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  2. Spin–orbit interaction - Wikipedia

    en.wikipedia.org/wiki/Spinorbit_interaction

    For rare-earth ions the spinorbit interactions are much stronger than the crystal electric field (CEF) interactions. [9] The strong spinorbit 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. 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 ...

  4. Angular momentum coupling - Wikipedia

    en.wikipedia.org/wiki/Angular_momentum_coupling

    In atomic physics, spinorbit coupling, also known as spin-pairing, describes a weak magnetic interaction, or coupling, of the particle spin and the orbital motion of this particle, e.g. the electron spin and its motion around an atomic nucleus. One of its effects is to separate the energy of internal states of the atom, e.g. spin-aligned and ...

  5. Landé interval rule - Wikipedia

    en.wikipedia.org/wiki/Landé_interval_rule

    In atomic physics, the Landé interval rule [1] states that, due to weak angular momentum coupling (either spin-orbit or spin-spin coupling), the energy splitting between successive sub-levels are proportional to the total angular momentum quantum number (J or F) of the sub-level with the larger of their total angular momentum value (J or F).

  6. Hund's rules - Wikipedia

    en.wikipedia.org/wiki/Hund's_rules

    These rules specify in a simple way how usual energy interactions determine which term includes the ground state. The rules assume that the repulsion between the outer electrons is much greater than the spinorbit interaction, which is in turn stronger than any other remaining interactions. This is referred to as the LS coupling regime.

  7. Zeeman effect - Wikipedia

    en.wikipedia.org/wiki/Zeeman_effect

    Note in particular that the size of the energy splitting is different for the different orbitals, because the g J values are different. On the left, fine structure splitting is depicted. This splitting occurs even in the absence of a magnetic field, as it is due to spinorbit coupling.

  8. 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]

  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 spinorbit 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 ...