Abstract
The formation of deuterated interstellar molecules is considered. This contribution (which, in the summarizing remarks of the conference, was admonished for being itself admonitory) has a simple purpose—to apply gas-phase ion chemistry to distinguish deuterium exchange reactions that can occur from those that cannot. Thus the exoergic reaction HCO+ + D → DCO+ + H is facile whereas the exoergic reaction HCO+ + HD —×→ DCO+ + H2 is not. Forbidden pathways involve energy barriers that can result from both reactants showing filled valence electron shells. A procedure is outlined for identifying such.
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Henchman, M., Smith, D., Adams, N., Paulson, J.F., Lindinger, W. (1988). Chemical Pathways for Deuterium Fractionation in Interstellar Molecules. In: Millar, T.J., Williams, D.A. (eds) Rate Coefficients in Astrochemistry. Astrophysics and Space Science Library, vol 146. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3007-0_13
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DOI: https://doi.org/10.1007/978-94-009-3007-0_13
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