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Lesson 12 - Neutron sourcesChapter 4 is concerned with the description of the physical mechanisms that give rise to neutron, gamma ray, or x-ray sources. The chapter forms a excellent reference for all sorts of useful information, but we are going to be more selective with the material we concentrate on. Source description is the first step of any shielding analysis. In many cases, the particle sources will be known from:
The other cases is the situation where material properties are specified and the analyst has to deduce the source from this known material. This is the situation that we will be concentrating on. Basically, we will be looking at the MAJOR sources of particles that I think you should be aware of, with an eye toward sensitizing you to look for sources that are likely to "sneak up" on you if you are not careful. (Our greatest danger is to underestimate a source because we overlook a complete category.) The book lists 5 neutron source categories:
From the reading, you should be able to describe the physical mechanism for each of these (as I had you do in the Reading Assignment) and work very simple problems that require basic skills you already have (e.g., atom density determinations for nuclides, time-dependent buildup and decay, reaction rate determination from fluxes and cross sections). In addition, we will be covering more detail about two of these, which are the
mechanisms of spontaneous fission and sources due to
Spontaneous Fission SourcesThe first of the neutron that we will concentrate on is spontaneous fission, which is a version of fission that occurs without the benefit of an inducing neutron being absorbed. Several notes:
When considering any of these sources, we are concerned with two factors: the yield (number of particles produced) and the spectrum (energy distribution of the particles produced). For spontaneous fission, the yield depends only on the underlying mass; the most convenient form of data for this is usually something like the last column of Table 4.2. You should be able to determine spontaneous fission yields with data from this table.
For the spectrum, we generally use the Watt spectrum form given by Equations 4.1 and 4.2 (with data from Table 4.3). Note from Figure 4.1 that all nuclides have a similar shape, differing primarily in the high-energy "tail". (Note that the plotted spectra differ by about a factor of 10 at 15 MeV in Figure 4.1.) This difference can be more significant than the logarithmic y-axis of this figure implies, since it is these high energy particles that are most likely to penetrate shielding. Notice, though, the mixed nature of Figure 4.1 . For all isotopes except Cf-252, the curve is for induced fission; therefore, to use the figure for spontaneous fission, one has to recognize that the spontaneously fissioning nuclide is the nuclide we have AFTER the inducing neutron has been absorbed. For example, the curve for induced Pu-239 fission corresponds to spontaneous Pu-240 fission (since, of course, for a neutron causing a fission in Pu-239, the nuclide that breaks apart is the compound nucleus Pu-240).
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Group number, g |
Upper limit of group, ![]() |
1 | (![]() |
2 | (![]() |
3 | 5. |
4 | 2. |
5 | 1. |
6 | 0.5 |
7 | 0.2 |
8 | 0.1 |
9 | 0.05 |
10 | 0.02 |
11 | 0.01 |
12 | 0.005 |
13 | 0.002 |
14 | 0.001 = 1 keV |
Note that the highest energy limit (i.e., the top of group 1) is called .
Also, this is just an example. Usually neutron energy group structures go down to
thermal range, bottoming out at about 0.001 eV (=0.000000001 MeV).
For a distribution, , (which, you will remember would have "per unit energy"
units), the corresponding group value is found by a simple integration over the energy
range of the group:
The best examples of when you would do this are the energy spectra (e.g., the Watt fission spectrum) described in this lesson. The resulting group value corresponds to the fraction of produced particles that would be emitted in the given group.
Note: Be sure that the sum of your group values is 1.0. If not, you will need to normalize the values by dividing each group value by the sum of all group values.
For example, if we normalize the Watt spectrum representation of the Cf-252 fission spectrum (given by Equation 4.2 with Table 4.3 data inserted):
we would get the following values (in the above energy group structure):
Group number, g |
Upper limit of group, ![]() |
![]() |
1 | 20. MeV | 0.00231 |
2 | 10. | 0.06579 |
3 | 5. | 0.35378 |
4 | 2. | 0.28434 |
5 | 1. | 0.16783 |
6 | 0.5 | 0.09007 |
7 | 0.2 | 0.02269 |
8 | 0.1 | 0.00845 |
9 | 0.05 | 0.00355 |
10 | 0.02 | 0.00079 |
11 | 0.01 | 0.00028 |
12 | 0.005 | 0.00011 |
13 | 0.002 | .00003 |
14 | 0.001 = 1 keV | .00001 |
NOTE: The integrations were done using an S32 Gauss-Legendre quadrature integration. The FORTRAN coding for this is given here, in case you are interested.
You can "eyeball" a spectrum from a spectrum plot by estimating the average value over the group range and multiplying by the group width.
Example: Verify that the above value for group 3 is reasonable using Figure 4.1 in the text.
Answer: Group 3 goes from 2 MeV to 5 MeV. The value of the function falls over the group from about 0.2 (or so) to 0.03. If we take the average of these as an average value and multiply by the group width, we get 0.115*3 = 0.345 as our estimate. This compares okay with the 0.354 value in the table.
Although in this lesson we are only interested in distributions, for completeness it
should be mentioned that for functions of energy (e.g., cross sections) the group value
corresponds to the average value of the function over the energy range, so we have to
divide by the energy width. For example, for a function , the group
value would be given by the equation:
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