Difference between revisions of "Atomic Units"
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The ''fine structure constant'' <math>\alpha</math> obtained its name from the appearance of <math>\alpha^2</math> in the ratio of fine structure splitting to the Rydberg; it 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) ), <math>\alpha</math>, as a dimensionless constant, is not defined by metrology. Rather, <math>\alpha</math> characterizes the strength of the electromagnetic interaction, as the following example will illustrate. | The ''fine structure constant'' <math>\alpha</math> obtained its name from the appearance of <math>\alpha^2</math> in the ratio of fine structure splitting to the Rydberg; it 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) ), <math>\alpha</math>, as a dimensionless constant, is not defined by metrology. Rather, <math>\alpha</math> characterizes the strength of the electromagnetic interaction, as the following example will illustrate. | ||
− | If energy uncertainties become become as large as <math>\Delta E=mc^2</math>, 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 | + | If energy uncertainties become become as large as <math>\Delta E=mc^2</math>, 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 (before e.g. spontaneous pair production may occur) |
<math>\Delta\simeq mc^2\Rightarrow \Delta p=mc</math> | <math>\Delta\simeq mc^2\Rightarrow \Delta p=mc</math> | ||
<math>\Delta x=\frac{\hbar}{mc}=\lambda_c</math> | <math>\Delta x=\frac{\hbar}{mc}=\lambda_c</math> |
Revision as of 04:06, 22 February 2010
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, . One thus arrives at atomic units, such as
- length: Bohr radius =
- energy: 1 hartree =
- velocity:
- electric field:
- Note: This is the characteristic value for the orbit of hydrogen.
As we see above, we can express atomic units in terms of instead of by introducing a single dimensionless constant
The fine structure constant obtained its name from the appearance of in the ratio of fine structure splitting to the Rydberg; it 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 (before e.g. spontaneous pair production may occur) 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.