Abstract
Phosphorus is a key and vital element for a diverse set of important biological molecules, being indispensable for life as we know. A deeper comprehension of its role in astrochemistry and atmospheric chemistry may aid in finding answers to how this element became available on Earth. The PO molecule is one of the main reservoirs of phosphorus in the interstellar medium (ISM), and a better understanding of the mechanisms and rate coefficients for its formation in the ISM is important for modelling its abundances. In this work, we perform multireference configuration interaction calculations on the formation of PO via the \(\mathrm {P}(^{4}S)+\mathrm {O}_{2}(^{3}\Sigma ^{-})\) reaction, analyzing its potential energy surface and rate coefficients for the global reaction on both doublet and quartet states. We also perform DFT (M06-2X) and CCSD(T) calculations, in order to compare the results. We found that the OPO system possesses a high multiconfigurational character, making DFT and CCSD methodologies not suitable for its potential energy landscape calculation. The rate coefficients have been calculated using the master equation system solver (MESS) package, and the results compared to recent experimental data. It is shown that the quartet state contributes for temperatures higher than 700K. The computed rate coefficient can be described by a modified Arrhenius equation [\(\alpha (T/300)^{\beta } \exp {(-\gamma /T)}\)] with \(\alpha =1.44\times 10^{-12}\text {cm}^{3}\,s^{-1}\), \(\beta =-1.66\) and \(\gamma =704\) K.
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Data availability
The datasets generated during and/or analyzed during the current study are available from the corresponding author on reasonable request.
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Acknowledgements
The authors also acknowledge the National Laboratory for Scientific Computing (LNCC/MCTI, Brazil) for providing HPC resources of the SDumont supercomputer, which have contributed to the research results reported within this paper. URL:http://sdumont.lncc.br, and the Academic Leiden Interdisciplinary Cluster Environment (ALICE) provided by Leiden University. Ahren W. Jasper would like to acknowledge the U. S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences, under Contract Number DE-AC02-06CH11357.
Funding
The authors received financial support from the Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - Brasil (CAPES) - Finance Code 001, Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), grant 311508-2021-9, and Fundação de Amparo à Pesquisa do estado de Minas Gerais (FAPEMIG). Rede Mineira de Química (RQ-MG) and CEFET-MG are also acknowledged. Carlos M. R. Rocha received financial support from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement no. 894321. Ahren W. Jasper would like to acknowledge the U. S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences, under Contract Number DE-AC02-06CH11357.
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Breno R. L. Galvão designed the research. Data collection and electronic structure calculations were performed by Alexandre C. R. Gomes and Carlos M. R. Rocha. Ahren W. Jasper supervised the kinetics calculations. All authors contributed to the analysis and interpretation. The first draft of the manuscript was written by Alexandre C. R. Gomes and Breno R. L. Galvão and all authors commented, revised and approved the final manuscript.
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Gomes, A.C.R., Rocha, C.M.R., Jasper, A.W. et al. Formation of phosphorus monoxide through the \(\mathbf {P}(^{4}S)+\mathbf {O}_{\mathbf {2}}(^{3}\Sigma ^{-})\rightarrow \mathbf {O}(^{3}P)+\mathbf {PO}(^{2}\Pi )\) reaction. J Mol Model 28, 259 (2022). https://doi.org/10.1007/s00894-022-05242-4
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DOI: https://doi.org/10.1007/s00894-022-05242-4