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Find the steady-state temperature distribution inside a sphere of radius 1 when the surface temperatures are as given in Problems 1 to 10.

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Short Answer

Expert verified

The steady-state temperature distribution inside a sphere of radius 1:

12P0(cosθ)+58r2P2(cosθ)−316r4P4(cosθ)+…

Step by step solution

01

Given Information

The surface temperature of sphere of radius 1 is|cos(θ)|.

02

Definition of steady-state temperature:

When a conductor reaches a point where no more heat can be absorbed by the rod, it is said to be at steady-state temperature.

03

Calculate the steady-state temperature distribution function

The standard Legendre polynomials is Pl(cos(θ)).

For simplicity, considerx=cosθ.

ur=1=|cos(θ)|=|x|

It is known that:

u=∑l=0∞clrlPl(cosθ).

Hence,

cm=2m+12∫−11|x|pm(x)dx … (1)

04

Simplify further

Take m = 0 and put in equation (1).

c0=12∫−11|x|dx=12[x22]−11=0

Take m = 1 and put in equation (1).

c1=32∫−11|x|dx=32[x22]−11=0

Take m = 2 and put in equation (1).

c2=54∫−11|x|(3x2−1)dx=54∫−11(3|x|x2−|x|)dx=54(3x44−x22)−11=54(34−12−34+12)

c2=58

Take m = 3 and put in equation (1).

c3=0

Take m = 4 and put in equation (1).

c4=916∫−11|x|(35x4−30x2+3)dx=2×916∫01(35x5−30x3+3x)dx

c4=98(35x66−30x44+3x22)01dx=98(356−304+32)=98(140−180+3624)

c4=98(356−304+32)=98(140−180+3624)=98(−424)=−316

Use the equation s given below.

u=∑l=0∞clrlPl(cosθ)

u=12P0(cosθ)+58r2P2(cosθ)−316r4P4(cosθ)+…

Hence the steady-state temperature distribution inside a sphere of radius 1:

12P0(cosθ)+58r2P2(cosθ)−316r4P4(cosθ)+….

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Most popular questions from this chapter

Consider the heat flow problem of Section 3. Solve this by Laplace transforms (with respect to t) by starting as in Example 1. You should get ∂2U∂x2−pα2U=−100α2lxand U(0,p)=U(l,p)=0.

Solve this differential equation to getU(x,p)=−100sinh(p1/2/α)xpsinh(p1/2/α)l+100plx

Assume the following expansion, and find u by looking up the inverse Laplace transforms of the individual terms of U:

sinh(p1/2/α)xpsinh(p1/2/α)l=xpl−2π[sin(πx/l)p+(π2α2/l2)−sin(2πx/l)2[p+(4π2α2/l2)]+sin(3πx/l)3[p+(9π2α2/l2)]⋯]sin−1θ

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Where G(r,r')is the Green function (8.28) which is zero on the surface σ, and ∂G/∂n'=∇G⋅n'is the normal derivative of G (see Chapter 6, Section 6).

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