Covariant derivatives in Wolfram Math

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The discussion centers on covariant derivatives in spherical coordinates as presented in Wolfram Mathworld, specifically questioning the vectors represented by A_r, A_theta, and A_phi. It clarifies that these derivatives can be computed for any covariant tensor, with the indices corresponding to the spherical coordinates. An example provided is the Coulomb force, where A_r is defined as CQ/r^2, while A_theta and A_phi are zero. The conversation also notes that any vector can be transformed into spherical coordinates, but calculations become complex without spherical symmetry. Understanding the proper use of Christoffel symbols is emphasized for accurate computations in this context.
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In the Wolfram Mathworld section on spherical coordinates there's given a list of nine covariant derivatives. The derivatives are given with respect to radius, azmuth, and zenith using the usual symbols r, theta and phi. The question is: what would be examples of the vectors whose derivatives are taken, sybolized by A(subscript)r, A(subscript)theta, and A(subscript)phi. These vectors appear explicitly on the right side of the equations. I would have expected the covariant derivatives to be of the position vector parameterized by r, theta, and phi, but not so. Anyone?
 
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In the Wolfram Mathworld section on spherical coordinates there's given a list of nine covariant derivatives. The derivatives are given with respect to radius, azmuth, and zenith using the usual symbols r, theta and phi. The question is: what would be examples of the vectors whose derivatives are taken, sybolized by A(subscript)r, A(subscript)theta, and A(subscript)phi. These vectors appear explicitly on the right side of the equations. I would have expected the covariant derivatives to be of the position vector parameterized by r, theta, and phi, but not so. Anyone?

You may compute covariant derivative for any covarinat tensor, and in this case for A_i. As expressions are in spherical coordinate system then subscript i must agree with names of coordinates, so then i \in {r,\theta, \phi}. You may treat it as usual as with {x,y,z}. The proper use of Christoffel symbols, and covariant derivatives is exactly for this - for computing with this coefficients as close as in Cartesian system.
So You ask for example of vector You may put into this formulas. Here You are ( please make some picture): simple Culomb force, notice angular parts are vanish so, it is easy to compute with it just exactly in spherical coordinates:

<br /> A_r = CQ/r^2<br />
<br /> A_{\phi} = 0<br />
<br /> A_{\theta} = 0<br />

Here is picture of something similar:
index.jpeg

Of course You may substitute anything You want for A_{r},A_{\theta},A_{\phi}, then You may obtain interesting vector fields. If You have Sage computing environment You may create some pictures with it: http://www.sagenb.org/home/pub/216/

Any vector (A_x,A_y,A_z) may be described in spherical coordinate system by taking simple and well known transformation between coordinate systems, but when there is no spherical symmetry this may be a paint to compute with it.

Best regards ;-)
Kazek
 
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I am studying the mathematical formalism behind non-commutative geometry approach to quantum gravity. I was reading about Hopf algebras and their Drinfeld twist with a specific example of the Moyal-Weyl twist defined as F=exp(-iλ/2θ^(μν)∂_μ⊗∂_ν) where λ is a constant parametar and θ antisymmetric constant tensor. {∂_μ} is the basis of the tangent vector space over the underlying spacetime Now, from my understanding the enveloping algebra which appears in the definition of the Hopf algebra...

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