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  2. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    Photodisintegration (also called phototransmutation, or a photonuclear reaction) is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, enters an excited state, and immediately decays by emitting a subatomic particle.

  3. Neutron scattering - Wikipedia

    en.wikipedia.org/wiki/Neutron_scattering

    Neutron scattering, the irregular dispersal of free neutrons by matter, can refer to either the naturally occurring physical process itself or to the man-made experimental techniques that use the natural process for investigating materials. The natural/physical phenomenon is of elemental importance in nuclear engineering and

  4. Neutron diffraction - Wikipedia

    en.wikipedia.org/wiki/Neutron_diffraction

    Neutron diffraction or elastic neutron scattering is the application of neutron scattering to the determination of the atomic and/or magnetic structure of a material. A sample to be examined is placed in a beam of thermal or cold neutrons to obtain a diffraction pattern that provides information of the structure of the material.

  5. Neutron spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Neutron_spectroscopy

    This allows the total spin of the unpaired electrons and neutron to be probed. The magnetic scattering length from one electron is b m = 𝛾r 0 = 1.348 fm which is on the same order of magnitude as the nuclear scattering length. Because of the dipole-dipole character of the interaction, the scattering is considered to be anisotropic. [7]

  6. Neutron capture - Wikipedia

    en.wikipedia.org/wiki/Neutron_capture

    In this process, the mass number increases by one. This is written as a formula in the form 197 Au + n → 198 Au + γ, or in short form 197 Au(n,γ) 198 Au. If thermal neutrons are used, the process is called thermal capture. The isotope 198 Au is a beta emitter that decays into the mercury isotope 198 Hg. In this process, the atomic number ...

  7. Neutron flux - Wikipedia

    en.wikipedia.org/wiki/Neutron_flux

    Neutron flux in asymptotic giant branch stars and in supernovae is responsible for most of the natural nucleosynthesis producing elements heavier than iron.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).

  8. Neutron transport - Wikipedia

    en.wikipedia.org/wiki/Neutron_transport

    Nuclear scientists and engineers often need to know where neutrons are in an apparatus, in what direction they are going, and how quickly they are moving. It is commonly used to determine the behavior of nuclear reactor cores and experimental or industrial neutron beams. Neutron transport is a type of radiative transport.

  9. Nuclear reaction - Wikipedia

    en.wikipedia.org/wiki/Nuclear_reaction

    Thus, a nuclear reaction must cause a transformation of at least one nuclide to another. If a nucleus interacts with another nucleus or particle, they then separate without changing the nature of any nuclide, the process is simply referred to as a type of nuclear scattering, rather than a nuclear reaction.