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  2. Perturbation theory (quantum mechanics) - Wikipedia

    en.wikipedia.org/wiki/Perturbation_theory...

    The first-order energy shift is not well defined, since there is no unique way to choose a basis of eigenstates for the unperturbed system. The various eigenstates for a given energy will perturb with different energies, or may well possess no continuous family of perturbations at all.

  3. Isotopic shift - Wikipedia

    en.wikipedia.org/wiki/Isotopic_shift

    Using perturbation theory, the first-order energy shift can be calculated as = >, which requires the knowledge of accurate many-electron wave function. Due to the 1 / M N {\displaystyle 1/M_{N}} term in the expression, the specific mass shift also decrease as 1 / M N 2 {\displaystyle 1/M_{N}^{2}} as mass of nucleus increase, same as normal mass ...

  4. Stark effect - Wikipedia

    en.wikipedia.org/wiki/Stark_effect

    If g = 1 (as is often the case for electronic states of molecules) the first-order energy becomes proportional to the expectation (average) value of the dipole operator , = | | = . Because the electric dipole moment is a vector ( tensor of the first rank), the diagonal elements of the perturbation matrix V int vanish between states that have a ...

  5. Zeeman effect - Wikipedia

    en.wikipedia.org/wiki/Zeeman_effect

    More precisely, if , each of these three components is actually a group of several transitions due to the residual spin–orbit coupling and relativistic corrections (which are of the same order, known as 'fine structure'). The first-order perturbation theory with these corrections yields the following formula for the hydrogen atom in the ...

  6. Fine structure - Wikipedia

    en.wikipedia.org/wiki/Fine_structure

    For example, it gives the 2s orbital the same energy as the 2p orbital by raising the 2s state by 9.057 × 10 −5 eV. The Darwin term changes potential energy of the electron. It can be interpreted as a smearing out of the electrostatic interaction between the electron and nucleus due to zitterbewegung , or rapid quantum oscillations, of the ...

  7. Isomeric shift - Wikipedia

    en.wikipedia.org/wiki/Isomeric_shift

    The isomeric shift on atomic spectral lines is the energy or frequency shift in atomic spectra, which occurs when one replaces one nuclear isomer by another. The effect was predicted by Richard M. Weiner [ 2 ] in 1956, whose calculations showed that it should be measurable by atomic (optical) spectroscopy (see also [ 3 ] ).

  8. Degenerate energy levels - Wikipedia

    en.wikipedia.org/wiki/Degenerate_energy_levels

    Degenerate states are also obtained when the sum of squares of quantum numbers corresponding to different energy levels are the same. For example, the three states (n x = 7, n y = 1), (n x = 1, n y = 7) and (n x = n y = 5) all have = and constitute a degenerate set.

  9. Shoolery's rule - Wikipedia

    en.wikipedia.org/wiki/Shoolery's_rule

    We can calculate shift of the CH 2 protons in a A–CH 2 –B structure using the formula δ = 0.23 p p m + S A + S B {\displaystyle \delta =0.23\,\mathrm {ppm} +S_{\mathrm {A} }+S_{\mathrm {B} }} where 0.23 ppm is the chemical shift of methane and the empirical adjustments S are based on the identities of the A and B groups:

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