Pressure in Hydrostatic Equlibrium

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SUMMARY

The discussion focuses on determining the pressure as a function of radius (r) in a hydrostatic equilibrium scenario where the density is defined as ρ = ρ₀ (r₀/r)². The primary challenge identified is the infinite density at r = 0, leading to an infinite pressure, which complicates calculations. Participants suggest that while the model may suffice for pressures at r = R or r = R/2, it is inadequate for evaluating pressure near the center (r = 0). An alternative model is proposed, incorporating a small parameter ε to avoid the singularity at r = 0.

PREREQUISITES
  • Understanding of hydrostatic equilibrium principles
  • Familiarity with density functions and their implications in physics
  • Knowledge of calculus, specifically integration techniques
  • Experience with Taylor series expansions and approximations
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  • Learn about pressure calculations in non-uniform spherical bodies
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Students and professionals in physics, particularly those studying astrophysics or fluid mechanics, as well as anyone interested in the mathematical modeling of pressure in spherical objects.

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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 \rho = \rho_o {(\frac{r_o}{r})}^2.

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 r_o 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: \rho = \rho _0 (\frac{r_o}{r+\epsilon})^2 where \epsilon &lt;&lt; R (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.
 

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