An ab Initio Based Global Potential Energy Surface Describing CH5+ → CH3+ + H2
Author:
Affiliation:
1. Cherry L. Emerson Center of Scientific Computation and Department of Chemistry, Emory University, Atlanta, Georgia 30322
Publisher
American Chemical Society (ACS)
Subject
Physical and Theoretical Chemistry
Link
https://pubs.acs.org/doi/pdf/10.1021/jp053848o
Reference36 articles.
1. Deuteration of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{CH}\,^{+}_{n}$ \end{document} (n= 3–5) in Collisions with HD Measured in a Low‐Temperature Ion Trap
2. Enhanced Deuterium Fractionation in Dense Interstellar Cores Resulting from Multiply Deuterated H[FORMULA][F][SUP]+[/SUP][INF]3[/INF][/F][/FORMULA]
3. The importance of new rate coefficients for deuterium fractionation reactions in interstellar chemistry
4. Does CH 5+ prefer a C2vrather than a Csstructure?
5. CH+5: The never‐ending story or the final word?
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