Detecting chiral asymmetry in the interstellar medium using propylene-oxide
Boy Lankhaar

TL;DR
This paper models circular dichroism in propylene-oxide to assess the feasibility of detecting molecular chirality in the interstellar medium, concluding current astronomical methods are insufficient but laboratory spectroscopy could succeed.
Contribution
It develops a theoretical model of circular dichroism in chiral molecules' microwave transitions, specifically applied to propylene-oxide, to guide detection strategies in space and laboratory settings.
Findings
Predicted circular polarization fractions are around 10^(-6).
Detection of enantiomeric excess in ISM with current techniques is unlikely.
Laboratory microwave dichroism spectroscopy may detect propylene-oxide chirality.
Abstract
(Abridged) Life is distinctly homochiral. The origins of this homochirality are under active debate. Recently, propylene-oxide has been detected in the gas-phase interstellar medium (ISM) (McGuire et al. 2016). The enantiomeric composition of ISM propylene-oxide may be probed through circular polarization measurements, but accurate estimates of the circular dichroism properties of the microwave transitions of propylene-oxide are not available. We develop a model of the circular dichroic activity in torsion-rotation transitions of closed-shell chiral molecules, such as propylene-oxide. With this model, we estimate the viability, and optimize observation strategies, of enantiomeric excess detection in ISM propylene-oxide. We present estimates for the dichroic activity of the torsion-rotation transitions of propylene-oxide, where we predict that the circular polarization fractions of…
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