Abstract
H2- and He-broadening coefficients of CO2 and their temperature dependence were measured for the R(18) and R(20) transitions of the ν1+ν3 band at 3728.4101 and 3729.7122 cm−1, respectively. Measurements were performed using a tunable distributed-feedback laser near 2.7 µm in a high-temperature optical cell. Absorbance spectra were recorded for mixtures of 1–4% CO2 in H2 or He at ten pressures between 75 and 600 Torr, covering temperatures of 295–805 K for H2 and 295–1005 K for He. The upper temperature limit for the H2 mixtures was imposed by the onset of the reverse water-gas shift reaction. The measured line shapes were fitted with Voigt profiles, with residuals typically less than 1%. Broadening coefficients were obtained from the linear pressure dependence of the fitted collisional widths, and temperature exponents were obtained from power-law fits. The room-temperature H2-broadening coefficients are 0.1124 and 0.1118 cm−1 atm−1 for the R(18) and R(20) transitions, with temperature exponents of 0.676 and 0.655, respectively. The corresponding He-broadening coefficients are 0.0591 and 0.0583 cm−1 atm−1, with exponents of 0.569 and 0.543. The measured H2 exponents are 13–16% larger than the constant value adopted in HITRAN 2024 but agree within 6% with recent requantized classical molecular dynamics predictions. These results provide the first H2- and He-broadening data for the ν1+ν3 band and the first experimental validation of He-broadening predictions above 760 K.
| Original language | English |
|---|---|
| Article number | 110092 |
| Journal | Journal of Quantitative Spectroscopy and Radiative Transfer |
| Volume | 364 |
| DOIs | |
| State | Published - Dec 2026 |
Bibliographical note
Publisher Copyright:© 2026 Elsevier Ltd.
Keywords
- CO
- H-broadening
- HITRAN
- He-broadening
- Pressure broadening
- Temperature exponent
ASJC Scopus subject areas
- Radiation
- Atomic and Molecular Physics, and Optics
- Spectroscopy
Fingerprint
Dive into the research topics of 'High-temperature H2- and He-broadening of CO2 in the ν1+ν3 band'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver