Separation of variables in spherical coordinates (electrostatics)

In summary, the problem was to find the c_i's for the equation ##V \left(r, \theta \right) = \sum_{\ell = 0}^{\infty} \left( A_\ell r^\ell + \frac{B_\ell}{r^{\ell + 1}}\right) P_\ell \left( \cos \theta\right)##. The person solved it by expanding the righthand side and equating coefficients.
  • #1
milkism
118
15
Homework Statement
Need help with setting up the first part of the problem.
Relevant Equations
See solution.
Problem:
fa5007c579a379e3e58e9fb1f28e4fd4.png


Solution:
When I looked at an example problem, they started writing the potential in terms of the Legendre polynomials.
The example problem:
8d13019377fe67349760b37632205e52.png

This is what I did:
$$V_0 \alpha P_2 (\cos(\theta)) \Rightarrow \frac{\alpha 3 \cos ^2 (\theta)}{2} - \frac{\alpha}{2} \Rightarrow \frac{\alpha 3}{2} - \frac{\alpha}{2}= 1 \Rightarrow \alpha = 1$$
Hence,
$$V(\theta) = V_0 P_2 (\cos(\theta)).$$
Have I done right?
 
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  • #2
milkism said:
Homework Statement: Need help with setting up the first part of the problem.
Relevant Equations: See solution.

Problem:
View attachment 325294

Solution:
When I looked at an example problem, they started writing the potential in terms of the Legendre polynomials.
The example problem:
View attachment 325295
This is what I did:
$$V_0 \alpha P_2 (\cos(\theta)) \Rightarrow \frac{\alpha 3 \cos ^2 (\theta)}{2} - \frac{\alpha}{2} \Rightarrow \frac{\alpha 3}{2} - \frac{\alpha}{2}= 1 \Rightarrow \alpha = 1$$
Hence,
$$V(\theta) = V_0 P_2 (\cos(\theta)).$$
Have I done right?
Also with radial dependance do they just mean calculate A_l and B_l?
 
  • #3
Yes you are supposed to find ##A_\ell## and ##B_\ell## and plug them into the generic formula

##V \left(r, \theta \right) = \sum_{\ell = 0}^{\infty} \left( A_\ell r^\ell + \frac{B_\ell}{r^{\ell + 1}}\right) P_\ell \left( \cos \theta\right)##

On physical grounds ##A_\ell = 0## outside and ##B_\ell = 0## inside because we cant have the potential blowing up at infinity or at the origin.
 
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  • #4
You may want to start with [tex]
\left.\begin{array}{r}
P_2(\cos \theta) = \frac{1}{2}(3 \cos^2 \theta - 1) \\
P_0(\cos \theta) = 1 \end{array}\right\} \quad \Rightarrow\quad
\cos^2 \theta = \frac23P_2(\cos \theta) + \frac13P_0(\cos \theta)[/tex]
 
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  • #5
milkism said:
Hence,
$$V(\theta) = V_0 P_2 (\cos(\theta)).$$
Have I done right?
No. Write out the righthand side as a polynomial in ##\cos\theta##, and you'll see it doesn't equal the given ##V(\theta)##.

In the example problem, you have the potential ##V = k \cos 3\theta= k(4\cos \theta^3-3\cos\theta)##, which is a third-order polynomial of ##\cos\theta##. That means it's an element of the vector space consisting of polynomials of degree 3 or fewer.

The first four Legendre polynomials are a basis for this vector space, so any element of the vector space can be expressed as a linear combination of the Legendre polynomials. In other words, you can say
$$4k\cos^3\theta - 3k\cos\theta = c_3 P_3(\cos\theta) + c_2 P_2(\cos\theta) + c_1 P_1(\cos\theta) + c_0 P_0(\cos\theta).$$ The problem is then finding the appropriate values for the ##c_i##'s.

A straightforward way to do that is to simply expand out the righthand side and then equating coefficients from the two sides of the equation. You'll get a system of four linear equations which is simple to solve. Griffiths used a useful shortcut to deduce ##c_0 = c_2 = 0##, so he ended up with a system of two equations and two unknowns.

In your problem, you have ##V=V_0 \cos^2\theta##. It's an element of the vector space consisting of polynomials of degree 2 or fewer, and the first three Legendre polynomials will span that space. So the problem is to find ##c_0##, ##c_1##, and ##c_2## so that
$$V_0 \cos^2\theta = c_2 P_2(\cos\theta) + c_1 P_1(\cos\theta) + c_0 P_0(\cos\theta).$$ Expand the righthand side and then equate coefficients to get the equations you need to solve.
 
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  • #6
Thanks you all, first time doing such problem and I completely understand it now!
 
  • #7
Also for finding the electrostatic dipole moment of the system can we just use the surface charge density on the surface to calculate it?
 
  • #8
milkism said:
Also for finding the electrostatic dipole moment of the system can we just use the surface charge density on the surface to calculate it?
I get zero for electrostatic dipole moment of the system, don't know if it's right.
Using this formula:
4c59089647f90ec8a9d86b847cfad38e.png

I get $$\frac{V_0 \epsilon_0}{R} \left( 5\cos ^2 (\theta) - \frac{4}{3} \right)$$.
Then for electrostatic dipole moment in spherical coordinates:
e935e3747ab3f491d60fc6d7b62c88c0.png

Computing the integral I get zero.
 
  • #9
Having solved this very problem myself, for the outside I do not get a 1/r^2 term for the potential. So I’d have to agree with you about your dipole moment.
 
  • #10
PhDeezNutz said:
Having solved this very problem myself, for the outside I do not get a 1/r^2 term for the potential. So I’d have to agree with you about your dipole moment.
Is it even possible for there to not be a dipole moment?
 
  • #11
Absolutely. The next higher up moment is the quadrupole which in the simplest illustration is two back to back opposing dipoles and therefore the dipole moments cancel out.

The Quadrupole is a 2nd rank (symmetric) tensor and is not so easy to visualize. This moment is scarcely dealt with in Griffiths however there is an exercise pertaining to it.
 
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  • #12
PhDeezNutz said:
Absolutely. The next higher up moment is the quadrupole which in the simplest illustration is two back to back opposing dipoles and therefore the dipole moments cancel out.

The Quadrupole is a 2nd rank (symmetric) tensor and is not so easy to visualize. This moment is scarcely dealt with in Griffiths however there is an exercise pertaining to it.
My next problem is to calculate the mono-di and quadrapole of 4 charges haha, luckily no octopole problem.
 
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  • #13
PhDeezNutz said:
Absolutely. The next higher up moment is the quadrupole which in the simplest illustration is two back to back opposing dipoles and therefore the dipole moments cancel out.

The Quadrupole is a 2nd rank (symmetric) tensor and is not so easy to visualize. This moment is scarcely dealt with in Griffiths however there is an exercise pertaining to it.
I think the dipole moment is zero because the angular dependant potential is symmetric (even), just like how symmetric molecules have no dipole moment 😅😅
 
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  • #14
That makes sense to me.

When you calculate the dipole moment of the 4 charges I bet it’s going to be zero.

Edit: your instructor knows how to choose good problems. It’s nice how one leads into the other with emphasis. I’m a fan.
 
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Related to Separation of variables in spherical coordinates (electrostatics)

What is the separation of variables method in spherical coordinates?

The separation of variables method in spherical coordinates is a mathematical technique used to solve partial differential equations, such as Laplace's equation, by expressing the solution as a product of functions, each depending on a single coordinate. In spherical coordinates, these coordinates are the radial distance (r), polar angle (θ), and azimuthal angle (φ).

How is Laplace's equation written in spherical coordinates?

Laplace's equation in spherical coordinates is written as:\[ \frac{1}{r^2} \frac{\partial}{\partial r} \left( r^2 \frac{\partial \Phi}{\partial r} \right) + \frac{1}{r^2 \sin \theta} \frac{\partial}{\partial \theta} \left( \sin \theta \frac{\partial \Phi}{\partial \theta} \right) + \frac{1}{r^2 \sin^2 \theta} \frac{\partial^2 \Phi}{\partial \phi} = 0 \]where \( \Phi \) is the potential function.

What are the boundary conditions commonly used in electrostatics problems involving spherical coordinates?

Common boundary conditions in electrostatics problems involving spherical coordinates include specifying the potential \( \Phi \) on the surface of a sphere (Dirichlet boundary condition), specifying the electric field (or derivative of \( \Phi \)) on the surface (Neumann boundary condition), or a combination of both. These conditions are essential for determining the specific form of the solution.

How are the solutions to Laplace's equation typically expressed in spherical coordinates?

The solutions to Laplace's equation in spherical coordinates are typically expressed as a series of spherical harmonics. The general solution can be written as:\[ \Phi(r, \theta, \phi) = \sum_{l=0}^{\infty} \sum_{m=-l}^{l} \left( A_{lm} r^l + \frac{B_{lm}}{r^{l+1}} \right) Y_{lm}(\theta, \phi) \]where \( Y_{lm}(\theta, \phi) \) are the spherical harmonics, and \( A_{lm} \) and \( B_{lm} \) are constants determined by boundary conditions.

Why is the separation of variables method useful in solving electrostatics problems?

The separation of variables method is useful in solving electrostatics problems because it simplifies complex partial differential equations into simpler, ordinary differential equations. This method leverages the symmetry of the problem, making it easier to find analytical solutions, especially in cases with spherical symmetry such as the potential around a spherical

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