ExoMol line lists – XXXVIII. High-temperature molecular line list of silicon dioxide (SiO2)
A. Owens, E. K. Conway, Jonathan Tennyson, S. N. Yurchenko
Abstract
ABSTRACT Silicon dioxide (SiO2) is expected to occur in the atmospheres of hot rocky super-Earth exoplanets but a lack of spectroscopic data is hampering its possible detection. Here, we present the first, comprehensive molecular line list for SiO2. The line list, named OYT3, covers the wavenumber range 0 – 6000 cm−1 (wavelengths λ > 1.67 μm) and is suitable for temperatures up to T = 3000 K. Almost 33 billion transitions involving 5.69 million rotation–vibration states with rotational excitation up to J = 255 have been computed using robust first-principles methodologies. The OYT3 line list is available from the ExoMol data base at www.exomol.com.
Topics & Concepts
ExoplanetPhysicsLine (geometry)SiliconAstrophysicsSilicon dioxideRotation (mathematics)ExcitationWavelengthAstronomyPlanetOpticsOptoelectronicsQuantum mechanicsMathematicsEngineeringChemical engineeringGeometrySpectroscopy and Laser ApplicationsAtmospheric Ozone and ClimateMolecular Spectroscopy and Structure