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 (before e.g. spontaneous pair production may occur)
 
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>
 
Even at this short distance of <math>\lambda_c</math>, the Coulumb
 
Even at this short distance of <math>\lambda_c</math>, the Coulumb

Revision as of 00:03, 20 February 2024

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 , , 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 . The fact that implies that the Coulomb interaction is weak.