Chapter4-4

4.4 Steady-State Temperature in a Disk

Figure 4.4-1 A thin circular plate with insulated top and bottom surfaces

The two-dimensional Laplace equation in polar coordinate can describe the steady-state temperature distribution u(r,) in a thin disk as shown in Figure 4.4-1.

+ = 00 < ra, 0  < 2(4.4-1)

The boundary condition for the disk at the circumference is

u(a,) = f(), for 0  < 2

u(a,) and f() must be 2periodic. We assume that u(r,) can be separated into R(r), a function of r alone, and T(), a function of  alone.

u(r,) = R(r) T()(4.4-2)

Differentiating the partial derivative, we get

= R = R

= T = T

In terms of R(r) and T(), Eq. (4.4-1) becomes

T+ + R= 0(4.4-3)

Multiply Eq. (4.4-3) by to obtain

 = + = n2(4.4-4)

Since the RHS of Eq. (4.4-4) depends on r only, and the LHS depends on  only, they must equal to a constant n2. The constant must be chosen so that the solution is 2periodic in the -direction. The ODE on  is

=  n2T T = ancos(n) + bnsin(n), n = 0, 1, 2, 3, ...

The ODE on r is

+ = n2r2+ r n2R = 0

The equation for R is an Euler equation that has the following solution

R = r

The constant  can be determined by substituting R = r and its derivatives into the original ODE

( 1)r + r n2r = 0

2 +  n2 = 0  =  n

The solution for R is written in the dimensionless form

R(r) = rn + r-n R(r) = c1 + c2, n = 1, 2, 3, ...

The case for n = 0 must be solved separately

+ = 0 r+ = 0 = 0

= dR =  R = ln r +

The solution for the case n = 0 is finally

R = c1 + c2ln

Since the temperature and hence R must be finite at r = 0, c2 = 0. The constant c2will have a non zero value for temperature distribution outside a disk or on an annular region as shown in Figure 4.4-2.

Figure 4.4-2 The shaded areas indicate the region where 2u = 0 is solved.

The solution for R with the value of 1 for c1 is

R(r) = , n = 0, 1, 2, 3, ...

The product solution is

un(r,) = [ancos(n) + bnsin(n)]

Superposing these solutions, we get the general solution for the temperature distribution in a disk

u(r,) = [ancos(n) + bnsin(n)]

The coefficients an and bn can be obtained from the boundary condition at r = a.

u(a,) = f() = a0 + [ancos(n) + bnsin(n)]

The coefficients a0, an, and bn are the Fourier coefficients of the boundary function f().

a0 =

an =

bn =

1