Final answer:
The differential equation for steady-state heat conduction through a sphere is derived using the heat equation in spherical coordinates with boundary conditions accounting for symmetry at the center and a set temperature at the surface.
Step-by-step explanation:
To derive the differential equation for heat conduction through a homogeneous spherical piece of radioactive material, we use the heat equation in spherical coordinates assuming steady-state conditions and one-dimensional radial heat transfer. This equation can be expressed as:
dT/dr = (1/r^2) * (d/dr) (r^2 * (-k) * dT/dr) + g/k
where T is the temperature, r is the radial coordinate, k is the thermal conductivity, and g is the volumetric heat generation rate.
The boundary conditions for this problem are:
- At r = 0, the symmetry requires that (d/dr)(-k * dT/dr) = 0, meaning the radial derivative of the heat flux is zero.
- At r = r0, the temperature is maintained at 80°C, so T(r0) = 80°C.
We can then solve this differential equation with the given boundary conditions to find the temperature distribution within the sphere.