Nuclear fission can occur when a nucleus is rendered sufficiently unstable by the absorption of a passing neutron. The probability for such a fission reaction to take place depends on how energetic these neutrons are, and so the knowledge of their energies spectrum is vital for an understanding of how nuclear reactors work. The custom is to classify these neutrons in groups corresponding to their energy ranges, the most important of which are the 'fast' and 'slow' neutrons.
After a series of collisions with different nuclei, the energy of neutrons produced by fission reactions drops to the order of a few electronvolts or a few fractions of an electronvolt. Neutrons with energies in this range are collectively referred to as 'slow', and neutrons whose energies match those of the surrounding atoms are known as 'thermal'.
It is these slow neutrons that allow for nuclear reactors to run with fuel based on natural uranium or uranium lightly-enriched in fissile isotope 235. Without them, the most common pressurised (PWR) and boiling water (BWR) reactors would not operate. As a result, the neutrons emitted by nuclear fission have to be slowed down by collisions with a 'moderating' medium. Reactors based on natural uranium, which contains comparatively little of the enriched uranium 235, require the use of special moderators which absorb very few of the neutrons : such moderators are heavy water and pure graphite.
TMORE ON SLOW NEUTRONS
Before they are slowed down by a large number of nuclear collisions, neutrons produced by fission reactions are known as 'fast'. They usually have energies between 0.1 and 2 or 3 MeV.
The fact that they possess a substantial amount of kinetic energy allows fast neutrons to fission more easily nuclei once they get captured. They can therefore split not only nuclei reputed fissile by slow neutrons, but also minor actinides, the heavy nuclei which build up inside nuclear fuel as radioactive waste. Fast neutrons are needed to eliminate these waste products.
The use of fast neutrons in so-called ‘fast reactors’ allows for the production of more fissile nuclei than are destroyed, as the absorption of at least one neutron per fission by an uranium 238 nucleus transforms this uranium 238 into a fissile plutonium 239 nucleus. This process is known as breeding, leading to an almost inexhaustible supply of nuclear fuel.
One drawback of fast neutrons in reactors is that the probabilities of their capture by nuclei are comparatively small. Travelling in matter, neutrons see nuclei as targets. The apparent cross-section of these targets is much more smaller for fast neutrons than it is for slower neutrons. As a result, an intense neutron flux and a fuel rich in fissile elements are both needed to compensate for this lower probability.
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