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Valine Radiolysis by H+, He+, N+, and S15+ MeV Ions.


ABSTRACT: Radiolysis of biomolecules by fast ions has interest in medical applications and astrobiology. The radiolysis of solid D-valine (0.2-2 ?m thick) was performed at room temperature by 1.5 MeV H+, He+, N+, and 230 MeV S15+ ion beams. The samples were prepared by spraying/dropping valine-water-ethanol solution on ZnSe substrate. Radiolysis was monitored by infrared spectroscopy (FTIR) through the evolution of the intensity of the valine infrared 2900, 1329, 1271, 948, and 716 cm-1 bands as a function of projectile fluence. At the end of sample irradiation, residues (tholins) presenting a brownish color are observed. The dependence of the apparent (sputtering + radiolysis) destruction cross section, ?d, on the beam stopping power in valine is found to follow the power law ?d = aSen, with n close to 1. Thus, ?d is approximately proportional to the absorbed dose. Destruction rates due to the main galactic cosmic ray species are calculated, yielding a million year half-life for solid valine in space. Data obtained in this work aim a better understanding on the radioresistance of complex organic molecules and formation of radioproducts.

SUBMITTER: Costa CAPD 

PROVIDER: S-EPMC7084508 | biostudies-literature | 2020 Mar

REPOSITORIES: biostudies-literature

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Valine Radiolysis by H<sup>+</sup>, He<sup>+</sup>, N<sup>+</sup>, and S<sup>15+</sup> MeV Ions.

Costa Cíntia A P da CAPD   Muniz Gabriel S Vignoli GSV   Boduch Philippe P   Rothard Hermann H   Silveira Enio F da EFD  

International journal of molecular sciences 20200310 5


Radiolysis of biomolecules by fast ions has interest in medical applications and astrobiology. The radiolysis of solid D-valine (0.2-2 μm thick) was performed at room temperature by 1.5 MeV H<sup>+</sup>, He<sup>+</sup>, N<sup>+</sup>, and 230 MeV S<sup>15+</sup> ion beams. The samples were prepared by spraying/dropping valine-water-ethanol solution on ZnSe substrate. Radiolysis was monitored by infrared spectroscopy (FTIR) through the evolution of the intensity of the valine infrared 2900, 1329  ...[more]

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