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Stationary states in a potential well
Haret Codratian Rosu
JOSE LUIS MORAN LOPEZ
Acceso Abierto
Atribución-NoComercial-SinDerivadas
Stationary states
Bohr’s atomic model
Schrödinger equation
Rutherford’s planetary model
Frank-Hertz experiment
Infinite square well potential
Quantum harmonic oscillator
Wilson-Sommerfeld theory
Hydrogen atom
"In the early days of the 20th century a set of important observations in atomic and molecular physics could not be explained on the basis of the laws of classical physics. One of the main findings was the emission of light by excited atoms with very particular frequencies. To explain those findings a new development in physics was necessary, now known as quantum mechanics. In particular, the concept of stationary states was introduced by Niels Bohr, in 1913, in order to explain those observations and the stability of atoms. According to E.C. Kemble (1929), the existence of discrete atomic and molecular energy levels brought into mechanics a new kind of atomicity superposed on the atomicity of electrons and protons. We review here in a historical context the topic of stationary states in the quantum world, including the generalization to the primary ideas. We also discuss the stationary states in one dimensional parabolic wells and the three dimensional Coulomb and parabolic cases."
UNESCO
2007
Capítulo de libro
H.C. Rosu and J.L. Morán-López, Stationary states in a potential well, Encyclopedia of Life Support Systems. 2007, Developed under the auspicies of the UNESCO, EOLSS Publishing, Oxford, UK (http://www.eolss.net)
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Aparece en las colecciones: Publicaciones Científicas Nanociencias y Materiales

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