Computing Potential of a Spherical Shell w/o using Newton's theorems

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Homework Help Overview

The discussion revolves around computing the gravitational potential due to a spherical shell without using Newton's theorems. Participants explore the challenges of deriving an analytic expression for the potential, particularly focusing on the implications of spherical symmetry and the appropriate coordinate transformations.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the difficulty of transforming the potential equation into spherical coordinates due to vector subtraction. Some suggest integrating in polar coordinates to simplify the integration process. Others question the nature of the spherical distribution, whether it is solid or a shell, and the implications of using Gauss's theorem versus direct computation.

Discussion Status

The conversation includes various attempts to clarify the problem and explore different methods of integration. Some participants have offered insights into using trigonometry and geometry to simplify the integration process, while others express interest in the original poster's resolution of the problem.

Contextual Notes

There is an emphasis on not using simplifications such as Gauss's theorem, as the goal is to compute the potential directly from the fundamental equation. The original poster's intent to avoid certain methods is noted, as well as the potential confusion regarding the type of spherical distribution being analyzed.

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Homework Statement


I'm well aware of how to compute the gravitational [electric] potential [tex]\Phi[/tex] due to a spherical mass [charge] distribution of radius [tex]R[/tex] by using Newton's theorems for spherical shells. However, how does one find an analytic expression for [tex]\Phi[/tex] without invoking these theorems?

Homework Equations


[tex]\rho(r, \theta, \phi) = \rho(r) = M \delta(r - R)[/tex]
or equivalently:
[tex]\rho(\vec{x}) = M \delta(x_1^2 + x_2^2 + x_3^2 - R^2)[/tex]

[tex]\Phi(\vec{x}) = -\int_{\tau} \frac{G \rho(\vec{x}')}{|\vec{x}' - \vec{x}|} \; d^3x'[/tex]

The Attempt at a Solution



Now I can't simply transform the equation for potential into spherical coordinates because vector subtraction is involved. Furthermore, taking the line integral of gravitational force does not make things easier, since [tex]\vec{F} = \int_{\tau} \frac{G \rho(\vec{x}')(\vec{x}' - \vec{x})}{|\vec{x}' - \vec{x}|^3} \; d^3x'[/tex].

Any help is welcome.
 
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why not integrate in polar coordinates? I'm sure you could get rid of [tex]\int d \theta[/tex] and [tex]\int d \phi[/tex] then.
 
v0id said:

Homework Statement


I'm well aware of how to compute the gravitational [electric] potential [tex]\Phi[/tex] due to a spherical mass [charge] distribution of radius [tex]R[/tex].
It is not clear ffrom your question whether the sphere is solid or just one shell.
If the charge distribution is spherically symmetric (as you seem to imply), you can use Gauss's theorem, which poor Newton didn't kinow.
 
Meir Achuz said:
It is not clear ffrom your question whether the sphere is solid or just one shell.
If the charge distribution is spherically symmetric (as you seem to imply), you can use Gauss's theorem, which poor Newton didn't kinow.

My apologies. I had originally meant a spherical shell, from which the potential of an arbitrary spherically symmetric distribution can be computed. Gauss's theorem is certainly very useful, but the objective here is to compute the potential using the equation for [tex]\Phi[/tex] only, without applying any such simplifications.


@ whatta: Converting to spherical/polar coordinates is the most efficient method, but how does one do so with factors of [tex]\vec{x}' - \vec{x}[/tex]?
 
If you want to compute the potential as seen at a given point, you can just use basic trigonometry to calculate the distance (vector magnitude) from that point to each infinitesimal volume of the sphere then integrate the corresponding expression for the potential over the shell.

I remember that at school (something like 35 years ago) I was given this problem for a solid sphere as an integration exercise, but I noticed that if I integrated in some way over a thin segment (like a segment of an orange) where the axis of the segment pointed to the location where the potential was being measured, using some geometry with right angles and so on, so many things canceled that I didn't have to actually do any integration. However, as far as I remember, it was probably easier to use a less ingenious model and do the integration.
 
Thanks everyone, I finally figured it out. Converting to spherical coordinates and using the law of cosines to represent the norm of the vector difference is needed.
 
Man, this topic is quite old but I'm very interested in knowing how this problem is solved. I hope the topic provider os still there. How did you figure this problem out if you don't mind that I ask? I'm in a rush actually and really want to know how this problem is solved. Thanks!

PS: By the way, I'm the first time user. I think I made a mistake by sending the message via "report." Please ignore it the "report reply."
 

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