrm{d} \vec s}{\mathrm{d} \phi}
should be identical to \frac{\partial \vec s}{\partial r},\frac{\partial \vec s}{\partial \theta}, \, \mathrm{and}\, \frac{\partial \vec s}{\partial \phi}.

If there is no flaw in my reasoning, this seems to directly conflict with:
d _{\alpha }\mathbf{\overrightarrow{V}} = \left (\partial _{\alpha }V^{\beta } \right )\overrightarrow{e_{\beta }} + V^{\beta }\left (\partial _{\alpha }\overrightarrow{e_{\beta }} \right )

This equation also appears in various forms as equations 1a, 1b, 2a, 2b, here: http://www.mathpages.com/rr/appendix/appendix.htm
surely there must be a simply explained flaw in either my reasoning, or my understanding of what is meant.
 
Last edited:

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