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  2. Spin–orbit interaction - Wikipedia

    en.wikipedia.org/wiki/Spin–orbit_interaction

    For rare-earth ions the spin–orbit interactions are much stronger than the crystal electric field (CEF) interactions. [9] The strong spin–orbit coupling makes J a relatively good quantum number, because the first excited multiplet is at least ~130 meV (1500 K) above the primary multiplet. The result is that filling it at room temperature ...

  3. Dresselhaus effect - Wikipedia

    en.wikipedia.org/wiki/Dresselhaus_effect

    Spin–orbit interaction is a relativistic coupling between the electric field produced by an ion-core and the resulting dipole moment arising from the relative motion of the electron, and its intrinsic magnetic dipole proportional to the electron spin. In an atom, the coupling weakly splits an orbital energy state into two states: one state ...

  4. Rashba effect - Wikipedia

    en.wikipedia.org/wiki/Rashba_effect

    The Rashba spin-orbit coupling is typical for systems with uniaxial symmetry, e.g., for hexagonal crystals of CdS and CdSe for which it was originally found [20] and perovskites, and also for heterostructures where it develops as a result of a symmetry breaking field in the direction perpendicular to the 2D surface. [2]

  5. Angular momentum coupling - Wikipedia

    en.wikipedia.org/wiki/Angular_momentum_coupling

    In quantum mechanics, coupling also exists between angular momenta belonging to different Hilbert spaces of a single object, e.g. its spin and its orbital angular momentum. If the spin has half-integer values, such as ⁠ 1 / 2 ⁠ for an electron, then the total (orbital plus spin) angular momentum will also be restricted to half-integer values.

  6. Intersystem crossing - Wikipedia

    en.wikipedia.org/wiki/Intersystem_crossing

    As the spin/orbital interactions in such molecules are substantial and a change in spin is thus more favourable, intersystem crossing is most common in heavy-atom molecules (e.g. those containing iodine or bromine). This process is called "spin-orbit coupling". Simply-stated, it involves coupling of the electron spin with the orbital angular ...

  7. Zeeman effect - Wikipedia

    en.wikipedia.org/wiki/Zeeman_effect

    The Paschen–Back effect is the splitting of atomic energy levels in the presence of a strong magnetic field. This occurs when an external magnetic field is sufficiently strong to disrupt the coupling between orbital and spin angular momenta. This effect is the strong-field limit of the Zeeman effect.

  8. Rashba–Edelstein effect - Wikipedia

    en.wikipedia.org/wiki/Rashba–Edelstein_effect

    For what concerns the Rashba–Edelstein effect, the spin-split dispersion relation consists in two bands displaced along the k-axis due to a structural inversion asymmetry (SIA), accordingly to the Rashba effect (i.e., these bands show a linear splitting in k due to the spin-orbit coupling [10] [16]).

  9. Magnetochemistry - Wikipedia

    en.wikipedia.org/wiki/Magnetochemistry

    The small deviations from the spin-only formula may result from the neglect of orbital angular momentum or of spin–orbit coupling. For example, tetrahedral d 3 , d 4 , d 8 and d 9 complexes tend to show larger deviations from the spin-only formula than octahedral complexes of the same ion, because "quenching" of the orbital contribution is ...