Heat conduction through sphere

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SUMMARY

The discussion focuses on solving heat conduction problems in spheres, specifically addressing two scenarios: a sphere with a cavity generating heat at a rate Q and a second sphere generating heat uniformly at q per unit volume. For part (a), the temperature at the cavity surface, T_a, is derived using the steady-state heat conduction equation and Newton's Law of Cooling. In part (b), the solution involves incorporating a source term into the heat conduction differential equation, leading to the temperature at the center of the sphere, T_0, being calculated with the modified equation that includes the heat generation term.

PREREQUISITES
  • Understanding of heat conduction principles and differential equations
  • Familiarity with Newton's Law of Cooling
  • Knowledge of steady-state solutions in thermal systems
  • Ability to solve partial differential equations
NEXT STEPS
  • Study the derivation of solutions for non-homogeneous heat conduction equations
  • Learn about the application of boundary conditions in thermal analysis
  • Explore the implications of heat generation terms in spherical coordinates
  • Investigate numerical methods for solving complex heat conduction problems
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Students and professionals in thermal engineering, physicists, and anyone involved in solving heat transfer problems in spherical geometries.

unscientific
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Homework Statement



In general, a sphere with conductivity ##\kappa##, heat capacity per unit volume ##C## and radius ##R## obeys the differential equation at time t:

C\frac{\partial T}{\partial t} = \kappa \frac{\partial^2 T}{\partial r^2} + \frac{2\kappa}{r}\frac{\partial T}{\partial r}

Part (a): A sphere with a cavity of radius ##a## generates heat at a rate Q. Heat is lost from the outer surface of the sphere to the surroundings, with surrounding temperature ##T_s##, given by Newton’s Law of Cooling with constant ##\alpha## per unit area. Find the temperature ##T_a## at the surface of the cavity at thermal equilibrium.

Part (b): A second sphere without a cavity generates heat uniformly at ##q## per unit volume. Like the first sphere, heat is lost to the surroundings at its surface. Find temperature at the center of the sphere ##T_0## at equilibrium.

Homework Equations


The Attempt at a Solution



Part (a)

Heat generated in cavity = Heat loss at surface
Q = \alpha (T_s - T_R)(4\pi R^2)
T_R = T_s - \frac{Q}{\alpha (4\pi R^2)}

We will use this to solve for the constants in the differential equation later on.

At steady state, ##C\frac{\partial T}{\partial t} = \kappa \frac{\partial^2 T}{\partial r^2} + \frac{2\kappa}{r}\frac{\partial T}{\partial r} = 0##.

\frac{\partial^2 T}{\partial r^2} + \frac{2}{r}\frac{\partial T}{\partial r} = 0

Solving, we get:

T = A + \frac{b}{r}

We need one more equation with the one for ##T_R## to solve for constants ##A## and ##B##.

Using ##\int \vec J \cdot d\vec S = k \int \nabla \vec T \cdot d\vec S##:
Q = -\kappa \frac{\partial T}{\partial r}(4\pi r^2)
Q = 4\pi \kappa b
b = \frac{Q}{4\pi \kappa}

Solving for A:
A = T_s - \frac{Q}{4\pi \alpha R^2} - \frac{Q}{4\pi \kappa R}

Together, temperature at surface of cavity is:

T_a = T_s - \frac{Q}{4\pi \alpha R^2} + \frac{Q}{4\pi \kappa}\left( \frac{1}{a} - \frac{1}{R} \right)

Part(b)

I'm not sure how to approach this, as ##T = A + \frac{b}{r}## doesn't work at ##r=0##..

I have found the temperature at surface though:
Q = \frac{4}{3}\pi R^3 q = \alpha (T_s - T_R)(4\pi R^2)
T_R = T_s - \frac{Rq}{3\alpha}
 
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You need to add the source term (q) in heat transfer partial differential equation.
You then again solve for the steady state solution.
 
maajdl said:
You need to add the source term (q) in heat transfer partial differential equation.
You then again solve for the steady state solution.

I don't understand what you mean. And is this for part (a) or part (b)?
 
I think you made a sign mistake in the Newton's law of cooling (part a). For part b you need a source term. That means you will solve the non-homogeneous heat conduction differential equation.
 
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unscientific said:
I don't understand what you mean. And is this for part (a) or part (b)?

This is for part b.

C\frac{\partial T}{\partial t} = \kappa \frac{\partial^2 T}{\partial r^2} + \frac{2\kappa}{r}\frac{\partial T}{\partial r} + q
 
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dauto said:
I think you made a sign mistake in the Newton's law of cooling (part a). For part b you need a source term. That means you will solve the non-homogeneous heat conduction differential equation.

For part (a), is the sign error here:

Q = \alpha (T_s - T_R)(4\pi R^2)

It should be ##T_r - T_s##, since the sphere is hotter. Other than that, is the rest of my working fine?


For part (b), I read up more on the chapter and I realized there should be a source per-unit-volume term per unit time term.

Thanks a lot!
 
dauto said:
I think you made a sign mistake in the Newton's law of cooling (part a). For part b you need a source term. That means you will solve the non-homogeneous heat conduction differential equation.

I have given this question another go. At steady state, the DE now becomes:

\kappa \frac{\partial^2T}{\partial r^2} + 2\frac{\kappa}{r} \frac{\partial T}{\partial r} + q = 0

Since the homogeneous solution is ##A + \frac{b}{r}##, we now seek the inhomogeneous solution.

I try ##\beta r^2## where I found ##\beta = -\frac{q}{6k}##.

So the solution for T is:
T = A + \frac{b}{r} - \frac{q}{6k}r^2

But now as ##r \rightarrow \infty##, ##T\rightarrow \infty##..
 

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