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  2. Energy level - Wikipedia

    en.wikipedia.org/wiki/Energy_level

    An equivalent formula can be derived quantum mechanically from the time-independent Schrödinger equation with a kinetic energy Hamiltonian operator using a wave function as an eigenfunction to obtain the energy levels as eigenvalues, but the Rydberg constant would be replaced by other fundamental physics constants.

  3. Bohr model - Wikipedia

    en.wikipedia.org/wiki/Bohr_model

    The energy level spacing between circular orbits can be calculated with the correspondence formula. For a hydrogen atom, the classical orbits have a period T determined by Kepler's third law to scale as r 3/2. The energy scales as 1/r, so the energy level spacing formula obeys to:

  4. Degenerate energy levels - Wikipedia

    en.wikipedia.org/wiki/Degenerate_energy_levels

    Degenerate energy levels. In quantum mechanics, an energy level is degenerate if it corresponds to two or more different measurable states of a quantum system. Conversely, two or more different states of a quantum mechanical system are said to be degenerate if they give the same value of energy upon measurement.

  5. Ground state - Wikipedia

    en.wikipedia.org/wiki/Ground_state

    Energy levels for an electron in an atom: ground state and excited states. After absorbing energy, an electron may jump from the ground state to a higher-energy excited state. The ground state of a quantum-mechanical system is its stationary state of lowest energy; the energy of the ground state is known as the zero-point energy of the system.

  6. Rydberg state - Wikipedia

    en.wikipedia.org/wiki/Rydberg_state

    Rydberg state. The Rydberg states[1] of an atom or molecule are electronically excited states with energies that follow the Rydberg formula as they converge on an ionic state with an ionization energy. Although the Rydberg formula was developed to describe atomic energy levels, it has been used to describe many other systems that have ...

  7. Fermi energy - Wikipedia

    en.wikipedia.org/wiki/Fermi_energy

    The Fermi energy is an important concept in the solid state physics of metals and superconductors. It is also a very important quantity in the physics of quantum liquids like low temperature helium (both normal and superfluid 3 He), and it is quite important to nuclear physics and to understanding the stability of white dwarf stars against ...

  8. Landau levels - Wikipedia

    en.wikipedia.org/wiki/Landau_levels

    The effects of Landau levels may only be observed when the mean thermal energy kT is smaller than the energy level separation, kT ≪ ħω c, meaning low temperatures and strong magnetic fields. Each Landau level is degenerate because of the second quantum number k y , which can take the values k y = 2 π N L y , {\displaystyle k_{y}={\frac {2 ...

  9. Finite potential well - Wikipedia

    en.wikipedia.org/wiki/Finite_potential_well

    The energy levels = / are determined once is solved as a root of the following transcendental equation = ⁡ ⁡ where =,,, … Existence of root to above equation is not always guaranteed, for example, one can always find a value of so small, that for given values of and , there exists no discrete energy level.

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