Heat conduction through sphere

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Homework Help Overview

The discussion revolves around heat conduction in spheres, specifically addressing a sphere with a cavity and a second sphere without a cavity. The participants explore the differential equations governing heat transfer, including the effects of heat generation and loss to the surroundings.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants discuss the application of Newton's Law of Cooling and the need to include source terms in the heat transfer equations. There are attempts to derive temperature equations for both parts of the problem, with some questioning the correctness of signs in the equations.

Discussion Status

There is ongoing exploration of the differential equations, with some participants suggesting corrections to previous attempts. Multiple interpretations of the equations are being considered, particularly regarding the steady-state solutions and the inclusion of source terms.

Contextual Notes

Participants note potential sign errors in the application of Newton's Law of Cooling and the necessity of addressing the non-homogeneous nature of the heat conduction equations for part (b). There is also mention of the challenge posed by the behavior of the solutions as variables approach certain limits.

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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