Atomic Units
The natural units for describing atomic systems are obtained by setting to unity the three fundamental constants that appear in the hydrogen Hamiltonian (Eq. \ref{eq:coulomb}), . One thus arrives at atomic units, such as
- length: Bohr radius =
- energy: 1 hartree =
- velocity:
- electric field: [1]
As we see above, we can express the atomic units in terms of instead of by introducing a single dimensionless constant
The \textit{fine structure constant} (footnote: The name "fine structure constant" derives from the appearance of in the ratio of fine structure splitting to the Rydberg.} is the only fundamental constant in atomic physics. As such, it should ultimately be predicted by a complete theory of physics. Whereas precision measurements of other constants are made in atomic physics for purely metrological purposes (see Appendix \ref{app:metrology) ), , as a dimensionless constant, is not defined by metrology. Rather, characterizes the strength of the electromagnetic interaction, as the following example will illustrate. If energy uncertainties become become as large as , the concept of a particle breaks down. This upper bound on the energy uncertainty gives us, via the Heisenberg Uncertainty Principle, a lower bound on the length scale within which an electron can be localized: Even at this short distance of , the Coulumb interaction---while stronger than that in hydrogen at distance --- is only:
i.e. in relativistic units the strength of this "stronger" Coulomb interaction is . That says that the Coulomb interaction is weak.
- ↑ This is the characteristic value for the orbit of hydrogen.