Mass conservation for pulsating sphere

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SUMMARY

The discussion focuses on the mass conservation equation for a pulsating sphere, specifically addressing the relationship between density, speed, and mass calculation. The equation presented involves the ambient density ρ₀ and a small deviation ρ', leading to confusion regarding the physical interpretation of multiplying area by speed and density. Additionally, the substitution of ρ to ρ' on the left-hand side (LHS) raises questions about the accuracy of the equation, particularly regarding the type of time derivative used and the assumptions of spherical symmetry in density and velocity.

PREREQUISITES
  • Understanding of mass conservation principles in fluid dynamics
  • Familiarity with the equation of continuity in fluid mechanics
  • Knowledge of spherical coordinates and their applications
  • Basic grasp of time derivatives (total vs. partial) in mathematical physics
NEXT STEPS
  • Study the equation of continuity in detail, focusing on its applications in fluid dynamics
  • Research the implications of spherical symmetry in physical systems
  • Explore the differences between total and partial time derivatives in mathematical modeling
  • Investigate the physical significance of pulsating spheres in various scientific contexts
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This discussion is beneficial for physicists, fluid dynamics researchers, and students studying mass conservation in pulsating systems, particularly those interested in the mathematical modeling of dynamic fluid behaviors.

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Hi,

I'm trying to understand the mass conservation equation for a pulsating sphere which has thickness dr. Please refer to the attached solution.

\rho = \rho_{0} (ambient density) + \rho' (small deviation)

There are two things I don't follow.

First, is that to obtain the mass, the area of the sphere is multiplied by the speed (and density) at which it is pulsating. Although the units work out, I don't see the physical meaning behind taking the product with speed :confused:.

Secondly, on the LHS, the ρ turns into a ρ'. I can't see how this substitution was made.

Thanks for your input!
 

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It's not clear what you mean by "pulsating sphere." What changes and what stays the same? It looks like the density is changing. The drawing makes it look like the sphere is a shell with inside radius r and outside radius r + dr.

Can you make things a bit more clear?
 
The equation 1) mentioned in your figure doesn't look correct. It may be tentatively correct if the time derivative on the left hand side (L.H.S.) is really a total time derivative and not a partial time derivative(as indicated in the figure) and the deviations of the density are assumed to be sufficiently small.
Also apparently spherical symmetry appears to have been assumed for the density and the velocity.
If you want to figure things out for yourself you can start out with the equation of continuity:
\nabla.(\rho\bar{v}) = -\frac{\partial\rho}{\partial t}
 

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