skip to content
Aymen Hafeez

Neutron flux in an infinite slab reactor

/ 4 min read

Table of Contents

In this post we derived the Helmholtz equation

2ϕ+B2ϕ=0\begin{equation*} \begin{aligned} \nabla^2\phi + B^2\phi = 0 \end{aligned} \end{equation*}

We saw how this can be solved in 2-dimensions. However, in the simple case of a slab reactor of width aa in the xx direction, and infinite in the yy and zz directions the Helmholtz equation reduces to 1-dimension:

d2ϕdx2+B2ϕ=0\begin{equation*} \begin{aligned} \frac{\text{d}^2 \phi}{\text{d} x^2} + B^2\phi = 0 \end{aligned} \end{equation*} Infinite slab reactor diagram

We can place the slab at x=0x = 0 with its width in the interval [a2,a2]\left[-\frac{a}{2}, \frac{a}{2}\right]. We know that the flux must be symmetric about x=0x = 0, and that the flux must be 0 at the extrapolated boundaries, ±aex2\pm\frac{a_{ex}}{2}. The boundary conditions are then

ϕ(aex2)=ϕ(aex2)=0\begin{equation*} \begin{aligned} \phi\left(\frac{a_{ex}}{2}\right) = \phi\left(-\frac{a_{ex}}{2}\right) = 0 \end{aligned} \end{equation*}

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\phi, at the center of the slab i.e. at x=0x = 0,

dϕdx=0\begin{equation*} \begin{aligned} \frac{\text{d} \phi}{\text{d} x} = 0 \end{aligned} \end{equation*}

Again, because the geometry of the slab is symmetric around x=0x = 0 this is equivalent to the condition of ϕ\phi being an even function

ϕ(x)=ϕ(x)\begin{equation*} \begin{aligned} \phi(-x) = \phi(x) \end{aligned} \end{equation*}

The 1-dimensional form of the flux equation has the general solution

ϕ(x)=Acos(Bx)+Csin(Bx),\begin{equation*} \begin{aligned} \phi(x) = A\cos(Bx) + C\sin(Bx), \end{aligned} \end{equation*}

where AA and CC are unknown constants. Taking the derivative and using the condition that the derivative is 0 at x=0x = 0 we get that C=0C = 0. The flux equation, therefore, becomes

ϕ(x)=Acos(Bx)\begin{equation*} \begin{aligned} \phi(x) = A\cos(Bx) \end{aligned} \end{equation*}

Applying the boundary condition stated above that the flux at the extrapolated boundaries is 0,

ϕ(aex2)=Acos(Baex2)=0,\begin{equation*} \begin{aligned} \phi\left(\frac{a_{ex}}{2}\right) = A\cos\left(\frac{Ba_{ex}}{2}\right) = 0, \end{aligned} \end{equation*}

gives A=0A = 0 with the trivial solution ϕ(x)=0\phi(x) = 0, or that

cos(Baex2)=0\begin{equation*} \begin{aligned} \cos\left(\frac{Ba_{ex}}{2}\right) = 0 \end{aligned} \end{equation*}

This solution leads to BB taking values BnB_n,

Bn=nπaex,\begin{equation*} \begin{aligned} B_n = \frac{n \pi}{a_{ex}}, \end{aligned} \end{equation*}

for odd values of nn. The square of the lowest value of BB, i.e. B12B_1^2, 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 BnB_n, i.e.

ϕ(x)=nAcos(Bnx)=n0Acos(nπxaex)\begin{equation*} \begin{aligned} \phi(x) = \sum_{n \geq}^{} A\cos(B_n x) = \sum_{n \geq 0}^{} A\cos\left(\frac{n\pi x}{a_{ex}}\right) \end{aligned} \end{equation*}

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(πxaex)\begin{equation*} \begin{aligned} \phi(x) = A\cos(B_1 x) = A\cos\left(\frac{\pi x}{a_{ex}}\right) \end{aligned} \end{equation*}

Note that the value of the constant AA, 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, EfE_f, is  200 MeV=3.2×1011 J~200 \text{ MeV} = 3.2 \times 10^{-11} \text{ J}. There are, therefore, Σfϕ(x)\Sigma_f \phi(x) fissions per cm3^3s1^{-1} at the point xx, where Σf\Sigma_f is the macroscopic cross section. And so, the power, PP (watts/cm2^2), is

P=EfΣfa2a2ϕ(x)dx\begin{equation*} \begin{aligned} P = E_f\Sigma_f \int_{-\frac{a}{2}}^{\frac{a}{2}} \phi(x) \text{d} x \end{aligned} \end{equation*}

Substituting in and integrating the expression we found for the reactor flux we get

P=2aexEfΣfAsin(πa2aex)π\begin{equation*} \begin{aligned} P = \frac{2a_{ex}E_f\Sigma_fA\sin\left(\frac{\pi a}{2a_{ex}}\right)}{\pi} \end{aligned} \end{equation*}

Rearranging this we get the constant AA as

A=πP2aEfΣfsin(πa2aex)\begin{equation*} \begin{aligned} A = \frac{\pi P}{2aE_f\Sigma_f\sin\left(\frac{\pi a}{2a_{ex}}\right)} \end{aligned} \end{equation*}

And so, the thermal flux in a slab reactor can be expressed as

ϕ(x)=πP2aexEfΣfsin(πa2aex)cos(πxaex)\begin{equation*} \begin{aligned} \phi(x) = \frac{\pi P}{2a_{ex}E_f\Sigma_f\sin\left(\frac{\pi a}{2a_{ex}}\right)}\cos\left(\frac{\pi x}{a_{ex}}\right) \end{aligned} \end{equation*}

References:

Lamarsh, A. J. Baratta, Introduction to Nuclear Engineering, 3d ed., Prentice-Hall, 2001, ISBN: 0-201-82498-1.