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      Surface Reaction of Methyl Mercaptan (CH 3SH) with Hydrogen Atoms on Amorphous Solid Water

      , , , , ,
      The Astrophysical Journal
      American Astronomical Society

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          Abstract

          Methyl mercaptan (CH 3SH) is one of the S-bearing organic compounds found in the interstellar medium (ISM). In this study, we investigated the surface reactions of solid CH 3SH with H atoms on amorphous solid water using experimental and computational methods to examine their physicochemical behavior in the ISM. Consequently, the primary product was discovered to be CH 4. As the computational studies show that the dominant reaction pathway is H + CH 3SH → CH 3 + H 2S, the observed CH 4 would result from H addition to CH 3. As relatively minor routes, the H abstraction processes from the –CH 3 and –SH functional groups of CH 3SH, giving rise to CH 2SH and CH 3S radicals, are confirmed. Although these radicals may form CH 3SH again by reactions with H atoms, the loss of CH 3SH from the ice surface by chemical desorption would be minor.

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          Balanced basis sets of split valence, triple zeta valence and quadruple zeta valence quality for H to Rn: Design and assessment of accuracy.

          Gaussian basis sets of quadruple zeta valence quality for Rb-Rn are presented, as well as bases of split valence and triple zeta valence quality for H-Rn. The latter were obtained by (partly) modifying bases developed previously. A large set of more than 300 molecules representing (nearly) all elements-except lanthanides-in their common oxidation states was used to assess the quality of the bases all across the periodic table. Quantities investigated were atomization energies, dipole moments and structure parameters for Hartree-Fock, density functional theory and correlated methods, for which we had chosen Møller-Plesset perturbation theory as an example. Finally recommendations are given which type of basis set is used best for a certain level of theory and a desired quality of results.
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            Long-range corrected hybrid density functionals with damped atom-atom dispersion corrections.

            We report re-optimization of a recently proposed long-range corrected (LC) hybrid density functional [J.-D. Chai and M. Head-Gordon, J. Chem. Phys., 2008, 128, 084106] to include empirical atom-atom dispersion corrections. The resulting functional, omegaB97X-D yields satisfactory accuracy for thermochemistry, kinetics, and non-covalent interactions. Tests show that for non-covalent systems, omegaB97X-D shows slight improvement over other empirical dispersion-corrected density functionals, while for covalent systems and kinetics it performs noticeably better. Relative to our previous functionals, such as omegaB97X, the new functional is significantly superior for non-bonded interactions, and very similar in performance for bonded interactions.
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                Author and article information

                Contributors
                Journal
                The Astrophysical Journal
                ApJ
                American Astronomical Society
                0004-637X
                1538-4357
                February 28 2023
                February 01 2023
                February 28 2023
                February 01 2023
                : 944
                : 2
                : 219
                Article
                10.3847/1538-4357/acafde
                151d851c-f8aa-4888-9127-61d9dc7582ff
                © 2023

                http://creativecommons.org/licenses/by/4.0/

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