1982
DOI: 10.1016/0301-0104(82)85047-7
|View full text |Cite
|
Sign up to set email alerts
|

Superfine and hyperfine structures in the v3 band of 32SF6

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

2
15
0

Year Published

1985
1985
2008
2008

Publication Types

Select...
5
1
1

Relationship

0
7

Authors

Journals

citations
Cited by 65 publications
(17 citation statements)
references
References 35 publications
2
15
0
Order By: Relevance
“…The parameters marked by an asterisk were fixed to zero. P (5) gives the value of the parameter obtained by fitting of the 136 lines of paper I with the fifth order Hamiltonian. 1 state Hamiltonian.…”
Section: Table 5 Values Of the 52 Adjusted Parameters Of The Tenth-ormentioning
confidence: 99%
See 1 more Smart Citation
“…The parameters marked by an asterisk were fixed to zero. P (5) gives the value of the parameter obtained by fitting of the 136 lines of paper I with the fifth order Hamiltonian. 1 state Hamiltonian.…”
Section: Table 5 Values Of the 52 Adjusted Parameters Of The Tenth-ormentioning
confidence: 99%
“…In this case, the linewidth was limited by transit and power broadening to a larger value for which the hyperfine structure was not resolved. Furthermore, for tight superfine clusters, the hyperfine mixing of levels with different vibration-rotation symmetry species (5,6) gives rise to complicated asymmetrical structures which are only partly resolved. For a number of these cases we have calculated the expected struc-ture to determine an approximate position of the true vibrationrotation line center (i.e., free of hyperfine effects).…”
mentioning
confidence: 99%
“…In the case of an octahedral-type molecule like the SF 6 , we can follow the discussion given in reference [5].…”
Section: Symmetry Considerationsmentioning
confidence: 99%
“…The study of magnetic hyperfine structures F o r P e e r R e v i e w O n l y detected in highly symmetric molecules like this has progressed enormously in the seventh and eighth decades of last century. Some of the fundamental tools for that progress were the ultra-high resolution infrared spectroscopy [1][2][3] and the development of a tensorial formalism suitable for the interpretation of the measured spectra [4][5][6][7][8]. However, the theoretical determination of the electronic contribution to the nuclear hyperfine constants included in the hamiltonian that describes the magnetic hyperfine structures, could not be achieved in those days due to the impossibility of achieving sufficiently accurate calculations.…”
Section: Introductionmentioning
confidence: 99%
“…It is not a trivial task to work out the relevant Hamiltonian in detail as some account should be taken of the direct vibration-spin coupling because of the vibrational angular momentum. However, as for spherical tops [16], effective spin-rotation constants in the upper level can describe the observed structure of a given rovibrational line. The match between observed and calculated spectra in Fig.…”
mentioning
confidence: 97%