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Published byAvice Lewis Modified over 6 years ago
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Scattering Reactions Scattering reactions - the incident particle collides with the target nucleus Elastic scattering – a collision between a particle and nucleus where the kinetic energy and momentum is conserved 0η1 + ZXA → ZXA + 0 η1 Inelastic scattering – a collision between a particle and a nucleus where a portion of the kinetic energy is used to raise the target nucleus to a higher energy level 0 η1 + ZXA → ZYA+1 * → ZXA η1 + γ
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Absorption Reactions Absorption reactions – the incident radiation transfers energy by becoming part of the nucleus Radiative capture – incident particle is captured by nucleus and excess energy is carried off by gamma emission 0η1 + ZXA → ZYA + 1 * → zXA γ Particle emission – incident particle is absorbed by the nucleus and the resultant excitation energy is high enough that a particle is ejected from the nucleus 0η1 + ZXA → ZYA + 1 * → Y + γ + p (p = particle; mass number of resultant nucleus is dependent on particle ejected, i.e. proton, neutron, or alpha) Fission – particle is absorbed by a heavy nucleus splitting the nucleus into fission fragments with the emission of neutrons 0η1 + ZXA → ZYA + 1 → 2FF + 0η1(s) + γ + E (FF = fission fragments; average number of neutrons released per fission is ~2.5)
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Neutron Production Fission 235U + 1η → 236U → 2 FF + ~2.5 1 η + Q
FF = fission fragment = average number Alpha neutron reactions (α,η) 4 α + 9Be → 12C + 1 η Photoneutron reactions (γ,η) γ + 9Be → 8Be* + 1 η *excited state
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Neutron Energy Classification
Fast neutrons > 0.1 MeV Intermediate neutrons 1.0 eV to 0.1 MeV Slow neutrons < 1.0 eV Thermal neutron kinetic energy equals the atoms of the material around them
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Prompt vs. Delayed Neutrons
Prompt neutrons are released when the fission event occurs Delayed Neutrons are released after the fission event Within seconds 10-14 seconds up to 89 seconds Average energy 2 MeV Average energy 0.5 MeV Occur in 99.36% of fission events Occur in 0.64% of fission events
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Moderator Properties Atomic mass close to that of a neutron
Small atomic cross section for neutron absorption Large cross section for neutron scatter Chemically non-reactive with reactor materials Provides a large energy loss per collision Stable isotope to avoid changing cross section characteristics
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Reactor States Subcritical – the number of neutrons in a generation is less than the number of neutrons in the previous generation Critical – the number of neutrons in a generation is equal to the number of neutrons in the previous generation Supercritical – the number of neutrons in a generation is greater than the number of neutrons in the previous generation
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Keff Keff = 1, the reactor is critical
Keff < 1, the reactor is subcritical Keff > 1, the reactor is supercritical
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Reactivity Coefficients
Changes in reactivity coefficients add positive or negative reactivity to the reactor system Moderator temperature coefficient Fuel temperature coefficient Pressure coefficient Void coefficient
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Neutron Absorbers and Poisons
Control Rods 1n Boric Acid Xenon – 135 Samarium – 149
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Reactor Power Control Reactor power is controlled and adjusted by careful management of: Neutron flux Reactivity coefficients Control rods Boron concentration (PWR)
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Enrichment Natural Uranium = 0.7 % 235U
Slightly enriched = 0.8 % to 3 % 235U Low enriched = 3 % to 5 % 235U
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Magnox
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AGR
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PWR
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BWR
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RBMK
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CANDU
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