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  2. Bohr model - Wikipedia

    en.wikipedia.org/wiki/Bohr_model

    The Bohr model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). [1]

  3. Bohr–Sommerfeld model - Wikipedia

    en.wikipedia.org/wiki/Bohr–Sommerfeld_model

    The Bohr–Sommerfeld model (also known as the Sommerfeld model or Bohr–Sommerfeld theory) was an extension of the Bohr model to allow elliptical orbits of electrons around an atomic nucleus. Bohr–Sommerfeld theory is named after Danish physicist Niels Bohr and German physicist Arnold Sommerfeld .

  4. Atomic electron transition - Wikipedia

    en.wikipedia.org/wiki/Atomic_electron_transition

    An electron in a Bohr model atom, moving from quantum level n = 3 to n = 2 and releasing a photon.The energy of an electron is determined by its orbit around the atom, The n = 0 orbit, commonly referred to as the ground state, has the lowest energy of all states in the system.

  5. Electron shell - Wikipedia

    en.wikipedia.org/wiki/Electron_shell

    In 1913, Niels Bohr proposed a model of the atom, giving the arrangement of electrons in their sequential orbits. At that time, Bohr allowed the capacity of the inner orbit of the atom to increase to eight electrons as the atoms got larger, and "in the scheme given below the number of electrons in this [outer] ring is arbitrary put equal to the normal valency of the corresponding element".

  6. Principal quantum number - Wikipedia

    en.wikipedia.org/wiki/Principal_quantum_number

    Schrödinger's equation developed the idea from a flat two-dimensional Bohr atom to the three-dimensional wavefunction model. In the Bohr model, the allowed orbits were derived from quantized (discrete) values of orbital angular momentum, L according to the equation = = where n = 1, 2, 3, ... and is called the principal quantum number, and h is ...

  7. Lyman series - Wikipedia

    en.wikipedia.org/wiki/Lyman_series

    In 1914, when Niels Bohr produced his Bohr model theory, the reason why hydrogen spectral lines fit Rydberg's formula was explained. Bohr found that the electron bound to the hydrogen atom must have quantized energy levels described by the following formula,

  8. Bohr radius - Wikipedia

    en.wikipedia.org/wiki/Bohr_radius

    Since the reduced mass of the electron–proton system is a little bit smaller than the electron mass, the "reduced" Bohr radius is slightly larger than the Bohr radius (meters). This result can be generalized to other systems, such as positronium (an electron orbiting a positron ) and muonium (an electron orbiting an anti-muon ) by using the ...

  9. Energy level - Wikipedia

    en.wikipedia.org/wiki/Energy_level

    This equation is obtained from combining the Rydberg formula for any hydrogen-like element (shown below) with E = hν = hc / λ assuming that the principal quantum number n above = n 1 in the Rydberg formula and n 2 = ∞ (principal quantum number of the energy level the electron descends from, when emitting a photon).