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Do Problem 11 if the curved surface is held at cos2θand the equatorial plane at zero. Careful: The answer does not involve P2; read the last sentence of this section.

Short Answer

Expert verified

Therefore, the steady-state temperature distribution inside a hemisphere isu(r,θ)=s=0{[Ps1(0)Ps+1(0)](2s+1)Ps(1)}(ra)sPs(x).

Step by step solution

01

Given Information:

The angle of the curved surface of hemisphere is cos2θand with the equatorial plane at0°.

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 a steady-state temperature.

03

Calculate the steady-state temperature distribution function:

Compute the steady-state temperature distribution u(r,θ)inside a hemisphere with a radius of a' in this problem. The equatorial plane is maintained at a temperature of 0°, whereas the spherical surface A(θ)is maintained at a temperature ofcos2θ.

Because there is no ϕdependence, express A(θ)in terms of standard Legendre polynomials in order to determine the associated coefficients clinside the Power series.

A(θ)=cos2θ0<θ<π20π2<θ<π

Substitute x=cosθandθx.

A(x)=01<x<0x20<x<1=x201<x<01   0<x<1=x2f(x)

04

Simplify Legendre polynomials:

Write A(x)standard Legendre polynomials Pl(x)for radius r = a.

ur=a(x)=l=0clalPl(x)

ur=a(x)=x2f(x) ….. (1)

Multiply Ps(x)in equation (1) and integrate.

l=0clal01Pl(x)Ps(x)dx=01x2f(x)Ps(x)dx ….. (2)

The orthogonal relation of standard Legendre polynomials is as follows:

01Pl(x)Ps(x)dx=1211Pl(x)Ps(x)dx

01Pl(x)Ps(x)dx=122(2l+1)δl,s ….. (3)

Use identity of Legendre polynomial. i.e.b1Pn(x)dx=1(2n+1)[Pn1(b)Pn+1(b)]

Use integration by part in equation (2).

01x2f(x)Ps(x)dx=01x2Ps(x)dx=x2Ps(x)|01012xPs(x)dx=Ps(1)2xPs(x)|01+201Ps(x)dx=Ps(1)2Ps(1)+2(2s+1)[Ps1(0)Ps+1(0)]

01x2f(x)Ps(x)dx=Ps(1)+2(2s+1)[Ps1(0)Ps+1(0)]

Calculate the value of coefficientcl.

Substitute equation (3) in equation (2).

l=0clal122(2l+1)δl,s=Ps(1)+2(2s+1)[Ps1(0)Ps+1(0)]csas1(2s+1)=1(2s+1)[Ps1(0)Ps+1(0)]Ps(1)cs=1as([Ps1(0)Ps+1(0)])(2s+1)Ps(1))

u(r,θ)=s=0[Ps1(0)Ps+1(0)](2s+1)Ps(1)(ra)sPs(x)

Therefore, the steady-state temperature distribution inside a hemisphere isu(r,θ)=s=0[Ps1(0)Ps+1(0)](2s+1)Ps(1)(ra)sPs(x).

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