Measurement of Hydrogen 1s 4s transition frequency

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Discussion Overview

The discussion revolves around the measurement of the hydrogen 1s-4s transition frequency, with participants exploring the accuracy of existing measurements and the availability of data compared to other transitions like 1s-2s and 1s-3s. The scope includes theoretical considerations, experimental data, and historical context regarding spectral lines in hydrogen.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Historical

Main Points Raised

  • One participant inquires about the accuracy of the measurement for the hydrogen 1s-4s transition, noting a lack of information compared to other transitions.
  • Another participant mentions the Lyman-γ line as relevant to the hydrogen spectrum and suggests searching for the "Lyman series" for more information.
  • A participant expresses interest in measurements with high accuracy, similar to the 1s-2s and 1s-3s transitions, and questions the reliability of calculated values compared to observed data.
  • Concerns are raised about the accuracy of NIST's reported wavelengths, with one participant suggesting that the measured values may need updating based on newer measurements.
  • Another participant references a paper by Kramida that compiles experimental data on hydrogen spectral lines and energy levels.
  • There is a discussion about the distinction between theoretical and experimental data, with some participants expressing skepticism about the reliability of quasi-calculated Ritz wavelengths.
  • A participant notes that 1s-ns transitions are two-photon transitions and suggests that measuring the 1s-4s transition directly may not be necessary, as it could be derived from other measurements.
  • One participant mentions the relevance of accurate transition measurements to resolving the proton radius anomaly and seeks additional data on Fraunhofer lines in the UV region.
  • A historical perspective is provided regarding rocket missions in the 50s and 60s that photographed the solar spectrum, highlighting the Lyman alpha line and questioning the current state of research in this area.

Areas of Agreement / Disagreement

Participants express varying degrees of uncertainty regarding the availability and accuracy of measurements for the hydrogen 1s-4s transition. While some agree on the importance of accurate data, there is no consensus on the current state of measurements or the necessity of direct measurement versus derived values.

Contextual Notes

Participants note limitations in the accuracy of measured versus calculated values and the potential need for updated measurements. The discussion also highlights the complexity of distinguishing between theoretical and experimental data in the context of spectral lines.

Who May Find This Useful

Readers interested in atomic physics, spectroscopy, and the historical context of hydrogen measurements may find this discussion relevant.

neilparker62
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Has this been accurately measured yet? Google searches yield results for H 1s-2s and H 1s-3s transitions but not 1s-4s.
 
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The hydrogen spectrum has been measured in exquisite detail. The line you are referring to is called the Lyman-γ line. If you search on "Lyman series", you will find the wavelength.
 
Ok thanks - I tried. Don't find much at all. I am looking for measurement in the same order of accuracy as the 1s-2s and 1s-3s transition frequencies have been measured.

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http://physics.nist.gov/cgi-bin/ASD/lines1.pl at NIST I think has the accuracy you are looking for (12 significant figures). When you are talking this level of accuracy, you need to specify which of the transitions you are talking about, taking into account the fine structure, hyperfine structure, etc. This site, also at NIST, gives the energy levels to about the same level of accuracy (12-13 figures).

Edit: I see the links don't work the way I've done them. Try going here, I entered H I for the spectrum, and 97.2 and 97.3 for the upper and lower wavelengths. Then at the bottom you can click on "Levels" and again put in H I to get the energy levels.
 
Thanks again - I think I tried that but the problem is the 12 sf figures seem to be calculated ones. I am interested in accurately observed data. It somehow doesn't make sense to calculate something to 12 sf when your measured is only accurate to about 7 sf ?? For example in the 1s-3s transition, the NIST site gives a measured wavelength of 102.5728 nm and that seems to be for 1s-3p rather than 1s-3s. I think they might need to update their observed data in light of more recent measurements such as those I mentioned in the previous post - you can easily convert to wavelength from v = fλ with v=c. When you do this you see the calculated numbers (Ritz wavelengths) are pretty good tracking the measured wavelength down to about 9 sf. Wonder what the formula for that is ?? I have a formula which tracks down to about 7sf on the 1s-2s and 1s-3s transitions.
 
Sounds like you know more than I do about it. However, the NIST Energy level page explicitly says " Most of the given level values are essentially experimental ones." It also gives a link to the paper by Kramida, which seems to have a wealth of information, but more than I want to delve into:

"A critical compilation of experimental data on spectral lines and energy levels of hydrogen, deuterium, and tritium",
 
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Thanks all the same for the NIST references - they certainly provide very thorough coverage of the various transition wavelengths in the Hydrogen spectrum.

From what I can understand, the Ritz wavelengths seem to be 'quasi calculated' so not really experimental. I think science become a bit hazy when we can't really distinguish between theoretical and measured data - the whole idea is to put up theories which are ultimately judged by the degree to which they concur with actual measurement. To date the only really accurate measured values I can find are those for the H 1s-2s and H 1s-3s transition frequencies. For interest here are references for these measurements:

Improved Measurement of the Hydrogen 1S–2S Transition Frequency

Optical frequency measurement of the 1S-3S two-photon transition in hydrogen
 
neilparker62 said:
Thanks all the same for the NIST references - they certainly provide very thorough coverage of the various transition wavelengths in the Hydrogen spectrum.

From what I can understand, the Ritz wavelengths seem to be 'quasi calculated' so not really experimental. I think science become a bit hazy when we can't really distinguish between theoretical and measured data - the whole idea is to put up theories which are ultimately judged by the degree to which they concur with actual measurement. To date the only really accurate measured values I can find are those for the H 1s-2s and H 1s-3s transition frequencies. For interest here are references for these measurements:

Improved Measurement of the Hydrogen 1S–2S Transition Frequency

Optical frequency measurement of the 1S-3S two-photon transition in hydrogen
1s-ns are going to be two photon transitions. There might not be much reason to do the1s-4s measurement directly, though, because you can do separate experiments to measure say 1s-2p (one photon) and measure 2p-4s (one photon). The precise measurement of the 2s-2p energy difference (Lamb shift) is something you can read about. QED is needed to explain the shift.
 
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Thanks - I think I read somewhere that accurate determination of 1s-2s, 1s-3s, 1s-4s etc transition energies/frequencies was needed to resolve the proton radius anomaly

Some more data I am looking for if anyone can help: accurate values of wavelengths for Fraunhofer lines stretching into the UV region for the H I Lymann series. I found this reference:

http://www.coseti.org/9006-025.htm

but it only seems to cover lines in the visible spectrum.
 
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Just by way of history, there were a lot of rocket missions in the late 50s, early 60s to photograph the solar spectrum in the UV region. Various Lymnan series lines are clear in these photos. Of particular note is the Lyman alpha line which shows up as a bright emission band with a very sharp absorption dip right in the centre (I hope I interepreted the plates I saw correctly). It seems surprising that interest in this region of the solar spectrum seems to have subsequently waned - one would of thought that with today's technology , much higher resolution photos of the spectrum would be available and it should also be possible to measure the important wavelengths to a great degree of precision. In particular the Lymann Alpha absorption dip. Or am I just missing something in my Google searches ??

Reference for the 50s/60s missions here.
 

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