The origin of the E/Z isomer ratio of imines in the interstellar medium
Juan Garc\'ia de la Concepci\'on, Izaskun Jim\'enez-Serra, Jos\'e, Carlos Corchado, V\'ictor M. Rivilla, and Jes\'us Mart\'in-Pintado

TL;DR
This study shows that quantum tunneling enables E-Z isomerization of imines in space, explaining observed abundance ratios by considering multidimensional tunneling effects at low temperatures.
Contribution
It introduces a multidimensional small curvature tunneling model to explain E-Z isomer ratios of imines in the interstellar medium, challenging previous assumptions about high energy barriers.
Findings
Tunneling enables isomerization at low temperatures (~150 K).
Predicted E/Z ratios match astronomical observations.
Isomer ratios depend on relative stability in space.
Abstract
Recent astronomical observations of both isomers E and Z of imines such as cyanomethanimine, ethanimine and 2-propyn-1-imine, have revealed that the abundances in the ISM of these isomers differ by factors of ~3-10. Several theories have been proposed to explain the observed behavior, but none of them successfully explains the [E]/[Z] ratios. In this work we present a detailed study of the kinetics of the one-step E-Z isomerization reactions of cyanomethanimine, ethanimine and 2-propyn-1-imine under interstellar conditions (in the 10-400 K temperature range). This reaction was previously thought to be non-viable in the ISM due to its associated high-energy barrier (about 13,000 K). In this Letter, we show that considering the multidimensional small curvature tunneling approximation, the tunneling effect enables the isomerization even at low temperatures. This is due to the fact that the…
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