Amino Acid Chiral Selection Via Weak Interactions in Stellar Environments: Implications for the Origin of Life

Abstract

Magnetochiral phenomena may be responsible for the selection of chiral states of biomolecules in meteoric environments. For example, the Supernova Amino Acid Processing (SNAAP) Model was proposed previously as a possible mode of magnetochiral selection of amino acids by way of the weak interaction in strong magnetic fields. In earlier work, this model was shown to produce an enantiomeric excess (ee) as high as 0.014% for alanine. In this paper we present the results of molecular quantum chemistry calculations from which $ee$s are determined for the alpha-amino acids plus isovaline and norvaline, which were found to have positive ees in meteorites. Calculations are performed for both isolated and aqueous states. In some cases, the aqueous state was found to produce larger $ee$s reaching values as high as a few percent under plausible conditions.

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Cited by in corpus (3)

• Chiral Selection, Isotopic Abundance Shifts, and Autocatalysis of Meteoritic Amino Acids
• Explaining the Variations in Isotopic Ratios in Meteoritic Amino Acids
• Single-Crystal NMR for 17O in Alanine Enantiomers