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  2. Nuclear binding energy - Wikipedia

    en.wikipedia.org/wiki/Nuclear_binding_energy

    Energy is released in the Sun when 4 protons combine into a helium nucleus, a process in which two of them are also converted to neutrons. [11] The conversion of protons to neutrons is the result of another nuclear force, known as the weak (nuclear) force. The weak force, like the strong force, has a short range, but is much weaker than the ...

  3. Neutron transport - Wikipedia

    en.wikipedia.org/wiki/Neutron_transport

    The number of neutrons produced per fission is multiplicatively modified by the dominant eigenvalue. The resulting value of this eigenvalue reflects the time dependence of the neutron density in a multiplying medium. k eff < 1, subcritical: the neutron density is decreasing as time passes; k eff = 1, critical: the neutron density remains ...

  4. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    A fast neutron is a free neutron with a kinetic energy level close to 1 MeV (1.6 × 10 −13 J), hence a speed of ~ 14 000 km/s (~ 5% of the speed of light). They are named fission energy or fast neutrons to distinguish

  5. Neutron imaging - Wikipedia

    en.wikipedia.org/wiki/Neutron_imaging

    For lower energy neutrons, a cold moderator such as liquid deuterium, can be used to produce low energy neutrons (cold neutron). If no or less moderator is present, high energy neutrons (termed fast neutrons), can be produced. The higher the temperature of the moderator, the higher the resulting kinetic energy of the neutrons is and the faster ...

  6. Neutron temperature - Wikipedia

    en.wikipedia.org/wiki/Neutron_temperature

    A fast neutron is a free neutron with a kinetic energy level close to 1 M eV (100 T J/kg), hence a speed of 14,000 km/s or higher. They are named fast neutrons to distinguish them from lower-energy thermal neutrons, and high-energy neutrons produced in cosmic showers or accelerators. Fast neutrons are produced by nuclear processes:

  7. Neutron radiation - Wikipedia

    en.wikipedia.org/wiki/Neutron_radiation

    e. Neutron radiation is a form of ionizing radiation that presents as free neutrons. Typical phenomena are nuclear fission or nuclear fusion causing the release of free neutrons, which then react with nuclei of other atoms to form new nuclides —which, in turn, may trigger further neutron radiation. Free neutrons are unstable, decaying into a ...

  8. Nuclear chain reaction - Wikipedia

    en.wikipedia.org/wiki/Nuclear_chain_reaction

    A possible nuclear fission chain reaction: 1) A uranium-235 atom absorbs a neutron and fissions into two fission fragments, releasing three new neutrons and a large amount of binding energy. 2) One of those neutrons is absorbed by an atom of uranium-238, and does not continue the reaction. Another neutron leaves the system without being absorbed.

  9. Beta decay - Wikipedia

    en.wikipedia.org/wiki/Beta_decay

    The two types of beta decay are known as beta minus and beta plus.In beta minus (β −) decay, a neutron is converted to a proton, and the process creates an electron and an electron antineutrino; while in beta plus (β +) decay, a proton is converted to a neutron and the process creates a positron and an electron neutrino. β + decay is also known as positron emission.