Gradient Tensor of a vector field

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Discussion Overview

The discussion revolves around the computation of the gradient tensor of a vector field expressed in spherical coordinates. Participants explore the use of covariant derivatives and the implications of contravariant versus covariant vectors in this context.

Discussion Character

  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant presents a vector field in spherical coordinates and expresses confusion over computing its gradient tensor using the covariant derivative.
  • Another participant questions whether the vector in question is contravariant or covariant, suggesting that this distinction may lead to errors in calculations.
  • There is a discussion about the correct form of the covariant derivative for contravariant tensors, with references to different sources leading to conflicting formulas.
  • Participants explore the implications of the Christoffel symbols in the calculations, particularly how they affect the terms in the gradient tensor.
  • One participant expresses uncertainty about the derivation of the gradient tensor, despite having a solution, and seeks clarification on the additional terms appearing in their calculations compared to those in a referenced paper.
  • Another participant acknowledges a sign error in their earlier calculations, which they believe does not affect the validity of the result but highlights the complexity of the expressions involved.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the correct application of the covariant derivative or the nature of the vector field. Multiple competing views and interpretations of the formulas remain present throughout the discussion.

Contextual Notes

There are unresolved questions regarding the definitions of contravariant and covariant vectors, the application of the covariant derivative, and the specific forms of the Christoffel symbols used in the calculations. Participants reference different texts, leading to variations in the formulas they apply.

stuxk
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Hi, I'm trying to compute the gradient tensor of a vector field and I must say I'm quite confused. In other words I have a vector field which is given in spherical coordinates as:
\vec{F}=\begin{bmatrix} 0 \\ \frac{1}{\sin\theta}A \\ -B \end{bmatrix}, with A,B some scalar potentials and I want to compute the gradient of the vector.

I found that I have to use the covariant derivative which is given by: \nabla\vec{B}= \frac{\partial{B_p}}{\partial{u^q}} - B_k\Gamma_{pq}^{k}

For some reason I can't get the right results. For instance the tensor element with p=2, q=1 is given as \frac{1}{\sin\theta}\frac{\partial A}{\partial r} = \frac{\partial F_\theta}{\partial r} whereas according the covariant derivative formula should be: \frac{\partial F_\theta}{\partial r} - \frac{1}{r} F_\theta.

Probably I'm doing a big mistake and I think I haven't really understood how I can calculate the gradient tensor. Any help will be appriciated.
 
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\Gamma^a_{bc}=\frac12 g^{ad}\left(\partial_bg_{cd}+\partial_cg_{bd}-\partial_dg_{bc}\right)

Aren't vectors usually contravariant? Does the problem state anything about this? Covariant vectors are usually gradiants or scalar-valued functions?

It turned out that your covariant vector is really contravariant. That may have caused the error.

Below this line is the calculation, so don't look unless you're fine with getting the key.

___________________________________

\nabla_qF^p=\partial_qF^p-\Gamma^p_{qk}F^k

setting p=2, q=1:

\nabla_rF^{\theta}=\partial_rF^{\theta}-\Gamma^{\theta}_{rk}F^k

=\frac{1}{\sin\,\theta}\frac{\partial A}{\partial r}-\Gamma^{\theta}_{rr}F^r-\Gamma^{\theta}_{r\theta}F^{\theta}-\Gamma^{\theta}_{r\phi}F^{\phi}

The metric is g_{rr}=1 , g_{\theta\theta}=r^2 , g_{\phi\phi}=r^2\sin^2\theta, others zero , so the only nonzero derivatives of the metric are

\partial_{r}g_{\theta\theta}=2r
\partial_{r}g_{\phi\phi}=2r\sin^2\theta
\partial_{\theta}g_{\phi\phi}=2r^2\sin\,\theta\,\cos\,\theta

Which means that -\Gamma^{\theta}_{rr}F^r-\Gamma^{\theta}_{r\theta}F^{\theta}-\Gamma^{\theta}_{r\phi}F^{\phi}=-\frac12g^{\theta\theta}\partial_rg_{\theta\theta}F^{\theta}=-\frac12 r^{-2}\cdot2r\cdot\frac{1}{\sin\,\theta}A=-\frac{A}{r\sin\,\theta}

so

\nabla_rF^{\theta}=\frac{1}{\sin\,\theta}\frac{\partial A}{\partial r}-\frac{A}{r\sin\,\theta}=\frac{\partial F^{\theta}}{\partial r}-\frac{1}{r}F^{\theta}
 
espen180 thanks for the reply. I'm reading a paper and the thing I'm trying to do is to understand how the gradient tensor of the before mentioned vector field is derived. That means that I have the solution for the gradient tensor but not the derivation...

I must say I'm still a bit confused. The vector field \vec{F} represents the magnetic field due to some currents in the atmosphere in spherical coordinates. Therefore I think you are right that it should be a contravariant vector. On the other hand, consulting the book "Mathematical Methods for Physicists" by Arfken the covariant derivative of a contravariant tensor is given by:
<br /> \nabla_qF^p=\partial_qF^p+\Gamma^p_{qk}F^k<br />​

So my first question is why do you have <br /> \nabla_qF^p=\partial_qF^p-\Gamma^p_{qk}F^k<br /> ?

Furthermore, If I calculate the element with p=2, q=1 as you nicely showed I get:

<br /> \nabla_rF^{\theta}=\frac{1}{\sin\,\theta}\frac{\partial A}{\partial r}+\frac{A}{r\sin\,\theta}=\frac{\partial F^{\theta}}{\partial r}+\frac{1}{r}F^{\theta}<br />​

But, checking with the already calculated gradient tensor in that paper, for this element I have:
<br /> \frac{1}{\sin\theta}\frac{\partial A}{\partial r} = \frac{\partial F^\theta}{\partial r}<br />​

So I don't get why I have this extra term \frac{1}{r}F^{\theta} or -\frac{1}{r}F^{\theta} in your case.

Note that in that paper in order to calculate the gradient tensor he uses the formula:

<br /> \nabla_qF^p=\nabla x^q(\frac{\partial F_q}{\partial x^p}-\Gamma^k_{pq}F_k)\nabla x^p<br />​

in which I'm not sure whether I understand why we multiply with the basis \nabla x^q , \nabla x^p. Is it because we use the covariant vector instead of the contravariant vector ?.
 
stuxk said:
espen180 thanks for the reply. I'm reading a paper and the thing I'm trying to do is to understand how the gradient tensor of the before mentioned vector field is derived. That means that I have the solution for the gradient tensor but not the derivation...

I must say I'm still a bit confused. The vector field \vec{F} represents the magnetic field due to some currents in the atmosphere in spherical coordinates. Therefore I think you are right that it should be a contravariant vector. On the other hand, consulting the book "Mathematical Methods for Physicists" by Arfken the covariant derivative of a contravariant tensor is given by:
<br /> \nabla_qF^p=\partial_qF^p+\Gamma^p_{qk}F^k<br />​

So my first question is why do you have <br /> \nabla_qF^p=\partial_qF^p-\Gamma^p_{qk}F^k<br /> ?

Haha. It turns out that I started with the wrong formula but made a sign error, so the ruesult is still valid. :-p

The term -\frac{1}{r}F^{\theta} comes from this mess:

-\Gamma^{\theta}_{rr}F^r-\Gamma^{\theta}_{r\theta}F^{\theta}-\Gamma^{\theta_{r\phi}F^{\phi} which is actually the sum -\Gamma^{\theta}_{rk}F^k written out using the Einstein summation convention. Anyway, there is a lone nonzero term in there, inside the middle Christoffel symbol:

\frac12g^{\thetax}\left( \partial_r g_{\theta x} + \partial_{\theta}g_{rx} - \partial_xg_{r\theta}\right)

which a whole 'nouther sum itself. :rolleyes:

In my previous post I listed all the nonzero derivatives of the metric for spherical coordinates. Just by looking at the this expression you can see the the only nonzero term will reveal itself when x=θ (the inverse metric multiplying the whole thing, plus that only metric elements on the diagonal have nonzero derivatives are two things which can lead to this conclusion), so plug in x=θ. Now, the only nonzero term inside the parenthesis will be the left one, so we are left with

-\Gamma^{\theta}_{rk}F^k=-\frac12g^{\theta\theta}\partial_rg_{\theta\theta}F^{\theta}=-\frac{A}{r\sin\,\theta}=-\frac{1}{r}F^{\theta}


Regarding the other covariant derivative formula you posted, I have never seen it before. The one I used is the one found in Shaum's Outline Series: Vector Analysis & Introduction to Tensor Analysis.
 

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