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

3sinθcosθsinϕHint: See equation (7.10) and Chapter 12, equation (10.6).

Short Answer

Expert verified

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

u(r,θ,ϕ)=τ=0{18(2τ+1)τ(τ+1)(Pτ(1)Pτ(1))+9τ(τ+1)[Pτ1(1)Pτ+1(1)]}rτPτ1(x)sin(ϕ)

Step by step solution

01

Given Information:

The radius of the sphere is 1.

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 function u(r,θ)inside a sphere with a radius of r = 1 in this issue. The surface temperature function is written asA(θ,ϕ).

Consider the equation below:

A(θ,ϕ)=3sin(θ)cos(θ)sin(ϕ)=31cos2(θ)cos(θ)sin(ϕ)

The surface temperature function A(θ,ϕ), unlike previous problems, is dependent onϕ.

The steady-state temperature distribution function will be written in a Power series that explicitly includes the corresponding Legendre polynomials Plm(cos(θ))due to the ϕdependence. From an algebraic standpoint, the analogous Power series is of the type .

u(r,θ)=l=0clrlPlm(cos(θ))

Its coefficients are calculated by expressing it as Plm(cos(θ))in terms of the corresponding Legendre polynomials. Let x=cos(θ)be the chosen value.

ur=1(x)=l=0clPl1(x)

ur=1(x)=31x2xsin(ϕ) ….. (1)

The term sin(mϕ)as one functional portion of the spherical harmonics Ylm(θ,ϕ)determines the of the corresponding Legendre polynomials Plm(cos(θ)). As can be observed from the surface temperature function A(x,ϕ)=31x2xsin(ϕ), where m=1in this case.

04

Simplify Legendre polynomials:

Write the Legendre polynomials with associated orthogonally:

11Pl1(x)Pτ1(x)dx=2(2l+1)(l+1)!(l1)!δl,τ ….. (2)

11Pl1(x)Pτ1(x)dx=2(2l+1)(l+1)!(l1)!δl,τ=2(2l+1)(l+1)l(l1)!(l1)!δl,τ=2l(l+1)(2l+1)δl,τ

Standard Legendre polynomials have the following identity:

a1Pn(x)dx=1(2n+1)[Pn1(a)Pn+1(a)] ….. (3)

Use integration by part in 1x2xPτ1(x)dx:

1x2xPτ1(x)dx=(1x2)xPτ(x)dx=(xx3)Pτ(x)dx=(xx3)Pτ(x)(13x2)Pτ(x)dx=(xx3)Pτ(x)[(13x2)Pτ(x)(6x)Pτ(x)dx]

1x2xPτ1(x)dx=(xx3)Pτ(x)(13x2)Pτ(x)+[(6x)Pτ(x)(6)Pτ(x)dx]=(xx3)Pτ(x)(13x2)Pτ(x)(6x)Pτ(x)+6Pτ(x)dx

Equations (2) and (3), as well as the multiple integration section, should be inserted into equation (1).

l=0cl2l(l+1)(2l+1)δl,τ=3(12(Pτ(1)Pτ(1))+6(2τ+1)[Pτ1(1)Pτ+1(1)])cτ2τ(τ+1)(2τ+1)=36(Pτ(1)Pτ(1))+18(2τ+1)[Pτ1(1)Pτ+1(1)])cτ=18(2τ+1)τ(τ+1)(Pτ(1)Pτ(1))+9τ(τ+1)[Pτ1(1)Pτ+1(1)]


u(r,θ,ϕ)=τ=0{18(2τ+1)τ(τ+1)(Pτ(1)Pτ(1))+9τ(τ+1)[Pτ1(1)Pτ+1(1)]}rτPτ1(x)sin(ϕ)

Therefore, the steady-state temperature distribution inside a sphere of radius 1 isu(r,θ,ϕ)=τ=0{18(2τ+1)τ(τ+1)(Pτ(1)Pτ(1))+9τ(τ+1)[Pτ1(1)Pτ+1(1)]}rτPτ1(x)sin(ϕ).

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