Difference between revisions of "Atomic Units"

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== Atomic Units ==
 
The natural units for describing atomic systems are obtained by setting to unity
 
The natural units for describing atomic systems are obtained by setting to unity
the three fundamental constants that appear in the hydrogen Hamiltonian (Eq.
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the three fundamental constants that appear in the hydrogen Hamiltonian, <math>\hbar=m=e=1</math>.  One thus arrives at atomic units, such as
\ref{eq:coulomb}), <math>\hbar=m=e=1</math>.  One thus arrives at atomic units, such as
 
  
* length: Bohr radius = <math>a_0=\frac{\hbar^2}{me^2}=\frac{1}{\alpha}\frac{\hbar}{mc}=0.53 {\rm \AA}</math>
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<!--<math>\def\AA\unicode{x212B}</math>-->
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* length: Bohr radius = <math>a_0=\frac{\hbar^2}{me^2}=\frac{1}{\alpha}\frac{\hbar}{mc}=0.53 A </math>
 
* energy: 1 hartree = <math>\frac{e^4 m}{\hbar^2}=(\frac{e^2}{c\hbar})^2mc^2=\alpha^2 mc^2=27.2\ \textrm{eV}</math>
 
* energy: 1 hartree = <math>\frac{e^4 m}{\hbar^2}=(\frac{e^2}{c\hbar})^2mc^2=\alpha^2 mc^2=27.2\ \textrm{eV}</math>
 
* velocity: <math>m v^2=\frac{e^{4}m}{\hbar^2}\Rightarrow v=\frac{e^2}{\hbar}=\alpha\cdot
 
* velocity: <math>m v^2=\frac{e^{4}m}{\hbar^2}\Rightarrow v=\frac{e^2}{\hbar}=\alpha\cdot
 
c=2.2\times 10^8\ \textrm{cm/s}</math>
 
c=2.2\times 10^8\ \textrm{cm/s}</math>
* electric field: <ref>This is the characteristic value for the <math>n=1</math> orbit of hydrogen.</ref><math>\frac{e}{a_0^2}=5.142\times 10^9~{\rm V/cm} </math>  
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* electric field: <math>\frac{e}{a_0^2}=5.142\times 10^9~{\rm V/cm} </math>  
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: Note: This is the characteristic value for the <math>n=1</math> orbit of hydrogen.
  
As we see above, we can express the atomic units in terms of <math>c</math> instead of <math>e</math> by introducing a single dimensionless constant
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As we see above, we can express atomic units in terms of <math>c</math> instead of <math>e</math> by introducing a single dimensionless constant
 
:<math>
 
:<math>
 
\alpha=\frac{e^2}{\hbar c}\approx\frac{1}{137}.
 
\alpha=\frac{e^2}{\hbar c}\approx\frac{1}{137}.
 
</math>
 
</math>
The \textit{fine structure constant} (footnote: The name "fine structure constant" derives from the appearance of <math>\alpha^2</math> in the ratio of fine structure splitting to the Rydberg.} <math>\alpha</math> 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.
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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.
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:
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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>
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<math>\Delta\simeq mc^2\Rightarrow \Delta p=mc</math>, so (uncertainty principle <math>\Rightarrow </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
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</math>
 
</math>
 
i.e. in relativistic units the strength of this "stronger" Coulomb
 
i.e. in relativistic units the strength of this "stronger" Coulomb
interaction is <math>\alpha</math>.  That <math>\alpha=\frac{1}{137}</math> says that the
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interaction is <math>\alpha</math>.  The fact that <math>\alpha=\frac{1}{137}</math> implies that the
 
Coulomb interaction is weak.
 
Coulomb interaction is weak.
 
<references/>
 

Latest revision as of 00:12, 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) , so (uncertainty principle ) 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.