Confusion with Dot Product in Polar Coordinates with the Metric Tensor

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SUMMARY

The discussion centers on the application of the metric tensor in polar coordinates for calculating the dot product of two vectors. The metric tensor is defined as g_{ab}=\begin{pmatrix}1&0\\0&r^2\end{pmatrix}, leading to the dot product expression A^1B^1+(r)^2A^2B^2. The confusion arises regarding which value of r to use, as both vectors A and B depend on r. It is clarified that the metric tensor is valid for computing the dot product of vectors at a specific point in space, with the understanding that the vectors must originate from the same point in the polar coordinate system.

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MrBillyShears
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Alright, so I was reading up on tensors and such with non-Cartesian coordinate systems all day but now I'm a bit tired an confused so you'll have to forgive me if it's a stupid question. So to express the dot product in some coordinate system, it's:
g(\vec{A}\,,\vec{B})=A^aB^bg_{ab}
And, if we're dealing with polar coordinates, then the metric is:
g_{ab}=\begin{pmatrix}1&0\\0&r^2\end{pmatrix}
Alright, so the dot product is:
A^1B^1+(r)^2A^2B^2
But which r? I know I'm probably only confused because I'm so tired right now, but both A and B have r's, do't they? Which r is used to compute this?
Remember, I'm just a student at this, so don't get too technical in the response, and sorry for any typos.
Thanks!
 
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In my experience, both, r, theta are given as functions.
 
I'm trying to figure this out on my own. Perhaps no one understands what I'm asking. I'm asking if the metric tensor I listed above is valid to use in the dot product of two different vectors. Because the basis vectors are different at different points,
\vec{e}_{a'}=\Lambda^b{}_{a'}\vec{e}_{b}
where
\Lambda^b{}_{a'}=\begin{pmatrix}cos{Θ}&sin{Θ}\\-rsin{Θ}&rcos{Θ}\end{pmatrix}
So, if there are different basis vectors for different points, you can't use the same metric tensor as you would to say, transform a polar vector to a polar covector. Is this correct?
 
The metric ##g## is a tensor field of type (2,0), so it associates a tensor ##g_{\vec r}## of type (2,0) with each ##\vec r\in\mathbb R^2##. This ##g_{\vec r}## is an inner product on ##T_{\vec r}\mathbb R^2##, the tangent space of ##\mathbb R^2## at ##\vec r##. You have determined the components (in the polar coordinate system) of ##g_{\vec r}## for an arbitrary ##\vec r##. Your r is the absolute value of this ##\vec r##.

If you want a mental image, imagine a second copy of ##\mathbb R^2## with its (0,0) point attached to the point ##\vec r##. The A and B that you feed into ##g_{\vec r}## are vectors in that space, so if you visualize them as arrows, those arrows should start at ##\vec r##.
 
Last edited:
Ok, thanks. It's becoming much clearer to me now.
 
You can calculate the metric like this g_{ij} = (\partial_{i}, \partial_{j}) for your parametrization i.e. for cylindrical coordinates. Then if you want to convert a vector in this coordinate system from a contravariant form into a covariant form you have to contract it with this metric tensor like A_{i}=g_{ij}A^{j}, the solution to this system of equations is your covariant vector in cylindrical coordinates. I'm not sure this helps...
 

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