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  2. Energy level - Wikipedia

    en.wikipedia.org/wiki/Energy_level

    An increase in energy level from E 1 to E 2 resulting from absorption of a photon represented by the red squiggly arrow, and whose energy is h ν. A decrease in energy level from E 2 to E 1 resulting in emission of a photon represented by the red squiggly arrow, and whose energy is h ν.

  3. File:Electron energy.pdf - Wikipedia

    en.wikipedia.org/wiki/File:Electron_energy.pdf

    You are free: to share – to copy, distribute and transmit the work; to remix – to adapt the work; Under the following conditions: attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses ...

  4. Jaynes–Cummings model - Wikipedia

    en.wikipedia.org/wiki/Jaynes–Cummings_model

    To realize the dynamics predicted by the Jaynes–Cummings model experimentally requires a quantum mechanical resonator with a very high quality factor so that the transitions between the states in the two-level system (typically two energy sub-levels in an atom) are coupled very strongly by the interaction of the atom with the field mode. This ...

  5. Aufbau principle - Wikipedia

    en.wikipedia.org/wiki/Aufbau_principle

    In this way, the electrons of an atom or ion form the most stable electron configuration possible. An example is the configuration 1s 2 2s 2 2p 6 3s 2 3p 3 for the phosphorus atom, meaning that the 1s subshell has 2 electrons, the 2s subshell has 2 electrons, the 2p subshell has 6 electrons, and so on.

  6. Principal quantum number - Wikipedia

    en.wikipedia.org/wiki/Principal_quantum_number

    In a simplistic one-electron model described below, the total energy of an electron is a negative inverse quadratic function of the principal quantum number n, leading to degenerate energy levels for each n > 1. [1] In more complex systems—those having forces other than the nucleus–electron Coulomb force—these levels split.

  7. Subatomic particle - Wikipedia

    en.wikipedia.org/wiki/Subatomic_particle

    The negatively charged electron has a mass of about ⁠ 1 / 1836 ⁠ of that of a hydrogen atom. The remainder of the hydrogen atom's mass comes from the positively charged proton. The atomic number of an element is the number of protons in its nucleus. Neutrons are neutral particles having a mass slightly greater than that of the proton.

  8. Hund's rules - Wikipedia

    en.wikipedia.org/wiki/Hund's_rules

    For sulfur (S) the lowest energy term is again with spin–orbit levels =,,, but now there are four of six possible electrons in the shell so the ground state is . If the shell is half-filled then L = 0 {\displaystyle L=0\,} , and hence there is only one value of J {\displaystyle J\,} (equal to S {\displaystyle S\,} ), which is the lowest ...

  9. Bohr–Sommerfeld model - Wikipedia

    en.wikipedia.org/wiki/Bohr–Sommerfeld_model

    This was a significant step in the development of quantum mechanics. It also described the possibility of atomic energy levels being split by a magnetic field (called the Zeeman effect). Walther Kossel worked with Bohr and Sommerfeld on the Bohr–Sommerfeld model of the atom introducing two electrons in the first shell and eight in the second. [8]