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  2. Discrete ordinates method - Wikipedia

    en.wikipedia.org/wiki/Discrete_Ordinates_Method

    The intensity field can in principle be solved from the integrodifferential radiative transfer equation (RTE), but an exact solution is usually impossible and even in the case of geometrically simple systems can contain unusual special functions such as the Chandrasekhar's H-function and Chandrasekhar's X- and Y-functions. [3]

  3. Neutron transport - Wikipedia

    en.wikipedia.org/wiki/Neutron_transport

    A fixed source calculation involves imposing a known neutron source on a medium and determining the resulting neutron distribution throughout the problem. This type of problem is particularly useful for shielding calculations, where a designer would like to minimize the neutron dose outside of a shield while using the least amount of shielding ...

  4. List of equations in nuclear and particle physics - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    2 Equations. Toggle Equations subsection. ... m n = neutron rest mass ... University Physics – With Modern Physics (12th ed.). Addison-Wesley (Pearson International).

  5. Shielding effect - Wikipedia

    en.wikipedia.org/wiki/Shielding_effect

    Additionally, there is also a shielding effect that occurs between sublevels within the same principal energy level. An electron in the s-sublevel is capable of shielding electrons in the p-sublevel of the same principal energy level. The size of the shielding effect is difficult to calculate precisely due to effects from quantum mechanics.

  6. Geometric and material buckling - Wikipedia

    en.wikipedia.org/wiki/Geometric_and_Material...

    Geometric buckling is a measure of neutron leakage and material buckling is a measure of the difference between neutron production and neutron absorption. [1] When nuclear fission occurs inside of a nuclear reactor, neutrons are produced. [1] These neutrons then, to state it simply, either react with the fuel in the reactor or escape from the ...

  7. Neutron flux - Wikipedia

    en.wikipedia.org/wiki/Neutron_flux

    In stars there is a relatively low neutron flux on the order of 10 5 to 10 11 cm −2 s −1, resulting in nucleosynthesis by the s-process (slow neutron-capture process). By contrast, after a core-collapse supernova, there is an extremely high neutron flux, on the order of 10 32 cm −2 s −1 , [ 4 ] resulting in nucleosynthesis by the r ...

  8. Skyshine - Wikipedia

    en.wikipedia.org/wiki/Skyshine

    Regardless of whether the upward incident beam is shaped like a circle, square or rectangle, specific calculation formalism has been described. [ 5 ] [ 6 ] The intensity of radiation measured at the surface immediately surrounding the facility increases with growing distance from the shielding barrier to reach a maximum and then fall again ...

  9. Effective nuclear charge - Wikipedia

    en.wikipedia.org/wiki/Effective_nuclear_charge

    In atomic physics, the effective nuclear charge of an electron in a multi-electron atom or ion is the number of elementary charges an electron experiences by the nucleus. It is denoted by Z eff . The term "effective" is used because the shielding effect of negatively charged electrons prevent higher energy electrons from experiencing the full ...

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