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  2. Parity (physics) - Wikipedia

    en.wikipedia.org/wiki/Parity_(physics)

    For example, the isotopes of oxygen include 17 O(5/2+), meaning that the spin is 5/2 and the parity is even. The shell model explains this because the first 16 nucleons are paired so that each pair has spin zero and even parity, and the last nucleon is in the 1d 5/2 shell, which has even parity since ℓ = 2 for a d orbital. [10]

  3. Nuclear shell model - Wikipedia

    en.wikipedia.org/wiki/Nuclear_shell_model

    Therefore, a nucleus with an even number of protons and an even number of neutrons has 0 spin and positive parity. A nucleus with an even number of protons and an odd number of neutrons (or vice versa) has the parity of the last neutron (or proton), and the spin equal to the total angular momentum of this neutron (or proton).

  4. Spin–orbit interaction - Wikipedia

    en.wikipedia.org/wiki/Spin–orbit_interaction

    The spin magnetic moment of the electron is =, where is the spin (or intrinsic angular-momentum) vector, is the Bohr magneton, and = is the electron-spin g-factor. Here μ {\displaystyle {\boldsymbol {\mu }}} is a negative constant multiplied by the spin , so the spin magnetic moment is antiparallel to the spin.

  5. Decay scheme - Wikipedia

    en.wikipedia.org/wiki/Decay_scheme

    The decay scheme of a radioactive substance is a graphical presentation of all the transitions occurring in a decay, and of their relationships. Examples are shown below. It is useful to think of the decay scheme as placed in a coordinate system, where the vertical axis is energy, increasing from bottom to top, and the horizontal axis is the proton number, increasing from left to right.

  6. Beta decay transition - Wikipedia

    en.wikipedia.org/wiki/Beta_decay_transition

    The Gamow–Teller transition is a pseudovector transition, that is, the selection rules for beta decay caused by such a transition involve no parity change of the nuclear state. [2] The spin of the parent nucleus can either remain unchanged or change by ±1. However, unlike the Fermi transition, transitions from spin 0 to spin 0 are excluded.

  7. Spin (physics) - Wikipedia

    en.wikipedia.org/wiki/Spin_(physics)

    The conventional definition of the spin quantum number is s = ⁠ n / 2 ⁠, where n can be any non-negative integer. Hence the allowed values of s are 0, ⁠ 1 / 2 ⁠, 1, ⁠ 3 / 2 ⁠, 2, etc. The value of s for an elementary particle depends only on the type of particle and cannot be altered in any known way (in contrast to the spin ...

  8. J-coupling - Wikipedia

    en.wikipedia.org/wiki/J-coupling

    In nuclear chemistry and nuclear physics, J-couplings (also called spin-spin coupling or indirect dipole–dipole coupling) are mediated through chemical bonds connecting two spins. It is an indirect interaction between two nuclear spins that arises from hyperfine interactions between the nuclei and local electrons. [ 1 ]

  9. Pauli matrices - Wikipedia

    en.wikipedia.org/wiki/Pauli_matrices

    That is, the resulting spin operators for higher spin systems in three spatial dimensions, for arbitrarily large j, can be calculated using this spin operator and ladder operators. They can be found in Rotation group SO(3) § A note on Lie algebras. The analog formula to the above generalization of Euler's formula for Pauli matrices, the group ...

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