Atomic electron transition: Difference between revisions

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== Theory ==
Consider an atom interact with electromagnetic radiation which produces an oscillationoscillating electric field <ref>{{Cite book|title=Atomic Physics|author=Foot, CJ|year=2004|
publisher=Oxford University Press|isbn=978-0-19-850696-6}}</ref>:
{{NumBlk|:|<math> E(t) = |\textbf{E}_0| Re( e^{-i{\omega}t} \hat{\textbf{e}}_{rad} )</math>|{{EquationRef|1}}}}
with amplitude <math>|\textbf{E}_0|</math>, angular frequency <math>\omega</math> and polarization vector <math>\hat{\textbf{e}}_{rad}</math>. Note that the actual phase of wave should be <math> (\omega t - \textbf{k} \cdot \textbf{r}) </math>. However, in many cases, the variation of <math> \textbf{k} \cdot \textbf{r} </math> is small over the atom, or equivalently, the radiation wavelength is much greater than the size of an atom. This is called dipole approximation, and this approximation allowallows us to replace <math> E(r, t) </math> with <math> E(0, t) </math> in ({{EquationNote|1}}). Atom can also interact with oscilationoscillating magnetic field produced in the radiaiton with the interaction being much weaker.
 
The Hamiltonian for this interaction is <math> H_I = e \textbf{r} \cdot \textbf{E}(t) </math>, analogous to the energy of a classical dipole in a electric field. [[Time-dependent perturbation theory]] is required for calculating the stimulate transition rate. However, the result can be summarized with Fermi's Golden rule: