Solving for Potential in an Incompressible Self-Gravitating Fluid Slab

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To find the gravitational potential in an infinite slab of incompressible self-gravitating fluid, start by applying the Poisson equation and using Gauss's law for the gravitational field. The gravitational flux through a closed surface relates to the total mass inside, leading to the potential being derived from the gravitational field. Inside the slab, the potential is quadratic, while outside it is linear. Consideration of pressure and boundary conditions is essential, as they affect the dynamics of the fluid. The final expressions for the potential are V = (1/2)G rho (z)^2 for |z|<a and V = G rho a (|z| - (1/2)a) for |z|>a.
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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...
 
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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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