Laplace's equation in spherical co-ords

In summary, the general solution to Laplace's equation in spherical coordinates is given by u(r, \theta, \phi) = \sum^{\infty}_{l=0}\sum^{l}_{m=-l}\left(a_{lm}r^{l} + \frac{b_{lm}}{r^{l+1}}\right)P_{lm}(cos\theta)e^{im\phi}, where the coefficients a_{lm} and b_{lm} can be determined using boundary conditions. There may be confusion about the limits on the summation, which can be resolved by considering the irreducible representation of SO(3) with dimension 2\ell + 1.
  • #1
benabean
31
0
I have a simple question about the general solution to Laplace's equation in spherical co-ords.
The general solution is:

[tex]u(r, \theta, \phi) = \sum^{\infty}_{l=0}\sum^{l}_{m=-l}\left(a_{lm}r^{l} + \frac{b_{lm}}{r^{l+1}}\right)P_{lm}(cos\theta)e^{im\phi}[/tex]

(where the [tex]a_{lm}, b_{lm}[/tex] coefficients can be found using the boundary conditions in question.)

My problem lies in trying to understand the limits on the summation [tex]\sum^{l}_{m=-l}[/tex]. Can anyone offer any help on this please?

Thanks for reading, b.
 
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  • #2
Probably due to the same reason why the irreducible representation of SO(3) has dimension
[tex]2\ell + 1[/tex] (physicist tends to use j for spin/orbital angular momentum number).
 

Related to Laplace's equation in spherical co-ords

1. What is Laplace's equation in spherical coordinates?

Laplace's equation in spherical coordinates is a partial differential equation that describes the relationship between the potential function and its derivatives in a three-dimensional spherical coordinate system. It is often used in physics and engineering to model the behavior of scalar fields, such as temperature or electric potential.

2. What are spherical coordinates?

Spherical coordinates are a type of coordinate system used to describe points in three-dimensional space. They consist of a radial distance from the origin, an angle measured from the positive z-axis, and an angle measured from the positive x-axis in the xy-plane. This system is useful for describing spherical objects or systems with spherical symmetry.

3. What is the Laplacian operator?

The Laplacian operator is a differential operator that is used to calculate the divergence of a vector field or the curvature of a scalar field. In spherical coordinates, it takes the form of 1/r^2 * ∂/∂r (r^2 ∂/∂r) + 1/r^2 sinθ ∂/∂θ (sinθ ∂/∂θ) + 1/r^2 sin^2θ ∂^2/∂φ^2.

4. How is Laplace's equation solved in spherical coordinates?

Laplace's equation in spherical coordinates can be solved using separation of variables. This involves assuming a solution of the form V(r, θ, φ) = R(r)Θ(θ)Φ(φ) and then substituting this into the equation to obtain three separate ordinary differential equations. These equations can then be solved individually to find the general solution to Laplace's equation.

5. What are some applications of Laplace's equation in spherical coordinates?

Laplace's equation in spherical coordinates has many applications in physics and engineering. It can be used to model the electric potential in a spherical region, the temperature distribution in a spherical object, or the gravitational potential of a spherical mass distribution. It is also used in fluid mechanics to describe the motion of a fluid in a spherical container or with spherical symmetry.

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