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20     CHAPTER 3 The point reactor kinetics equations




                         There are differences between the delayed neutron data for thermal fissions and fast
                         fissions in U-235, U-233 and Pu-239, but they are small.
                            The reader should be aware that different references report slightly different
                         values for delayed neutron data. These differences have little influence on practical
                         reactor simulations. Also, note that Pu-239 and U-233 have much smaller delayed
                         neutron fractions than U-235. This has an impact on dynamic behavior.
                            A reactor fueled with low-enrichment U-235 produces Pu-239 by neutron capture
                         in U-238. Consequently, the ratio of Pu-239 to U-235 increases as the reactor oper-
                         ates and the “effective” delayed neutron fraction decreases.
                            A single delayed neutron group is often used for approximate calculations. In this
                         case, approximate average values for the effective delayed neutron fraction and
                         effective delayed neutron decay constant are required. Typical values for a U-235
                         fueled reactor are 0.0067 for the effective delayed neutron fraction and 0.08s  1
                         for the effective decay constant (see Section 4.6 for calculating the effective decay
                         constant). The main utility of the model with a single delay group is that it provides a
                         simple, easy-to-implement tool for illustrating the features of reactor transients. We
                         will use the model with a single delayed neutron precursor group for illustrating some
                         features of a reactor transient, but the full six-group model will be used in simulations
                         to illustrate reactor maneuvers.


                         3.2.2 Photoneutrons from nuclei excited by gamma rays
                         Several isotopes can produce photoneutrons by interaction with high energy gamma
                         rays produced in fission reactions. The materials that can produce neutrons by inter-
                         acting with fission gamma rays are deuterium, lithium, beryllium, and carbon. These
                         materials have a small enough binding energy (all have binding energies of 7.25MeV
                         or less) to enable photoneutron-producing reactions with gamma rays having ener-
                         gies that occur during fission reactions. Fission gamma rays are not energetic enough
                         to cause (γ, n) reactions in other materials.
                            In photoneutron production, the high energy gamma ray causes the target nucleus
                         to transition to an excited state. This excited state persists until the nucleus emits a
                         neutron. The process of neutron emission follows the law of radioactive decay as
                         characterized by a half-life. The different photoneutron producing nuclei have
                         half-lives ranging from around 2.5s to 12.5days.
                            The photoneutron yield is much smaller than the delayed neutron yield from
                         fission products, but the half-lives of some of the photoneutron precursors are
                         much longer than the precursor half-lives of delayed neutrons from fission
                         products. Consequently, photoneutron production can become larger than delayed
                         neutron production from fission products after time passage following shutdown
                         of the reactor. This occurs after several minutes after shutdown in CANDU
                         reactors.
                            Photoneutrons are produced in reactors that use Deuterium by the (γ, n) reaction
                         between Deuterium and 2.225MeV gamma rays. The coolant and moderator in
                         CANDU reactors are almost pure D 2 O. Even light water reactors have a small
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