Literature DB >> 25903884

A comparative study of the Au + H₂, Au⁺ + H₂, and Au⁻ + H₂ systems: Potential energy surfaces and dynamics of reactive collisions.

Anaís Dorta-Urra1, Alexandre Zanchet2, Octavio Roncero2, Alfredo Aguado3.   

Abstract

In order to study the Au(-) + H2 collision, a new global potential energy surface (PES) describing the ground electronic state of AuH2(-) system is developed and compared with the PESs of the neutral [Zanchet et al., J. Chem. Phys. 132, 034301 (2010)] and cationic systems [Anaís et al., J. Chem. Phys. 135, 091102 (2011)]. We found that Au(-) - H2 presents a H-Au-H insertion minimum attributed to the stabilization of the LUMO 3b2 orbital, which can be considered as the preamble of the chemisorption well appearing in larger gold clusters. While the LUMO orbital is stabilized, the HOMO 6a1 is destabilized, creating a barrier at the geometry where the energy orbitals' curves are crossing. In the anion, this HOMO is doubly occupied, while in the neutral system is half-filled and completely empty in the cation, explaining the gradual disappearance of the well and the barrier as the number of electrons decreases. The cation presents a well in the entrance channel partially explained by electrostatic interactions. The three systems' reactions are highly endothermic, by 1.66, 2.79, and 3.23 eV for AuH, AuH(+), and AuH(-) products, respectively. The reaction dynamics is studied using quasi-classical trajectory method for the three systems. The one corresponding to the anionic system is new in this work. Collision energies between 1.00 and 8.00 eV, measured for the cation, are in good agreement with the simulated cross section for the AuH(+). It was also found that the total fragmentation, in three atoms, competes becoming dominant at sufficiently high energy. Here, we study the competition between the two different reaction pathways for the anionic, cationic, and neutral species, explaining the differences using a simple model based on the topology of the potential energy surfaces.

Entities:  

Year:  2015        PMID: 25903884     DOI: 10.1063/1.4916615

Source DB:  PubMed          Journal:  J Chem Phys        ISSN: 0021-9606            Impact factor:   3.488


  6 in total

1.  Full dimensional potential energy surface and low temperature dynamics of the H2CO + OH → HCO + H2O reaction.

Authors:  Alexandre Zanchet; Pablo Del Mazo; Alfredo Aguado; Octavio Roncero; Elena Jiménez; André Canosa; Marcelino Agúndez; José Cernicharo
Journal:  Phys Chem Chem Phys       Date:  2018-02-21       Impact factor: 3.676

2.  Gas phase Elemental abundances in Molecular cloudS (GEMS): I. The prototypical dark cloud TMC 1.

Authors:  A Fuente; D G Navarro; P Caselli; M Gerin; C Kramer; E Roueff; T Alonso-Albi; R Bachiller; S Cazaux; B Commercon; R Friesen; S García-Burillo; B M Giuliano; J R Goicoechea; P Gratier; A Hacar; I Jiménez-Serra; J Kirk; V Lattanzi; J C Loison; J Malinen; N Marcelino; R Martín-Doménech; G Muñoz-Caro; J Pineda; M Tafalla; B Tercero; D Ward-Thompson; S P Treviño-Morales; P Riviére-Marichalar; O Roncero; T Vidal; Maikel Y Ballester
Journal:  Astron Astrophys       Date:  2019-04-19       Impact factor: 5.802

3.  Is the gas-phase OH+H2CO reaction a source of HCO in interstellar cold dark clouds? A kinetic, dynamic and modelling study.

Authors:  A J Ocaña; E Jiménez; B Ballesteros; A Canosa; M Antiñolo; J Albaladejo; M Agúndez; J Cernicharo; A Zanchet; P Del Mazo; O Roncero; A Aguado
Journal:  Astrophys J       Date:  2017-11-14       Impact factor: 5.874

4.  Formation and Destruction of SiS in Space.

Authors:  Alexandre Zanchet; Octavio Roncero; Marcelino Agúndez; José Cernicharo
Journal:  Astrophys J       Date:  2018-07-20       Impact factor: 5.874

5.  Quantum and quasi-classical calculations for the S⁺ + H₂(v,j) → SH⁺(v',j') + H reactive collisions.

Authors:  Alexandre Zanchet; Octavio Roncero; Niyazi Bulut
Journal:  Phys Chem Chem Phys       Date:  2016-04-28       Impact factor: 3.676

6.  Ionization fraction and the enhanced sulfur chemistry in Barnard 1.

Authors:  A Fuente; J Cernicharo; E Roueff; M Gerin; J Pety; N Marcelino; R Bachiller; B Lefloch; O Roncero; A Aguado
Journal:  Astron Astrophys       Date:  2016-09-29       Impact factor: 5.802

  6 in total

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