Effect of collisions on line profiles in the vibrational spectrum of molecular hydrogen
- 1 October 1986
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review A
- Vol. 34 (4), 3003-3014
- https://doi.org/10.1103/physreva.34.3003
Abstract
A semiclassical calculation of density-broadening and line-shift coefficients in the vibrational-rotational spectrum of molecular hydrogen is presented. These parameters are obtained as functions of temperature and upper-state quantum numbers, and the calculated results are in good agreement with experimental values obtained from fundamental and overtone electric quadrupole spectra, except for the 4-0 overtone density-broadening coefficient. Results from Raman and electric-field-induced spectra in the fundamental band are also discussed. The calculation includes construction of an intermolecular potential for the - interaction. The vibrational phase shift resulting from collision is shown to account for the vibrational state dependence of the broadening and shift coefficients, and the observed temperature dependence of the line shift is reproduced by the calculation.
Keywords
This publication has 44 references indexed in Scilit:
- Temperature dependence of the Raman linewidth and line shift for the Q(1) and Q(0) transitions in normal and para-Physical Review A, 1986
- High-resolutions cars measurement of Raman linewidths of H2Optics Communications, 1985
- Vibration–rotation line shifts for 1Σg+ H2 (v, J)–1S He computed via close coupling: temperature dependenceThe Journal of Chemical Physics, 1980
- Determination of the H2 4-0 S/1/ quadrupole line strength and pressure shiftThe Astrophysical Journal, 1980
- Intensity and pressure shift of the H2 /4,0/ S/1/ quadrupole lineThe Astrophysical Journal, 1978
- Pressure shifts in the vibrational Raman spectra of hydrogen and deuterium, 315–85 KCanadian Journal of Physics, 1978
- The pressure broadening of the rotational Raman lines of hydrogen isotopesPhysica, 1974
- The significance of pressure shifts for the interpretation of H2 quadrupole lines in planetary spectraIcarus, 1974
- Measurements on Spectra of Gases of Planetary Interest. II. H_{2}, CO_{2}, NH_{3}, and CH_{4}The Astrophysical Journal, 1966
- Line-widths of pressure-broadened spectral linesJournal of Quantitative Spectroscopy and Radiative Transfer, 1962