The octopole and hexadecapole moments of N2O from collision-induced absorption measurements

1990 ◽  
Vol 68 (12) ◽  
pp. 1440-1445 ◽  
Author(s):  
I. R. Dagg ◽  
A. Anderson ◽  
T. F. Gmach ◽  
C. G. Joslin ◽  
W. Smith

The absorption spectrum of gaseous N2O was measured in the spectral region from approximately 15–120 cm−1 at 11 different densities from 3.3 to 64.5 amagat. (An amagat is defined as the density of a gas at N.T.P.) The data were obtained with a Michelson Fourier transform IR spectrometer and a far IR laser using a stainless steel absorption cell 9.26 cm in length. From the density dependence of the absorption, the collision-induced spectrum above approximately 60 cm−1 was clearly separated from the relatively strong allowed transitions peaking at the lower frequency near 22 cm−1. From theoretical expressions for the line shape, derived using information theory, and a reliable value of the quadrupole moment (obtained from the birefringent measurements), we estimate the octopole moment to be 7.6 × 10−34 esu and the hexadecapole moment to be 16.9 × 10−42 esu. Alternatively, if the hexadecapolar contribution is considered to be negligible, then we estimate the octopole moment to be 9 × 10−34 esu. These results are consistent with measurements of the total integrated absorption of the IR band assuming a theoretical expression for the contribution due to the allowed dipole transitions.

1991 ◽  
Vol 69 (6) ◽  
pp. 671-678 ◽  
Author(s):  
C. G. Joslin ◽  
C. G. Gray ◽  
I. R. Dagg ◽  
A. Anderson ◽  
T. F. Gmach ◽  
...  

The absorption spectrum of gaseous sulphur hexafluoride has been measured in the spectral region from approximately 20 to 140 cm−1 at 339 K. The experiments were performed over a range of densities from 65 to 109.6 amagat (for SF6, 1 amagat = 45.3 mol m−3), using FTIR spectroscopy. From the density dependence of the absorption, the collision-induced spectrum was clearly separated from the strong allowed transitions of vibrational difference bands at 26 and 91 cm−1. Our results for the induced spectrum differ substantially, both in overall magnitude and in shape, from earlier data. We interpret the absorption as due to anisotropic overlap induction; however, a substantial contribution from a hexadecapolar mechanism cannot be ruled out. We can place an upper limit of approximately 7 × 10−42 esu on the hexadecapole moment. The induced line shape is calculated using information theory, based on our knowledge of the zeroth and second moment of the frequency spectrum. Reasonable agreement is found between theory and experiment.


2007 ◽  
Vol 77 (12) ◽  
pp. 2130-2139 ◽  
Author(s):  
A. A. Gazizova ◽  
R. R. Shagidullin ◽  
A. V. Chernova ◽  
Ya. A. Vereshchagina ◽  
D. V. Chachkov ◽  
...  

2017 ◽  
Vol 5 (1) ◽  
pp. 17 ◽  
Author(s):  
V. Manikandan ◽  
S. Balaji ◽  
R. Senbagam ◽  
R. Vijayakumar ◽  
M. Rajarajan ◽  
...  

About ten substituted (E)-N'-1-(substituted benzylidene) benzohydrazides have been synthesized. They are analyzed by their analytical, ultra violet (UV), Fourier transform-IR (FT-IR) and nuclear magnetic resonance (NMR) spectral data and evaluated by antimicrobial activities such antibacterial and antifungal activities.


2008 ◽  
Vol 36 (6) ◽  
pp. 1165-1168 ◽  
Author(s):  
Amandine Maréchal ◽  
W. John Ingledew ◽  
Peter R. Rich

Vibrational changes associated with CO recombination to ferrous horseradish peroxidase were investigated by rapid-scan FTIR (Fourier-transform IR) spectroscopy in the 1200–2200 cm−1 range. At pH 6.0, two conformers of bound CO are present that appear as negative bands at 1905 and 1934 cm−1 in photolysis spectra. Their recombination rate constants are identical, confirming that they arise from two substates of bound CO that are in rapid thermal equilibrium, rather than from heterogeneous protein sites. A smaller positive band at 2134 cm−1 also appears on photolysis and decays with the same rate constant, indicative of an intraprotein geminate site involved in recombination or, possibly, a weak-affinity surface CO-binding site. Other signals arising from protein and haem in the 1700–1200 cm−1 range can also be time-resolved with similar kinetics.


1989 ◽  
Vol 67 (11) ◽  
pp. 1027-1035 ◽  
Author(s):  
A. R. W. McKellar

The spectrum of CH4 obtained in CH4 plus N2 mixtures at a temperature of 77 K has been recorded with a spectral resolution of 0.14 cm−1 in the region 3800 to 9100 cm−1. The experiments were performed with long paths (66 or 88 m) in a cooled absorption cell using a Fourier-transform spectrometer. Data are presented here at low and medium resolution, and examples of some spectral regions are also shown at high resolution. The complete results are available from the author in an Appendix. Comparisons are made with previous model calculations of CH4 absorption, and with the observed spectrum of Neptune's satellite, Triton. The results should be useful for the interpretation of the spectra of Triton, Titan, and Pluto. They will also be of value for testing model calculations of low-temperature CH4 absorption, which, thus verified, can be used with greater confidence to analyze observations of Jupiter, Saturn Uranus, and Neptune.


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