In this post we derived the
Helmholtz equation
∇2ϕ+B2ϕ=0
We saw how this can be solved
in 2-dimensions. However, in the simple case of a slab reactor of width a in
the x direction, and infinite in the y and z directions the Helmholtz
equation reduces to 1-dimension:
dx2d2ϕ+B2ϕ=0
We can place the slab at x=0 with its width in the interval
[−2a,2a]. We know that the flux must be
symmetric about x=0, and that the flux must be 0 at the extrapolated
boundaries, ±2aex. The boundary conditions are then
ϕ(2aex)=ϕ(−2aex)=0
Furthermore, because of the symmetrical geometry there is no net flow of
neutrons at the center of the slab. Because the neutron current density is
proportional to the derivative of ϕ, at the center of the slab i.e. at x=0,
dxdϕ=0
Again, because the geometry of the slab is symmetric around x=0 this is
equivalent to the condition of ϕ being an even function
ϕ(−x)=ϕ(x)
The 1-dimensional form of the flux equation has the general solution
ϕ(x)=Acos(Bx)+Csin(Bx),
where A and C are unknown constants. Taking the derivative and using the
condition that the derivative is 0 at x=0 we get that C=0. The flux
equation, therefore, becomes
ϕ(x)=Acos(Bx)
Applying the boundary condition stated above that the flux at the extrapolated
boundaries is 0,
ϕ(2aex)=Acos(2Baex)=0,
gives A=0 with the trivial solution ϕ(x)=0, or that
cos(2Baex)=0
This solution leads to B taking values Bn,
Bn=aexnπ,
for odd values of n. The square of the lowest value of B, i.e. B12, is
the buckling of the reactor, which represents the fuel material in an infinite
medium. Under non-critical conditions, the reactor flux is the sum of the
cosine functions for all values of Bn, i.e.
ϕ(x)=n≥∑Acos(Bnx)=n≥0∑Acos(aexnπx)
However, the only physically possible case is that of a critical reactor where
all the cosine functions except the first one die out in time. And so, the
flux in a critical slab reactor is given by
ϕ(x)=Acos(B1x)=Acos(aexπx)
Note that the value of the constant A, which determines the magnitude of the
flux, has not been determined. Because the Helmholtz equation we started with is
homogeneous, multiplying the flux by any constant still gives a valid solution.
Furthermore, the magnitude of the flux in the reactor is determined by the
reactor power rather than its material properties. The recoverable energy per
fission in a nuclear reactor, Ef, is 200 MeV=3.2×10−11 J. There are, therefore, Σfϕ(x) fissions per cm3s−1
at the point x, where Σf is the macroscopic cross section. And so, the
power, P (watts/cm2), is
P=EfΣf∫−2a2aϕ(x)dx
Substituting in and integrating the expression we found for the reactor flux we get
P=π2aexEfΣfAsin(2aexπa)
Rearranging this we get the constant A as
A=2aEfΣfsin(2aexπa)πP
And so, the thermal flux in a slab reactor can be expressed as
ϕ(x)=2aexEfΣfsin(2aexπa)πPcos(aexπx)
Lamarsh, A. J. Baratta, Introduction to Nuclear Engineering, 3d ed.,
Prentice-Hall, 2001, ISBN: 0-201-82498-1.