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  2. Neutron–proton ratio - Wikipedia

    en.wikipedia.org/wiki/Neutron–proton_ratio

    For many elements with atomic number Z small enough to occupy only the first three nuclear shells, that is up to that of calcium (Z = 20), there exists a stable isotope with N/Z ratio of one. The exceptions are beryllium ( N / Z = 1.25) and every element with odd atomic number between 9 and 19 inclusive (though in those cases N = Z + 1 always ...

  3. Six factor formula - Wikipedia

    en.wikipedia.org/wiki/Six_factor_formula

    The symbols are defined as: [2], and are the average number of neutrons produced per fission in the medium (2.43 for uranium-235). and are the microscopic fission and absorption cross sections for fuel, respectively.

  4. Neutron cross section - Wikipedia

    en.wikipedia.org/wiki/Neutron_cross_section

    In nuclear physics, the concept of a neutron cross section is used to express the likelihood of interaction between an incident neutron and a target nucleus. The neutron cross section σ can be defined as the area in cm 2 for which the number of neutron-nuclei reactions taking place is equal to the product of the number of incident neutrons that would pass through the area and the number of ...

  5. 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).

  6. Shape of the atomic nucleus - Wikipedia

    en.wikipedia.org/wiki/Shape_of_the_atomic_nucleus

    If the nucleus is assumed to be spherically symmetric, an approximate relationship between nuclear radius and mass number arises above A=40 from the formula R=R o A 1/3 with R o = 1.2 ± 0.2 fm. [6] R is the predicted spherical nuclear radius, A is the mass number, and R o is a constant determined by experimental

  7. Delayed neutron - Wikipedia

    en.wikipedia.org/wiki/Delayed_neutron

    These fragments emit, on average, two or three free neutrons (in average 2.47), called "prompt" neutrons. A subsequent fission fragment occasionally undergoes a stage of radioactive decay (which is a beta minus decay ) that yields a new nucleus (the emitter nucleus) in an excited state that emits an additional neutron, called a "delayed ...

  8. Strong interaction - Wikipedia

    en.wikipedia.org/wiki/Strong_interaction

    On a scale less than about 0.8 fm (roughly the radius of a nucleon), the force is carried by gluons and holds quarks together to form protons, neutrons, and other hadrons. On a larger scale, up to about 3 fm, the force is carried by mesons and binds nucleons (protons and neutrons) together to form the nucleus of an atom. [2]

  9. Neutron number - Wikipedia

    en.wikipedia.org/wiki/Neutron_number

    The neutron number (symbol N) is the number of neutrons in a nuclide. Atomic number (proton number) plus neutron number equals mass number : Z + N = A . The difference between the neutron number and the atomic number is known as the neutron excess: D = N − Z = A − 2 Z .