ExoMol line lists – XLIV. Infrared and ultraviolet line list for silicon monoxide (28Si16O)

Author:

Yurchenko Sergei N1,Tennyson Jonathan1ORCID,Syme Anna-Maree2,Adam Ahmad Y3,Clark Victoria H J1ORCID,Cooper Bridgette1,Dobney C Pria1,Donnelly Shaun T E4,Gorman Maire N4,Lynas-Gray Anthony E156,Meltzer Thomas1,Owens Alec1ORCID,Qu Qianwei1ORCID,Semenov Mikhail17,Somogyi Wilfrid1,Upadhyay Apoorva1,Wright Samuel1,Zapata Trujillo Juan C2

Affiliation:

1. Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK

2. School of Chemistry, University of New South Wales, Sydney, NSW 2052, Australia

3. Physikalische und Theoretische Chemie, Fakultät für Mathematik und Naturwissenschaften, Bergische Universität Wuppertal, D-42097 Wuppertal, Germany

4. Department of Physics, University of Aberystwyth, Ceredigion SY23 3BZ, UK

5. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK

6. Department of Physics and Astronomy, University of the Western Cape, Bellville 7535, South Africa

7. Department of Science and Research, Moscow Witte University, 2nd Kozhukhovskiy passage, Moscow 115432, Russian Federation

Abstract

ABSTRACT A new silicon monoxide (28Si16O) line list covering infrared, visible, and ultraviolet regions called SiOUVenIR is presented. This line list extends the infrared EBJT ExoMol line list by including vibronic transitions to the $A\, {}^{1}\Pi$ and $E\, {}^{1}\Sigma ^{+}$ electronic states. Strong perturbations to the $A\, {}^{1}\Pi$ band system are accurately modelled through the treatment of six dark electronic states: $C\, {}^{1}\Sigma ^{-}$, $D\, {}^{1}\Delta$, $a\, {}^{3}\Sigma ^{+}$, $b\, {}^{3}\Pi$, $e\, {}^{3}\Sigma ^{-}$, and $d\, {}^{3}\Delta$. Along with the $X\, {}^{1}\Sigma ^{+}$ ground state, these nine electronic states were used to build a comprehensive spectroscopic model of SiO using a combination of empirical and ab initio curves, including the potential energy (PE), spin–orbit, electronic angular momentum, and (transition) dipole moment curves. The ab initio PE and coupling curves, computed at the multireference configuration interaction level of theory, were refined by fitting their analytical representations to 2617 experimentally derived SiO energy levels determined from 97 vibronic bands belonging to the X–X, E–X, and A–X electronic systems through the MARVEL (Measured Active Rotational–Vibrational Energy Levels) procedure. 112 observed forbidden transitions from the C–X, D–X, e–X, and d–X bands were assigned using our predictions, and these could be fed back into the MARVEL procedure. The SiOUVenIR line list was computed using published ab initio transition dipole moments for the E–X and A–X bands; the line list is suitable for temperatures up to 10 000 K and for wavelengths longer than 140 nm. SiOUVenIR is available from www.exomol.com and the CDS data base.

Funder

STFC

European Research Council

EPSRC

NERC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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