Hamiltonian for hydrogen atom?

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Discussion Overview

The discussion revolves around the Hamiltonian formulation for the hydrogen atom, particularly focusing on the inclusion of radiation and radiation reaction terms. Participants explore the implications of external magnetic fields and the self-interaction of electrons within the context of classical and quantum mechanics.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants question why radiation terms are not included in the Hamiltonian for the hydrogen atom, especially when considering an electron moving in a magnetic field.
  • Others argue that classical quantum mechanics does not incorporate couplings to external radiation, suggesting that such terms are neglected in the Hamiltonian derivation.
  • One participant mentions that the external magnetic field is generally ignored in initial considerations, but can be included to account for effects like the Zeeman effect.
  • There is a discussion about whether the electron creates its own magnetic field and how this relates to electromagnetic theory, with some participants asserting that electrons are typically treated as point particles without internal structure.
  • Another point raised is that radiation reaction forces do not fit well into the Hamiltonian framework, as they involve higher derivatives of momentum.
  • Participants discuss the conditions under which radiative effects become significant, referencing specific time scales and parameters relevant to the hydrogen atom.
  • One participant proposes a relativistic Hamiltonian for an electron in an external magnetic field, suggesting a different formulation may be necessary in that context.
  • There is mention of the smallness of radiative corrections in the context of the hydrogen atom, with references to specific time parameters that indicate their relevance.

Areas of Agreement / Disagreement

Participants express differing views on the necessity and implications of including radiation terms in the Hamiltonian. There is no consensus on whether self-interaction should be considered, and the discussion remains unresolved regarding the treatment of radiation effects in this context.

Contextual Notes

Participants note that the inclusion of radiation terms depends on specific conditions and time scales, with some arguing that for the hydrogen atom, these effects are negligible based on the parameters discussed.

cragar
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When I write down the Hamiltonian for the hydrogen atom why do we not include a radiation term or a radiation reaction term? If I had an electron moving in a B field it seems like I would need to have these terms included.
 
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Where do you see a magnetic field? The electron "moves"*, but the nucleus does not (if you reduced the 2-body problem to a 1-body problem).
"Classical" quantum mechanics (no quantum field theory) cannot include couplings to external radiation, or has to use effective models for that, so this is neglected in the derivation.

Edit:
*well, not really, but at least it has a wave function which has expressions similar to a velocity
 
Last edited:
Generally, to begin with, the external magnetic field is ignored. You can add a magnetic field which interacts with the magnetic moment of the atom. This gives rise to the Zeeman effect, the splitting of energy levels based on the z-component of the total angular momentum (usually denoted m).

http://en.wikipedia.org/wiki/Zeeman_effect
 
I was just thinking that the electron was moving into its own B field that it created.
Dont they have something like this in E&M?
 
No, you don't get this.
In quantum field theory, there is some sort of self-interaction, but that cannot be explained with a classical electromagnetic field.
 
I was just thinking that the electron was moving into its own B field that it created.
Dont they have something like this in E&M?
Only if the particle was extended in space. Then one part of the particle could move in the field of another part. However, there is not much evidence for such structured electron and it is difficult even to formulate such theory consistently, so most usually electrons are assumed as points, both in classical electrodynamics and in quantum theory.

When I write down the Hamiltonian for the hydrogen atom why do we not include a radiation term or a radiation reaction term?

Because the Hamiltonian description is well suited for forces which are given by values of r and p. Radiation reaction force k\dot \mathbf{a} does not fit into this framework - it contains second derivative of momentum.

If I had an electron moving in a B field it seems like I would need to have these terms included.

If it is external magnetic field (due to magnet), then one can include it via vector potential or terms like -\boldsymbol{\mu}\cdot\mathbf B into the Hamiltonian. However, there is not much reason to include self-interaction of electron with its own field in the Hamiltonian. For example, most quantum-chemical calculations never use such terms and give quite good results (see Slater, Solid State and Molecular Theory: A Scientific Biography).
 
ok thanks for all of your responses. If I had a relativistic electron moving in a B field would I then have a radiation term? The electron is a free particle moving through an external B field.
 
In relativistic theory, for electron in external magnetic field, I would use

<br /> H = \sqrt{(\mathbf p - \frac{q}{c}\mathbf A)^2c^2 + m^2c^4}<br />
with \mathbf A such that give the magnetic field in question.
 
  • #10
andrien said:
see the page 747 from jackson,here
http://books.google.co.in/books?id=8qHCZjJHRUgC&pg=PA747&dq=radiation+reaction+jackson&hl=en#v=onepage&q=radiation%20reaction%20jackson&f=false
where it is stated that only for time greater than τ which is of the order of 10-24
,radiative effects become important.it is only important when motion changes suddenly in that much time which is of course not the case.
for hydrogen atom the only time parameter we can see is of order of10-10/107(bohr radius/velocity).velocity is only some approximate idea here.It is of order of 10-17,which is far from 10-24.
 
  • #11
andrien said:
It is of order of 10-17,which is far from 10-24.
This shows that radiative corrections are small.
 
  • #12
mfb said:
This shows that radiative corrections are small.
sure,it shows it.the parameter τ is the only parameter in classical electrodynamics which is relevant for considering whether radiative corrections should be included or not.
 

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