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Astronuc
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Cross section data are available over ~12 orders of magnitude of neutron energy, from about 1E-5 ev up to 10 MeV.Moniz_not_Ernie said:Interesting geometry there. And I didn't know the fissions from fast neutrons was so high. But that depends on your definition of "fast". I have seen fission yield data for three speed bins, labeled 0.0253, 500K, and. 14 million eV. Do you include the middle energy bin in you 8-10%? What is your upper limit for slow neutrons?
I ask because I'm designing an MSR simulation. One basic question is whether we want fast or slow reactors. However, if the data comes in three speeds, So I may allow the user to choose reactor specs a little precisely. It will probably require aggregating ENDSF data into two or three bins. Wish I could contract that task out, but I'm on a tight budget ($=0).
I'm not a nuclear engineer. I'm a simulation designer, who got interested in this stuff through my hobbies; first astronomy (your username is intriguing), then cosmology and stellar evolution. I'll be asking some newbie questions here.
Many texts have the fission cross-sections for thermal (0.0235 eV), fast (~0.7 MeV), and 14.1 MeV (neutron energy from d,t fusion). These are arbitrary. For any simulation, e.g., steady-state core depletion or power distribution analysis in a reactor, one must consider the array of cross-sections from fissile and fertile isotopes, burnable poisons, fission products, coolant, and structural materials as functions of the energy spectrum. Fission neutrons are created in the MeV range (0.1 MeV to 10 MeV), so one has to consider the fission spectrum. In a thermal reactor, the thermal flux is somewhat less than the fast flux, but the thermal cross-sections are substantially greater, by about two to three orders of magnitude.
Data is compiled in various government issued databases.
http://www.nndc.bnl.gov/sigma/index.jsp?as=235&lib=endfb7.1&nsub=10