Find the steady-state temperature distribution in a spherical shell of inner radius 1 and outer radius 2 if the inner surface is held at 0°and the outer surface has its upper half at 100°and its lower half at role="math" localid="1664359640240" 0°. Hint: r = 0 is not in the region of interest, so the solutions rl1in (7.9) should be included. Replace clrlin (7.11) by(clrl+blrl1).

Short Answer

Expert verified

Therefore, the steady-state temperature distribution in a spherical shell is u(r,θ,ϕ)=l,m=0Al(i)rlPlm(cosθ)e±imϕ+l,m=0Bl(e)r(l+1)Plm(cosθ)e±imϕ.

Step by step solution

01

Given Information:

The inner radius of spherical shell is 1 and outer radius of spherical shell is 2.

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:

Solve Laplace equation for a sphere having radius r = a whereΔu=0.

Write Laplace operator in spherical coordinate.

Δ=1r2r(r2r)+1r2sinθθ(sinθθ)+1r2sin2θ2ϕ2

Solve the equation

u(r,θ,ϕ)=R(r)W(θ)Q(ϕ)

WQr2r(r2Rr)+RQr2sinθθ(sinθWθ)+RWr2sin2θ2Qϕ2=01Rr(r2Rr)+1Wsinθθ(sin(θ)Wθ)+1Qsin2θ2Qϕ2=0

04

Separate the equation by angle dependence:

Write equation for θdependence as below.

1Rr(r2Rr)+1Wsinθθ(sinθWθ)m2sin2θ=01Wsinθθ(sinθWθ)+m2sin2θ=αsinθθ(sinθWθ)m2W+αsin2(θ)W=0

W(θ)=Plm(cosθ)

Write equation for ϕ-dependence.

1Q2Qϕ2=m22Qϕ2+m2Q=0

Q(ϕ)=e±imϕ={Re(Q)=cos(mϕ)Im(Q)=sin(mϕ)

Write equation for r-dependence.

1Rr(r2Rr)=αr(r2Rr)αR=0r(r2Rr)αR=0r22Rr2+2rRrl(l+1)R=0

The general solution is Rl(r)=Alrl+Blr(l+1)

Therefore, the steady-state temperature distribution in a spherical shell is u(r,θ,ϕ)=u(i)(r,θ,ϕ)+u(e)(r,θ,ϕ)=l,m=0Al(i)rlPlm(cosθ)e±imϕ+l,m=0Bl(e)r(l+1)Plm(cosθ)e±imϕ

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Write the Schrödinger equation (3.22) if ψis a function ofx, and V=12mω2x2 (this is a one-dimensional harmonic oscillator). Find the solutions ψn(x)and the energy eigenvalues En . Hints: In Chapter 12, equation (22.1) and the first equation in (22.11), replace xby αxwhere α=mω/. (Don't forget appropriate factors of αfor the x' 's in the denominators of D=ddxand ψ''=d2ψdx2.) Compare your results for equation (22.1) with the Schrödinger equation you wrote above to see that they are identical if En=(n+12)ω. Write the solutions ψn(x)of the Schrödinger equation using Chapter 12, equations (22.11) and (22.12).

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