Global modeling of the 15N216O line positions within the framework of the polyad model of effective Hamiltonian and a room temperature 15N216O line list

Author(s):  
S.A. Tashkun ◽  
V.I. Perevalov ◽  
A.-W. Liu ◽  
S.-M. Hu
2012 ◽  
Vol 113 (11) ◽  
pp. 1004-1012 ◽  
Author(s):  
V.I. Perevalov ◽  
S.A. Tashkun ◽  
R.V. Kochanov ◽  
A.-W. Liu ◽  
A. Campargue

2013 ◽  
Vol 288 ◽  
pp. 28-37 ◽  
Author(s):  
Clara Sousa-Silva ◽  
Sergei N. Yurchenko ◽  
Jonathan Tennyson

2019 ◽  
Vol 21 (6) ◽  
pp. 3264-3277 ◽  
Author(s):  
Phillip A. Coles ◽  
Sergei N. Yurchenko ◽  
Richard P. Kovacich ◽  
James Hobby ◽  
Jonathan Tennyson

Calculations are reported on the rotation–vibration energy levels of the arsine molecule with associated transition intensities.


2015 ◽  
Vol 28 (3) ◽  
pp. 216-231 ◽  
Author(s):  
A. A. Lukashevskaya ◽  
O. M. Lyulin ◽  
A. Perrin ◽  
V. I. Perevalov

1980 ◽  
Vol 34 (1) ◽  
pp. 81-84 ◽  
Author(s):  
T. Koike ◽  
W. C. Gardiner

Absorptivity measurements for the 3.39 μm He-Ne laser line are reported for acetylene, ethylene, and propylene over the temperature ranges 1500 to 3000 K (acetylene), 1000 to 2000 K (ethylene), and 700 to 2300 K (propylene). In contrast to the behavior of other hydrocarbons, the absorptivities of acetylene and ethylene increase with increasing temperature. The conventional spectroscopic analysis of line positions based upon high-resolution infrared spectroscopy at room temperature and approximate line-broadening theory indicate that no absorption at all would be expected for acetylene or ethylene. The time-resolved absorption profiles and computer models of the chemical behavior expected for shock-heated test gas confirm that the absorption is really due to these molecules, but must be attributed to some heretofore unidentified absorption process.


Author(s):  
Brana Jovanić ◽  
Marco Bettinelli ◽  
Bozidar Radenković ◽  
Marijana Despotović-Zrakić ◽  
Fabio Piccinelli ◽  
...  

The effect of hydrostatic pressure (varying up to 110 kbar) at the room temperature on three lines at 594nm, 615nm and 619nm positions in emission spectra and fluorescence lifetime t of the Eu3+ for 0-2 line (5D0→7F2 transition) in LuVO4: Eu3+ nanoparticles was studied. The results showed that the increase of the pressure induced lines red shift towards longer wavelengths for all considered lines with different rate. Also, the fluorescence lifetime τ for 5D0 → 7F2 transition nonlinearly decreased with pressure in the considered pressure range. Line positions and fluorescence lifetime τ, were explained by a model which took into account the effect of high pressure on: refractive index of crystal; compression, polarizability of the crystal and individual ions. Satisfactory agreement between measured and theoretical predicted values with error less than 2% was obtained.


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