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Abstract

The Schrödinger equation is based on the classical relationship between the total energy E, the kinetic energy \(T = \frac{{{p^2}}}{{2\mu }}\) and the potential energy V, T + V = E, of a particle of mass μ and momentum \(\overrightarrow p \). The relation \(\frac{{{{\left| {\overrightarrow p } \right|}^2}}}{{2\mu }} + V = E\) is transcribed into quantum mechanics by substituting operators for the physical observables total energy, momentum, and potential energy according to:

$$E \to \underline E = i\hbar \frac{\partial }{{\partial t}}$$

,

$$\overrightarrow p \to \underline {\overrightarrow p } = - i\hbar \underline {\overrightarrow \nabla }$$

,

$$V \to \underline V$$

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References

  • This type integral occurs frequently in line strength calculations. The notation varies. Sometimes the notation Pnℓ(r) = rRnℓ(r) is used for the wavefunction. Representative values are given in 4.6. For more extensive coverage see for in­stance: L.C. Green, P.P. Rush, and C.D. Chandler, Astrophys. J. Suppl. 3, 37 (1957).

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© 1987 Springer-Verlag Berlin Heidelberg

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Fischbeck, H.J., Fischbeck, K.H. (1987). Basic wave mechanics. In: Formulas, Facts and Constants for Students and Professionals in Engineering, Chemistry, and Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-72555-5_4

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  • DOI: https://doi.org/10.1007/978-3-642-72555-5_4

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-17610-7

  • Online ISBN: 978-3-642-72555-5

  • eBook Packages: Springer Book Archive

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