Pressure in Hydrostatic Equlibrium

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zachzach
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Homework Statement



Find the pressure as a function of r for the region r<< R where R is the radius of the object. The density goes as [tex]\rho = \rho_o {(\frac{r_o}{r})}^2[/tex].

Homework Equations


I know how to get to the answer my problem is dealing with the infinite density at r = 0.

The Attempt at a Solution



My pressure integrates to an equation that is inversely proportional to the square of r. But at r = 0 the central pressure, will be infinite. How can you deal with this infinite. It makes sense since the density is infinite at r = 0, but there must be an answer. If the [tex]r_o[/tex] was an R you could do a taylor expansion but it is not.
 
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Then just take it as an approximate model :wink: A better model may look somewhat like this: [tex]\rho = \rho _0 (\frac{r_o}{r+\epsilon})^2[/tex] where [tex]\epsilon << R[/tex] (I devise it, so don't take it for real :biggrin:). If you're interested in the pressure at r=R, r=R/2, etc, then the model given by the problem might be sufficient. If you're interested in the pressure near the center of the object, then there is a need for another model.
In short, don't take the formula given in the problem too seriously :smile:
 
Hi,
Sorry, I overlooked the r<<R part, which made my reply above rather stupid :biggrin: But then, my conclusion is still the same: this model is not sufficient for calculating pressure near r=0. It's very non-intuitive to have the density to go to infinity, and thus, this non-intuitive model will probably lead to non-intuitive result.