Derivation of Laplace in spherical co-ordinates

In summary, you can derive the Laplace equation in spherical coordinates by identifying it with the Laplacian.
  • #1
darwined
18
0
I have been trying to derive the Laplace in spherical co ordinates.
I have attached a file which has basic equations.
I am trying to get the following equation.

d(phi)/dx= -sin(phi)/(r sin (theta)).

I have also attached the materials I am referring to.
Can someone please help me derive the equation.

Thank you.
 

Attachments

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  • #2
This is a pretty cumbersome way. The most easy is to use the action principle. The action
[tex]A[\phi]=\int \mathrm{d}^3 \vec{x} [(\vec{\nabla} \phi)^2+f \phi][/tex]
leads to the equation
[tex]\Delta \phi=f.[/tex]
Now you write the gradient in terms of spherical coordinates (which is easy to derive by your direct method)
[tex]\vec{\nabla} \phi=\vec{e}_r \partial_r \phi+\frac{1}{r} \vec{e}_{\theta} \partial_{\theta} \phi + \frac{1}{r \sin \theta} \vec{e}_{\varphi} \partial_{\varphi} \phi.[/tex]
The volume element is
[tex]\mathrm{d}^3 {\vec{r}}=\mathrm{d} r \mathrm{d} \theta \mathrm{d} \varphi r^2 \sin \theta.[/tex]
This you plug into the action integral and use the Euler-Lagrange equations to derive the field equation in terms of spherical coordinates. This leads to the Laplacian by identifying it with [itex]f[/tex].
 
  • #3
darwined said:
I have been trying to derive the Laplace in spherical co ordinates.
I have attached a file which has basic equations.
I am trying to get the following equation.

d(phi)/dx= -sin(phi)/(r sin (theta)).

I have also attached the materials I am referring to.
Can someone please help me derive the equation.

Thank you.
Show us your attempt at deriving that equation.
 
  • #4
I second Vela. Vanhees is focusing on ##\Delta##. If you want a hint for your ## {d\phi \over dx} ## question: ##\tan \phi = {y \over x} ## is a good starting point.
 
  • #5
Thank you for your reply vanhees71. But I am not sure how you even got the equation.

A[ϕ]=∫d3x→[(∇→ϕ)2+fϕ]

I am a beginner trying to learn this derivation.

Thank you BvU, your idea helped.

Thank you all.
 
  • #6
Your attached references are just a straightforward transformation of coordinates that you learn how to do in a course on partial differential equations. Have you had a course that covers partial differential equations yet?

Chet
 

FAQ: Derivation of Laplace in spherical co-ordinates

What are spherical coordinates?

Spherical coordinates are a coordinate system used to describe the position of a point in three-dimensional space. It uses two angles, usually denoted as theta (θ) and phi (φ), along with a distance or radius (r) from the origin to specify a point.

Why is Laplace's equation important in spherical coordinates?

Laplace's equation is a fundamental equation in mathematics and physics that describes the behavior of many physical systems, including those in spherical coordinates. It is used to solve problems involving electric and gravitational potentials, heat flow, and fluid dynamics, among others.

What is the derivation of Laplace's equation in spherical coordinates?

The derivation of Laplace's equation in spherical coordinates involves using the divergence theorem and the spherical coordinate expression for the gradient operator. This results in the familiar form of the equation, ∇²f = 0, where f is a function of the spherical coordinates r, θ, and φ.

How is Laplace's equation solved in spherical coordinates?

There are several methods for solving Laplace's equation in spherical coordinates, including separation of variables, the method of images, and the method of integral transforms. Each method has its own advantages and is suited for different types of problems.

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

Laplace's equation in spherical coordinates has many practical applications in science and engineering, such as in the study of electromagnetic fields, fluid flow, heat transfer, and quantum mechanics. It is also used in geophysics to model the gravitational potential of the Earth and other celestial bodies.

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