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  2. Arthur Erich Haas - Wikipedia

    en.wikipedia.org/wiki/Arthur_Erich_Haas

    Arthur Erich Haas (April 30, 1884, in Brno – February 20, 1941, in Chicago) was an Austrian physicist, noted for a 1910 paper [1] he submitted in support of his habilitation as Privatdocent at the University of Vienna that outlined a treatment of the hydrogen atom involving quantization of electronic orbitals, thus anticipating the Bohr model (1913) by three years.

  3. Bohr–Sommerfeld model - Wikipedia

    en.wikipedia.org/wiki/Bohr–Sommerfeld_model

    This allowed the orbits of the electron to be ellipses instead of circles, and introduced the concept of quantum degeneracy. The theory would have correctly explained the Zeeman effect, except for the issue of electron spin. Sommerfeld's model was much closer to the modern quantum mechanical picture than Bohr's.

  4. Atomic physics - Wikipedia

    en.wikipedia.org/wiki/Atomic_physics

    The total energy of an electron in the nth orbit is: E_n = -\frac{13.6}{n^2} \ \text{eV}, where 13.6 \ \text{eV} is the ground-state energy of the hydrogen atom. 4.Emission or Absorption of Energy: •Electrons can transition between orbits by absorbing or emitting energy equal to the difference between the energy levels: \Delta E = E_f - E_i ...

  5. Free electron model - Wikipedia

    en.wikipedia.org/wiki/Free_electron_model

    In solid-state physics, the free electron model is a quantum mechanical model for the behaviour of charge carriers in a metallic solid. It was developed in 1927, [1] principally by Arnold Sommerfeld, who combined the classical Drude model with quantum mechanical Fermi–Dirac statistics and hence it is also known as the Drude–Sommerfeld model.

  6. Sommerfeld expansion - Wikipedia

    en.wikipedia.org/wiki/Sommerfeld_expansion

    Integrals of this type appear frequently when calculating electronic properties, like the heat capacity, in the free electron model of solids. In these calculations the above integral expresses the expected value of the quantity H ( ε ) {\displaystyle H(\varepsilon )} .

  7. Delta potential - Wikipedia

    en.wikipedia.org/wiki/Delta_potential

    The delta potential is the potential = (), where δ(x) is the Dirac delta function. It is called a delta potential well if λ is negative, and a delta potential barrier if λ is positive. The delta has been defined to occur at the origin for simplicity; a shift in the delta function's argument does not change any of the following results.

  8. Delta ray - Wikipedia

    en.wikipedia.org/wiki/Delta_ray

    A delta ray is a secondary electron with enough energy to escape a significant distance away from the primary radiation beam and produce further ionization. [ 1 ] : 25 The term is sometimes used to describe any recoil particle caused by secondary ionization .

  9. Thomas–Fermi model - Wikipedia

    en.wikipedia.org/wiki/Thomas–Fermi_model

    Thomas–Fermi model Orbital-free density functional theory Linearized augmented-plane-wave method Projector augmented wave method: Electronic band structure; Nearly free electron model Tight binding Muffin-tin approximation k·p perturbation theory Empty lattice approximation GW approximation Korringa–Kohn–Rostoker method