Deriving the critical radius of Uranium using diffusion equation

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SUMMARY

The discussion focuses on deriving the critical radius of Uranium using the diffusion equation, specifically the equation del squared (n) - A(dn/dt) = -Bn. The user has solved for neutron density in spherical coordinates and established boundary conditions where neutron density is zero at the surface of the sphere. They deduced that at the critical radius, the neutron density must be stable, leading to the condition B-K = 0. The challenge lies in determining the integer value of m to eliminate the infinite solutions for the critical radius.

PREREQUISITES
  • Understanding of diffusion equations in physics
  • Knowledge of spherical coordinates and boundary conditions
  • Familiarity with neutron density concepts in nuclear physics
  • Basic grasp of separation constants and their application in differential equations
NEXT STEPS
  • Research boundary conditions in diffusion equations
  • Study the implications of spherical symmetry in neutron diffusion
  • Learn about the physical properties of Uranium affecting neutron behavior
  • Explore methods to determine integer values in boundary value problems
USEFUL FOR

Students and researchers in nuclear physics, particularly those studying neutron diffusion and critical radius calculations in Uranium. This discussion is also beneficial for anyone tackling advanced differential equations in a physical context.

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Homework Statement



I have solved the equation for the neutron density as a function of position and time. I need the boundary conditions to change my infinite number of solutions (the varying separation constant) into one value so that my answer for the critical radius does not contain a sum!

Homework Equations



del squared (n) - A(dn/dt) = -Bn (which i have solved)

The Attempt at a Solution



i assumed spherically symmetric solutions so using spherical polar coordinates n varies only (spatially) from the distance to the centre of the sphere. The r dependence is of form cos(kr)/r + sin(kr)/r. So the coefficients of cos term must all be 0 (as the density at the centre of any given sphere cannot be infinite). I thought that at the surface, the density is 0 as neutrons do not diffuse back into the sphere once they are out. Is this right?
 
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maybe i should add a little more to this. The time dependence part of the neutron density is found to be exp(B-K)t where K=k*k (k is the separation constant). now at the critical radius i know that the neutron density cannot be increasing or decreasing with time (it must be stable). So i reasoned that B-K = 0. If also we reason that the density of neutrons on the surface of a sphere R must be zero, then we have that sin(kR)=0 or kR=m*pi where m is an integer. So k=m*pi/R and subbing this to B-K=0, i have an expression for the critical radius in terms of B (which are the product of some intrinsic properties of uranium like mean free path etc). The only problem I have now is that the expression for R, the critical radius, contains m! so I have infinitely many expressions! How do I fix the value of m using the boundary conditions?! this is driving me insane..
 
Help Please!
 

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