Fundamental series

The fundamental series is a set of spectral lines in a set caused by transition between d and f orbitals in atoms.

Originally the series was discovered in the infrared by Fowler and independently by Arno Bergmann.[1] This resulted in the name Bergmann series used for such a set of lines in a spectrum. However the name was changed as Bergmann also discovered other series of lines. And other discoverers also established other such series. They became known as the fundamental series.[2] Bergmann observed lithium at 5347 cm−1, sodium at 5416 cm−1 potassium at 6592 cm−1.[2] Bergmann observed that the lines in the series in the caesium spectrum were double. His discovery was announced in Contributions to the Knowledge of the Infra-Red Emission Spectra of the Alkalies, Jena 1907.[3] Carl Runge called this series the "new series". He predicted that the lines of potassium and rubidium would be in pairs.[3] He expressed the frequencies of the series lines by a formula and predicted a connection of the series limit to the other known series. In 1909 W. M. Hicks produced approximate formulas for the various series and noticed that this series had a simpler formula than the others and thus called it the "fundamental series" and used the letter F.[1][4]

The formula that more resembled the hydrogen spectrum calculations was because of a smaller quantum defect. There is no physical basis to call this fundamental.[5] The fundamental series was described as badly-named.[6] It is the last spectroscopic series to have a special designation.[6] The next series involving transitions between F and G subshells is known as the FG series.[6]

Frequencies of the lines in the series are given by this formula:

R is the Rydberg constant, is the series limit, represented by 3D, and is represented by mF. A shortened formula is then given by with values of m being integers from 4 upwards.[7] The two numbers separated by the "−" are called terms, that represent the energy level of an atom.

The limit of the fundamental series is the same as the 3D level.[5]

The terms can have different designations, mF for single line systems, mΦ for doublets and mf for triplets.[8]

Lines in the fundamental series are split into compound doublets, due to the D and F subshells having different spin possibilities. The splitting of the D subshell is very small and that of the F subshell even less so, so the fine structure in the fundamental series is harder to resolve than that in the sharp or diffuse series.[7]

  1. ^ a b Saunders, F. A. (August 1919). "Review of Recent Work on the Series Spectra of Helium and of Hydrogen". Astrophysical Journal. 50: 151. Bibcode:1919ApJ....50..151S. doi:10.1086/142490.
  2. ^ a b Brand, J. C. D. (24 Nov 1995). Lines of Light. CRC Press. p. 135. ISBN 9782884491631.
  3. ^ a b Runge, Carl (December 1907). "The Spectra of the Alkalies". Astrophysical Journal. 27: 158–160. Bibcode:1908ApJ....27..158R. doi:10.1086/141538.
  4. ^ Hicks, W. M. (9 December 1909). "A Critical Study of Spectral Series.-Part I. The Alkalies H and He". Philosophical Transactions of the Royal Society of London A. 210 (459–470): 57–111. doi:10.1098/rsta.1911.0003. JSTOR 90988.
  5. ^ a b Candler, A. C. (1937). Atomic Spectra and the Vector Model: Volume 1. Cambridge, UK: Cambridge University Press. p. 22. ISBN 9781001286228. Retrieved 28 August 2015. {{cite book}}: ISBN / Date incompatibility (help)
  6. ^ a b c Fowler, A. (23 February 1928). "Spectra and atoms". Journal of the Chemical Society (Resumed): 764–780. doi:10.1039/JR9280000764. S2CID 37856069. (subscription required)
  7. ^ a b Herzberg, Gerhard (January 1944). Atomic Spectra and Atomic Structure. Courier Corporation. p. 56. ISBN 9780486601151. {{cite book}}: ISBN / Date incompatibility (help)
  8. ^ Saunders, F. A. (1915). "Some Recent Discoveries in Spectrum Series". Astrophysical Journal. 41: 323. Bibcode:1915ApJ....41..323S. doi:10.1086/142175.

© MMXXIII Rich X Search. We shall prevail. All rights reserved. Rich X Search