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Thermal Rate Coefficients for the Astrochemical Process C + CH+ → C2+ + H by Ring Polymer Molecular Dynamics

  • Published:2016-12-09 Issue:50 Volume:120 Page:9887-9893
  • ISSN:1089-5639
  • Container-title:The Journal of Physical Chemistry A
  • language:en
  • Short-container-title:J. Phys. Chem. A

Author:

Rampino Sergio1ORCID,Suleimanov Yury V.23

Affiliation:

1. Scuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italia

2. Computation-based Science and Technology Research Center, Cyprus Institute, 20 Kavafi Street, Nicosia 2121, Cyprus

3. Department of Chemical Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, United States

Funder

European Research Council

Research Promotion Foundation

European Regional Development Fund

Publisher

American Chemical Society (ACS)

Subject

Physical and Theoretical Chemistry

Cited by 19 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Modeling the structure of the dayside Venusian ionosphere: Impacts of protonation and Coulomb interaction;Astronomy & Astrophysics;2024-05

2. Bibliography;Chemistry at the Frontier with Physics and Computer Science;2022

3. Towards complexity;Chemistry at the Frontier with Physics and Computer Science;2022

4. Assessing parameters for ring polymer molecular dynamics simulations at low temperatures: DH + H chemical reaction;Chemical Physics Letters;2021-06

5. Gas-Phase Formation and Isomerization Reactions of Cyanoacetaldehyde, a Prebiotic Molecule of Astrochemical Interest;ACS Earth and Space Chemistry;2021-05-11
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