How to write the unit vector for the spherical coordinates

In summary, the conversation discusses the application of Coulomb's Law in finding the electric field due to a uniformly charged disk and a sphere. The formula for finding the electric field is given, followed by a discussion on how to calculate the unit vector and the distance from the surface of the disk or sphere to the point of observation. The conversation also includes a question about the angular component in the equation, which is determined by the orientation of the disk or sphere. Finally, the conversation touches on the construction of the vector and the geometry involved in finding the correct result in the denominator.
  • #1
unicornflyers
8
0
So I'm reading the Schaum's outlines while trying to prepare for a big test I have in September. And I'm trying to understand something here that maybe someone can offer some clarification and guidance.

So, using Coulomb's Law, we can find the electric field as follows:

\begin{equation}
dE = k\frac{dQ}{d^{2}} a_{R}
\end{equation}

I'm letting k be the constant since I don't want to have to constantly type of the 4*pi*epsilon_{0}

To help figure this out (and get to my question), let's consider a simple example in cylindrical coordinates due to a uniformly charged disk. And let's find the electric field at some point z above the axis.

We can write the unit vector as:

\begin{equation}
a_{R} = \frac{R}{|R|}
\end{equation}

For the uniformly charged disk, R is the distance from the surface of the disk. In cylindrical coordinates, we can write this as:

\begin{equation}
R = -r a_{r} + z a_{z}
\end{equation}
thus
\begin{equation}
R^{2} = r^{2} + z^{2}
\end{equation}

oh, and we know $dQ = \rho dV = \rho r dr d\phi dz$ in cylindrical coordiantes

We can plug all of this into the equation. (First question is can someone explain to me why the angular component is zero in the R equation (i.e. notice we have a_r, a_z, but no a_phi, and or how we'd put this in here?)

In any event, we get:

\begin{equation}
dE = k\frac{dQ}{d^{2}} a_{R} = k\frac{\rho r dr d\phi dz}{(r^{2}+z^{2}} \frac{-r a_{r} + z a_{z}}{(r^{2} + z^{2})^{1/2}}
\end{equation}

From here, it's just math and I get that part.

Here's where my question comes in. If I want to follow this same prescription for a sphere instead, I get confused.

So with a sphere, we have some element on the surface. In doing so, we have a height z from the origin to the point above the sphere. We have a radius r from the origin out to the small element we choose. and we have R which is from the element to the point at the sphere.

Trying to follow the prescription I did above, I get lost.

So using the law of cosines, I can find the d^2 as:

\begin{equation}
d^{2} = r^{2} +z^{2} - 2rzcos\theta
\end{equation}

but here is where I run into issues:

when trying to construct a_{R}:

we can construct the vector similarly as:

\begin{equation}
A_{R} = A_{r} \hat{r} + A_{\theta} \hat{theta} +A_{\phi} \hat{\phi}
\end{equation}

And this is where I don't know how to proceed. We can say that $A_{r} = r \rhat$, but what do we say for the other components? And how would we go about plugging them into get the correct result in the denominator, as we did for the ring's case? It seems to me that this should work so long as we have the geometry right.
 
Physics news on Phys.org
  • #2
unicornflyers said:
R is the distance from the surface of the disk
You should have phrased the above statement more precisely. I believe it would better describe the situation if you had said instead "R is the distance from a point on the surface of the disk to the point of observation."
unicornflyers said:
First question is can someone explain to me why the angular component is zero in the R equation
If the axis of the disk is aligned along the z axis, then it's because the point of observation lies in the z axis. Try projecting this vector ##\mathbf R## onto the plane of the disk, you should see that the projection goes straight toward the disk center, which means that the projection vector only has radial component.
 

Related to How to write the unit vector for the spherical coordinates

1. What are spherical coordinates?

Spherical coordinates are a coordinate system used to locate points in three-dimensional space. They are defined by three parameters: radius (r), inclination angle (θ), and azimuth angle (φ).

2. How do you write the unit vector for spherical coordinates?

The unit vector for spherical coordinates is written as ur for the radial direction, uθ for the inclination direction, and uφ for the azimuth direction.

3. What is the unit vector for the radial direction in spherical coordinates?

The unit vector for the radial direction in spherical coordinates is ur = (cosθcosφ, cosθsinφ, sinθ). It points in the direction from the origin to the point in question.

4. How do you find the unit vector for the inclination direction in spherical coordinates?

The unit vector for the inclination direction in spherical coordinates is uθ = (-sinθcosφ, -sinθsinφ, cosθ). It points in the direction of increasing inclination angle.

5. How do you determine the unit vector for the azimuth direction in spherical coordinates?

The unit vector for the azimuth direction in spherical coordinates is uφ = (-sinφ, cosφ, 0). It points in the direction of increasing azimuth angle and is perpendicular to both the radial and inclination directions.

Similar threads

  • Advanced Physics Homework Help
Replies
1
Views
811
  • Introductory Physics Homework Help
Replies
2
Views
397
  • Calculus and Beyond Homework Help
Replies
5
Views
975
  • Electromagnetism
Replies
4
Views
829
Replies
1
Views
2K
  • Advanced Physics Homework Help
Replies
9
Views
2K
  • Other Physics Topics
Replies
1
Views
670
Replies
24
Views
4K
  • Advanced Physics Homework Help
Replies
3
Views
438
  • Calculus and Beyond Homework Help
Replies
3
Views
585
Back
Top