Solving for Potential in an Incompressible Self-Gravitating Fluid Slab

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SUMMARY

The discussion focuses on calculating the gravitational potential of an infinite slab of incompressible self-gravitating fluid with density ρ, confined within the region |z|a. The analysis also highlights the necessity of considering Euler's equations and mass continuity for a comprehensive understanding of the fluid dynamics involved.

PREREQUISITES
  • Understanding of gravitational potential and gravitational fields
  • Familiarity with the Poisson equation in gravitational contexts
  • Knowledge of Gauss's law and its application in physics
  • Basic concepts of fluid dynamics, particularly Euler's equations
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  • Study the derivation of the Poisson equation in gravitational fields
  • Learn about the application of Gauss's law in different geometries
  • Explore the implications of Euler's equations in incompressible fluid dynamics
  • Investigate boundary conditions in gravitational potential problems
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Physicists, mathematicians, and engineers working on gravitational fields, fluid dynamics, or related fields, particularly those interested in theoretical models of self-gravitating fluids.

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If I have an infinite slab of incompressible self-gravitating fluid of density rho within the region |z|<a, and I am asked to find the potential both inside and outside the slab, where should I start?
 
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With writing the (differential) equations which account for the dynamics...??

Daniel.
 
Do you mean by "potential" the gravitational potential and by "rho" the mass density?
 
A very fast solution to this problem can be obtained using a Gauss-like law for the gravitational field (it can be demostrated by direct integration of the Poisson equation and using the divergence theorem). The "gravitational flux" through a closed surface must equal the total mass inside the surface times gravitational constant.
\oint_S \vec{\Gamma}\cdot d\vec{S}=-\gamma \int \rho dv
Then, if you know \Gamma(z), the potential is just
V=-\int \Gamma dz
(for the integration constant you can impose V(0)=0)
You can choose a cylindrical gaussian surface with its axis parallel to Oz and play with this theorem. For this cylinder, the total flux is 2\Gamma S (S is basis area)

I think \Gamma will vary linearly from z=0 to z=a and would be uniform for z>a. So the potential will be quadratic and linear respectively...but you must verify that...
 
Last edited:
Your analysis would be okay,if the "infinite slab of incompressible self-gravitating fluid of density rho" would not mean what i think it does:namely a fluid to which u have to apply not only the Poisson equation (for a gravitostatic field),but also Euler's equations and the continuity of mass (for an incompressible fluid).You'd have then 5 equations with 5 unknowns:the gravity potential,the velocity field and the density field...
It would be really nasty,indeed.

Daniel.
 
Thanks Clive. But wouldn't using Gauss Law introduce a factor of 4*Pi? The answers have no 4*Pi in it. And do I have to consider also the pressure and the boundary condition?

By the way, here's the answers provided:
Code:
V = (1/2)G rho (z)^2             |z|<a
             = G rho a (|z| - (1/2)a)     |z|>a
 

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