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  2. Energy level - Wikipedia

    en.wikipedia.org/wiki/Energy_level

    In a very general way, energy level differences between electronic states are larger, differences between vibrational levels are intermediate, and differences between rotational levels are smaller, although there can be overlap. Translational energy levels are practically continuous and can be calculated as kinetic energy using classical mechanics.

  3. Hyperfine structure - Wikipedia

    en.wikipedia.org/wiki/Hyperfine_structure

    The term transition frequency denotes the frequency of radiation corresponding to the transition between the two hyperfine levels of the atom, and is equal to f = ΔE/h, where ΔE is difference in energy between the levels and h is the Planck constant.

  4. Particle in a box - Wikipedia

    en.wikipedia.org/wiki/Particle_in_a_box

    The energy difference between two energy levels, n f and n i is: = () The difference between the ground state energy, n, and the first excited state, n+1, corresponds to the energy required to excite the system.

  5. Bohr model - Wikipedia

    en.wikipedia.org/wiki/Bohr_model

    For the hydrogen atom Bohr starts with his derived formula for the energy released as a free electron moves into a stable circular orbit indexed by : [28] = The energy difference between two such levels is then: = = Therefore, Bohr's theory gives the Rydberg formula and moreover the numerical value the Rydberg constant for hydrogen in terms of ...

  6. Rabi frequency - Wikipedia

    en.wikipedia.org/wiki/Rabi_frequency

    Population transfer between the levels of such a 2-level system illuminated with light exactly resonant with the difference in energy between the two levels will occur at the Rabi frequency; when the incident light is detuned from this energy difference (detuned from resonance) then the population transfer occurs at the generalized Rabi frequency.

  7. Hydrogen spectral series - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_spectral_series

    The energy of an emitted photon corresponds to the energy difference between the two states. Because the energy of each state is fixed, the energy difference between them is fixed, and the transition will always produce a photon with the same energy. The spectral lines are grouped into series according to n′. Lines are named sequentially ...

  8. Energy level splitting - Wikipedia

    en.wikipedia.org/wiki/Energy_level_splitting

    In quantum physics, energy level splitting or a split in an energy level of a quantum system occurs when a perturbation changes the system. The perturbation changes the corresponding Hamiltonian and the outcome is change in eigenvalues ; several distinct energy levels emerge in place of the former degenerate (multi- state ) level.

  9. Schottky anomaly - Wikipedia

    en.wikipedia.org/wiki/Schottky_anomaly

    Schottky anomalous heat capacity for a two-level system. is the absolute temperature, is the Boltzmann constant and is the energy difference between the levels. The Schottky anomaly is an effect observed in solid-state physics where the specific heat capacity of a solid at low temperature has a peak.