The trans-HOCO radical: quartic force fields, vibrational frequencies, and spectroscopic constants
Ryan C Fortenberry1, Xinchuan Huang, Joseph S Francisco
1Department of Chemistry, Virginia Tech, Blacksburg, Virginia 24061, USA.
Researchers computed the vibrational frequencies of the hydroxyformyl (HOCO) radical. These findings aid in understanding CO2 formation and its presence in the Martian atmosphere.
Area of Science:
- Atmospheric Chemistry
- Quantum Chemistry
- Spectroscopy
Background:
- The hydroxyformyl (HOCO) radical is a key intermediate in the OH + CO reaction, crucial for CO2 formation.
- HOCO's role in the high CO2 concentrations on Mars is suspected but poorly understood due to limited spectroscopic data.
- Previous gas-phase spectroscopic studies of HOCO have not provided a complete set of fundamental vibrational frequencies.
Purpose of the Study:
- To compute the fundamental vibrational frequencies and spectroscopic constants for the trans-HOCO radical in the gas phase.
- To provide reliable theoretical data for comparison with future experimental observations.
- To aid in identifying HOCO in the Martian atmosphere and understanding its role in CO2 chemistry.
Main Methods:
- Utilized high-accuracy quantum chemical coupled cluster techniques.
- Employed quartic force fields for precise calculations.
- Computed all six fundamental vibrational frequencies and rotational constants for trans-HOCO.
Main Results:
- Calculated rotational constants show excellent agreement with experimental values (within 0.01 cm(-1) for A(0) and 10(-4) cm(-1) for B(0) and C(0)).
- Computed fundamental vibrational frequencies are within 4 cm(-1) of known experimental gas-phase modes (ν(1) and ν(2)).
- Predicted the remaining four fundamental modes, with potential for larger discrepancies in the anharmonic torsional mode.
Conclusions:
- The computational methods employed are reliable for predicting trans-HOCO spectroscopic properties.
- The calculated data can assist the ExoMars Trace Gas Orbiter in detecting HOCO on Mars.
- This study contributes to understanding the OH + CO reaction mechanism and Martian atmospheric CO2 retention.
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