Hi L.,
The hyperfine coefficients are used to calculate the hyperfine energy level plot for a given level (e.g. 2P3/2). The ‘A’ coefficient is the magnetic dipole contribution (which is typically discussed in textbooks) and the ‘B’/’C’ coefficients are higher order corrections (electric quadrupole/octupole). For a given atom, the coefficients must be found in the spectroscopy literature.
However, pylcp includes the hyperfine coefficients for most of the relevant levels of alkali atoms in the pylcp.atom classes (see https://python-laser-cooling-physics.readthedocs.io/en/latest/atom_class.html). We’re working on adding support for some alkaline-earths as well.
Daniel
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Hi L.,
At least for bosonic isotopes, simulations of singlet-to-singlet and single-to-triplet transitions of alkaline-earth elements can proceed using the same code in pylcp. The only change that you’ll need to make is to update the cell [2] in the Recoil-limited MOT example with the wavenumber, natural decay rate, etc. of the transition that you want to simulate. (Of course, you’ll also have to adjust the saturation and detuning in cell [3]).
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Hi L.,
That’s correct (at least for bosons). If you want to simulate a fermion, then significant changes will be in order.
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