
Multi-Photon Absorption and Ionization


Each s-state transition shows up as one peak on the spectrum. With the d-state transitions, there are technically two peaks, though this is observable in our data only at lower energy states. If you look closely at the 11d, 12d, and 13d lines, you will observe that they have two smaller peaks within the larger peaks. These hyperfine levels result from spin-orbit interaction in states with angular momentum>0. |
11d3/2 and 11d5/2 Spectral Lines
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When an external magnetic field is applied to the atom, the interaction between the spin magnetic moment and the electric field causes an addition or subtraction of potential energy from the electron's energy level. As a result, electrons with spin up will have slightly different energy that electrons in the same state with spin down. When an electron is in a state with angular momentum greater than zero (p, d, f, . . .) the angular magnetic moment will be greater than zero. Thus, for p, d and higher L-states, there will be an intrinsic magnetic field in the atom caused by the angular momentum. This magnetic field causes the spliting of spectral lines when it interacts with the spin magnetic moment of electrons in these higher states. In our experiement we see this splitting only in d-states; s-states have angular momentum zero and, therefore, have no angular magnetic moment to interact with the spin magnetic moment. |
12d3/2 and 12d5/2 Spectral Lines
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