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    • https://phys.libretexts.org/Bookshelves/Quantum_Mechanics/Essential_Graduate_Physics_-_Quantum_Mechanics_(Likharev)/06%3A_Perturbative_Approaches/6.04%3A_The_Zeeman_Effect
      5.7) it has at most two non-vanishing terms, with the Clebsh-Gordan coefficients (5.190): \[\begin{aligned} &\left|j=l \pm 1 / 2, m_{j}\right\rangle \\ &=\pm\left(\frac{l \pm m_{j}+1 / 2}{2 l+1}\right...5.7) it has at most two non-vanishing terms, with the Clebsh-Gordan coefficients (5.190): |j=l±1/2,mj=±(l±mj+1/22l+1)1/2|ml=mj1/2,ms=+1/2+(lmj+1/22l+1)1/2|ml=mj+1/2,ms=1/2. Taking into account that the operator ˆSz gives non-zero brackets only for ms=ms, the \…
    • https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Stellar_Atmospheres_(Tatum)/07%3A_Atomic_Spectroscopy/7.22%3A_Paschen-Back_Effect
      Rather, the g-factor is the ratio of the sum of the components of the orbital and spin magnetic moments in the direction of B to the sum of the components of the orbital and spin angu...Rather, the g-factor is the ratio of the sum of the components of the orbital and spin magnetic moments in the direction of B to the sum of the components of the orbital and spin angular momenta in that direction.

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