Hyperfine structure in hydrogen

In summary, the conversation discusses the Dirac equation for a bounded electron in a hydrogen atom and the various mathematical terms that appear in the Hamiltonian and energy spectrum. These terms include kinetic and Coulombic potential, mass variation, spin-orbit interaction, the Darwin term, electron and proton spin interactions, and corrections for fluctuations in radiation vacuum and when the electron is inside the proton. The question is raised about whether there are other contributing energies, such as gravity or the electron's own Coulombic potential. The conversation also touches on the Taylor series expansion of the fine structure constant and the approximation of the exact eigenstate without neglecting any source of energy. It is noted that there are infinitely many terms that would be needed for an exact solution
  • #1
victorvmotti
155
5
Consider the Dirac equation for bounded electron in hydrogen atom.

I am trying to get a clear physical explanation for all mathematical terms that appear in the Hamiltonian and energy spectrum.

Kinetic and Coulombic potential and rest energies are the first terms and easy to identify.

Then we have mass variation term and spin-orbit interaction term.

The Darwin term is due to Zitterbewegung or oscillation about the mean position.

Also we need to add electron spin and proton spin interaction.

Another correction is due to fluctuations in radiation vacuum.

Yet another correction is that when electron wavefunction is inside proton and Coulombic potential does not apply.

The question is that should we consider any other contributing energy?

How about gravity? Or electron Coulombic potential on itself?

Also related is that when expanding a Taylor series of the square of fine structure constant to obtain energy eigenvalues should there be a physical meaning or interpretation for all mathematical terms in the series and not only the few beginning terms?

In brief where our approximation ends and the full exact eigen state is obtained without neglecting any source of energy?
 
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  • #2
victorvmotti said:
In brief where our approximation ends and the full exact eigenstate is obtained without neglecting any source of energy?
Never. There are infinitely many terms that would be needed to account for everything exactly. You may find out the approximations that very high precision predictions of electronic properties require by searching scholar.google.com for papers on NRQED (nonrelativistic QED).
 

1. What is hyperfine structure in hydrogen?

Hyperfine structure in hydrogen refers to the small but measurable differences in energy levels of the hydrogen atom due to the interaction between the nucleus and the electron. This results in a splitting of the spectral lines, which can be observed in the hydrogen spectrum.

2. How is hyperfine structure in hydrogen important in atomic physics?

Hyperfine structure in hydrogen is important in atomic physics because it provides a way to study the properties of the nucleus, such as its spin and magnetic moment. It also allows for a more precise measurement of fundamental physical constants, such as the fine structure constant.

3. What causes hyperfine structure in hydrogen?

The hyperfine structure in hydrogen is caused by the interaction between the nuclear spin, which is a result of the proton's magnetic moment, and the electron's spin. This interaction results in a splitting of the energy levels, as the electron can have two different orientations relative to the nucleus.

4. How is hyperfine structure in hydrogen measured?

The hyperfine structure in hydrogen can be measured using spectroscopy techniques, such as the Michelson interferometer or the Fabry-Perot interferometer. These techniques allow for the precise measurement of the energy levels and the splitting of the spectral lines.

5. What is the significance of hyperfine structure in hydrogen for astronomy?

Hyperfine structure in hydrogen is significant for astronomy because it allows for the measurement of the redshift of distant objects in the universe. This redshift can then be used to determine the expansion rate of the universe and its age. It also helps in studying the composition and properties of interstellar gas clouds.

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