Infrared analysis of Glycine dissociation by MeV ions and keV electrons
Abstract Knowledge on amino acid's dissociation rates by solar wind is relevant for the study of biomaterial resistance in space. The radiolysis and sputtering of glycine by 1 keV electron beam and by 1.8 MeV H+, 1.5 MeV He+ and 1.5 MeV N+ ion beams are studied in laboratory, at room temperature. The column density decrease rates due to each beam are measured via infrared spectroscopy and destruction cross sections are determined. Present results stand in good agreement with those found in the literature and show that over five orders of magnitude, apparent destruction cross sections (which includes sputtering), σdap, are approximately proportional to the electronic stopping power, Se, that is (σdap ≈ a Se), where 1/a ≈ 120 eV/nm3. This value corresponds to the mean absorbed energy density necessary to dissociate (and/or eject) glycine; it also suggests that the stopping power threshold for molecular destruction is 23 keV μm−1. Assuming σdap = a Se for electron and ion projectiles, the half-life of pure α-glycine is estimated for the solar wind processing at 1 AU: about 10 days for protons or electrons and 40 days for He ions.