Multipole Expansion for Two Charged Hemispheres

In summary, the study of multipole expansion for two charged hemispheres examines the electric potential and field generated by two hemispherical charged surfaces. The method involves expressing the potential as a series of multipole moments, which simplifies the analysis of the system's interactions at various distances. The work highlights the contributions of monopole, dipole, and higher-order multipole terms, providing insights into the charge distribution and its effects on the surrounding space. This approach aids in understanding complex electrostatic configurations and can be applied to various physical situations involving charged geometries.
  • #1
the_fater
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Homework Statement
Consider two homogeneously charged solid hemispheres with radius R separated in the x-y-plane by a negligible slit. The upper hemisphere has a total charge of +Q, and the lower hemisphere has a total charge of −Q.
1. Write down an expression for the volume charge density ρ of the two hemispheres.
2. Calculate the spherical and the Cartesian dipole moment.
Relevant Equations
electric dipole moment ##\vec P = \int \rho(\vec r^{'}) r^{'} \, dv^{'}##
My thought: First of all, I find the upper hemisphere (with a total charge +Q): ##ρ(\vec r)=\frac {V} {Q}## where V is the volume of the upper hemisphere = ## \frac {2} {3} \pi R^3##. Secondly, find the lower hemisphere (with a total charge −Q): ##ρ(\vec r)=\frac {V} {Q}## where V is the volume of the lower hemisphere = ## \frac {2} {3} \pi R^3##. I suggest that these expressions represent the volume charge densities for the upper and lower hemispheres. However, I am not entirely sure about it, so I am uncertain if I can find the correct dipole moments in Cartesian and spherical coordinates. Thanks for any help!
 
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  • #2
Isn’t density Q/V and not V/Q?

Where as you said V is volume.
 
  • #3
PhDeezNutz said:
Isn’t density Q/V and not V/Q?

Where as you said V is volume.
Thank you for noticing. It's Q/V, sorry for the typo.
 
  • #4
I'm considering the calculation of the volume charge density ##\rho## for the two hemispheres. It can be obtained by dividing the total charge of each hemisphere by its volume. The volume of a hemisphere is given by ##\frac {2}{3} \pi R^3##. Therefore, the volume charge density for the upper hemisphere is ##\rho = \frac {3Q}{2 \pi R^3} ##, and for the lower hemisphere, it is ##\rho = \frac {-3Q}{2 \pi R^3} ##.
Now, considering the dipole moment, which is the product of the charge and the distance between the charges. In spherical coordinates, the dipole moment is zero because the charges are symmetrically distributed about the origin. Similarly, in Cartesian coordinates, the dipole moment is also zero due to the symmetric distribution of charges about the origin.
Please correct me if I have misunderstood or made mistakes anywhere. Thank you!
 
  • #5
I am most definitely not getting a dipole moment of 0. Intuitively it should be anything BUT 0. You have 2 opposite charges separated by negligible distance........this is practically the definition of a dipole.

I'll give you a hint

##d_{volume} = r^2 \sin \theta \, dr \, d\theta \, d \phi##

for a sphere

for both of the top and the bottom ##r## goes from ##0## to ##R##

for both and the and the bottom ##\phi## goes from ##0## to ##2 \pi##

Here's two questions:

For the top what is the range of ##\theta##?

For the bottom what is the range of ##\theta##?
 
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  • #6
the_fater said:
However, I am not entirely sure about it, so I am uncertain if I can find the correct dipole moments in Cartesian and spherical coordinates.
Your equation ##\vec P = \int \rho(\vec r^{'}) r^{'} \, dv^{'}## is inconsistent and will not take you very far. You show a vector on the LHS and a scalar on the RHS. Since the charge density is uniform in each hemisphere, you might as well write ##\rho(\vec r')=\pm \rho=\text{const.}## Then the correct expression would be (I prefer to use bold characters for vectors) $$\mathbf{P} = \int \rho~\mathbf{r}' \, dv^{'}.$$That's 3 equations in 1:$$\begin{align}
& P_x = \int \rho~x'\, dv^{'} \nonumber \\
& P_y = \int \rho~y'\, dv^{'} \nonumber \\
& P_z = \int \rho~z'\, dv^{'} \nonumber \\
\end{align}$$Once you have the Cartesian components, it should be easy to write this in spherical coordinates using the standard unit vector transformations from one to the other.

This is in addition to what @PhDeezNutz said with which I concur.
 
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  • #7
kuruman said:
$$\mathbf{P} = \int \rho~\mathbf{r}' \, dv^{'}.$$
I guess that can be arrived at by notionally pairing each small region with its diametrically opposite equivalent. From the symmetry, we could instead pair it with its reflection in the XY plane.
 
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  • #8
PhDeezNutz said:
I am most definitely not getting a dipole moment of 0. Intuitively it should be anything BUT 0. You have 2 opposite charges separated by negligible distance........this is practically the definition of a dipole.

I'll give you a hint

##d_{volume} = r^2 \sin \theta \, dr \, d\theta \, d \phi##

for a sphere

for both of the top and the bottom ##r## goes from ##0## to ##R##

for both and the and the bottom ##\phi## goes from ##0## to ##2 \pi##

Here's two questions:

For the top what is the range of ##\theta##?

For the bottom what is the range of ##\theta##?
Thanks for the hint! Here's my idea below. I hope I'm on the right track!
Spherical Dipole Moment = ##\int \rho(\vec r) \vec r \, dV##. For the upper hemisphere = ##\int_{0}^{\pi/2} \int_{0}^{2\pi} \int_{0}^{R} \frac {3Q} {2 \pi R^3} \vec r r^2 \sin(\theta) \, dr \, d\phi \, d\theta ##. For the lower hemisphere = ##\int_{\pi/2}^{\pi} \int_{0}^{2\pi} \int_{0}^{R} \frac {-3Q} {2 \pi R^3} \vec r r^2 \sin(\theta) \, dr \, d\phi \, d\theta ##. In Cartesian coordinates, the dipole moment for the upper hemisphere = ##\int_0^R \int_0^R \int_0^R \frac {3Q} {2 \pi R^3} \vec r \, dx \, dy \, dz ##. The dipole moment for the lower hemisphere = ##\int_{-R}^{0} \int_0^R \int_0^R \frac {-3Q} {2 \pi R^3} \vec r \, dx \, dy \, dz ##.
 
  • #9
I have no idea what a spherical dipole moment is. To me a dipole moment is a dipole moment regardless of what basis it is expressed in.

Read the post quoted below more carefully.

Also you seem to think that to find the dipole moment in Cartesian you must integrate in Cartesian…….that is not correct and I would highly advise against it. Integrate in spherical coordinates when dealing with a sphere.
kuruman said:
$$\mathbf{P} = \int \rho~\mathbf{r}' \, dv^{'}.$$That's 3 equations in 1:$$\begin{align}
& P_x = \int \rho~x'\, dv^{'} \nonumber \\
& P_y = \int \rho~y'\, dv^{'} \nonumber \\
& P_z = \int \rho~z'\, dv^{'} \nonumber \\
\end{align}$$Once you have the Cartesian components, it should be easy to write this in spherical coordinates using the standard unit vector transformations from one to the other.

This is in addition to what @PhDeezNutz said with which I concur.

@the_fater what is x in spherical coordinates?

What is y in spherical coordinates?

What is z in spherical coordinates?
 
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  • #10
haruspex said:
I guess that can be arrived at by notionally pairing each small region with its diametrically opposite equivalent. From the symmetry, we could instead pair it with its reflection in the XY plane.
I always thought that it is the definition of the dipole term in general. It does not have to be a "pure" dipole that has the symmetry you mentioned. In a multipole expansion, point charge ##q## at position vector ##\mathbf{a}## from the origin has a monopole potential due to charge ##q## at the origin plus a dipole term due to a dipole moment ##\mathbf{p}=q~\mathbf{a}## at the origin plus higher order terms.
 

FAQ: Multipole Expansion for Two Charged Hemispheres

What is the purpose of using multipole expansion for two charged hemispheres?

The purpose of using multipole expansion for two charged hemispheres is to simplify the calculation of the electrostatic potential at points far away from the hemispheres. By representing the potential as a series of terms with decreasing magnitude, it becomes easier to analyze and approximate the behavior of the system without solving the full problem directly.

How do you derive the multipole expansion for two charged hemispheres?

To derive the multipole expansion for two charged hemispheres, you start by expressing the electrostatic potential due to each hemisphere using spherical harmonics. Then, you combine these potentials and expand them in terms of multipole moments. This involves calculating the monopole, dipole, quadrupole, and higher-order terms, which describe the distribution of charge in increasingly fine detail.

What are the key multipole moments for two charged hemispheres?

The key multipole moments for two charged hemispheres include the monopole moment (total charge), the dipole moment (related to the separation and orientation of the hemispheres), and the quadrupole moment (related to the shape and charge distribution). Higher-order moments, such as the octupole and hexadecapole, may also be relevant depending on the precision required for the analysis.

How does the separation between the hemispheres affect the multipole expansion?

The separation between the hemispheres significantly affects the multipole expansion, particularly the dipole and higher-order moments. As the separation increases, the dipole moment becomes more pronounced, and higher-order terms may become more significant. The exact influence depends on the relative positioning and the specific charge distribution of the hemispheres.

In what scenarios is the multipole expansion for two charged hemispheres particularly useful?

The multipole expansion for two charged hemispheres is particularly useful in scenarios where the distance from the hemispheres to the point of interest is much larger than the size of the hemispheres. This includes applications in fields such as electrostatics, antenna theory, and molecular physics, where understanding the far-field behavior of charge distributions is important.

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