Is 3s to 2s transition for Hygrogen forbidden?

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Discussion Overview

The discussion centers on the possible transitions in hydrogen's emission spectra, specifically examining the transitions from the n = 3 energy level to the n = 2 level, including various orbital types (s, p, d). Participants explore the implications of selection rules and the observed versus theoretical spectrum lines.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants assert that the selection rule \(\Delta l = \pm 1\) must be satisfied for any transition, particularly for one-photon transitions.
  • Others note that for many-photon transitions, the selection rule does not apply in the same way, suggesting these transitions can occur with lower probabilities.
  • A participant references Max Born's atomic physics text, indicating that the number of observed hydrogen spectrum lines is fewer than theoretically expected, raising questions about the relevance of selection rules.
  • Another participant suggests that relativistic corrections may affect selection rules, proposing that they are not strictly "broken" but rather supplemented by additional rules when corrections are considered.
  • It is mentioned that what are commonly referred to as selection rules pertain specifically to electric dipole transitions, and that other types of transitions (magnetic dipole, quadrupole) follow different rules and are less likely to occur.

Areas of Agreement / Disagreement

Participants generally agree on the importance of selection rules but express differing views on their applicability and the impact of relativistic corrections. The discussion remains unresolved regarding the implications of these factors on the observed spectrum lines.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the nature of transitions and the dependence on definitions of selection rules. The scope of the discussion is also limited to hydrogen and does not extend to other elements or systems.

SimonZ
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For hydrogen emission spectra from n = 3 to n = 2:


My question is: In the following transition which is (are) possible or impossible and why?

3s --> 2s, 3s --> 2p
3p --> 2s, 3p --> 2p,
3d --> 2s, 3d --> 2p,
 
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Selection rules! If you have a copy of Griffiths' "Introduction to Quantum Mechanics", take a look at section 9.3.3.
 
You need to have [tex]\Delta l = \pm 1[/tex] for any transition.
 
The number of observed hydrogen spectrum lines is much fewer than theoretically expected.

Atomic physics by Max Born
In page 167, it is written as follows,

-------------------------------------------------------------------------
The case of hydrogen is peculiar in one respect. Experiment gives distinctly fewer terms than are specified in the term scheme of fig 9; for n=2 only two terms are found, for n=3 only three, and so on.
The theoretical calculation shows that here (by a mathematical coincidense, so to speak) two terms sometimes coincide, the reason beeing that the relativity and spin corrections partly compensate each other.

It is found that terms with the same inner quantum number j but different azimuthal quantum numbers l always strictly coincide.
----------------------------------------------------------
http://books.google.com/books?id=NmM-KujxMtoC&printsec=frontcover&dq=Max+Born&lr=

Hydrogen atom has only one electron. So is it relevant?

To search spectrum line, please see http://physics.nist.gov/PhysRefData/ASD/lines_form.html
and enter "H" into "Spectrum" part. "Observed wavelength" is observed line, and "Configurations" is theoretically permitted transition.

Even if we consider selection rules(due to spin 1 of photon), the observed spectrum lines are fewer than expected.
 
Last edited:
Nabeshin said:
You need to have [tex]\Delta l = \pm 1[/tex] for any transition.
It is valid for one-photon transition. For many-photon transitions this is not true. Such processes occur, just with much smaller probability.
 
Bob_for_short said:
It is valid for one-photon transition. For many-photon transitions this is not true. Such processes occur, just with much smaller probability.

Thank you for the correction :)
 
Also, aren't selection rules broken by relativistic corrections?

I have a friend who's really into super conductors and he's showed me before where selection rules and gauge symmetry get broken up. Most of the experiments comes form the ESA:

http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6TVJ-4H57JRK-2&_user=6861066&_rdoc=1&_fmt=&_orig=search&_sort=d&_docanchor=&view=c&_searchStrId=960704834&_rerunOrigin=google&_acct=C000055858&_version=1&_urlVersion=0&_userid=6861066&md5=9454a1fb6b2b2da44f5ff095d6b70ccc
 
The selection rules are not "broken" so much as supplemented when you introduce the corrections. For example, when you introduce fine and hyperfine structure corrections, you get more selection rules.

One thing to note about selection rules, what you are calling "selection rules" are "selection rules for a electric dipole transition", you can have higher order electric transitions and you can have magnetic transitions, which will follow different rules. Magnetic dipole, quadrupole, etc and electric quadrupole, etc transitions are orders of magnitude less likely to occur, and so are often ignored. So cases where you see them broken, they may just not be electric dipole transitions.
 

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