Rydberg constant: Difference between revisions
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imported>John R. Brews (Rydberg constant stub) |
imported>John R. Brews No edit summary |
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:<math>R_{\infty} = \frac{m_ee^4}{4\pi \hbar^3 c}\ \left( {\mu_0 c^2}{4 \pi}\right)^2 \ . </math> | :<math>R_{\infty} = \frac{m_ee^4}{4\pi \hbar^3 c}\ \left( \frac{\mu_0 c^2}{4 \pi}\right)^2 \ . </math> | ||
==Notes== | ==Notes== | ||
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Revision as of 11:11, 13 March 2011
The Rydberg constant, often denoted as R∞, originally defined empirically in terms of the spectrum of hydrogen, is given a theoretical value by the Bohr theory of the atom as:[1]
Notes
- ↑ GW Series (1988). “Chapter 10: Hydrogen and the fundamental atomic constants”, The Spectrum of atomic hydrogen--advances: a collection of progress reports by experts. World Scientific, p. 485. ISBN 9971502615.