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

被引:13
|
作者
da Costa, Cintia A. P. [1 ]
Muniz, Gabriel S. Vignoli [2 ]
Boduch, Philippe [3 ]
Rothard, Hermann [3 ]
da Silveira, Enio F. [1 ]
机构
[1] Pontificia Univ Catolica Rio de Janeiro, Dept Phys, Rua Marques de Sao Vicente 225, BR-22451900 Rio De Janeiro, Brazil
[2] Univ Sao Paulo, Inst Phys, Rua Matao, BR-13710550 Sao Paulo, Brazil
[3] Normandie Univ, Ctr Rech Ions Mat & Photon, ENSICAEN, CEA,CNRS,CIMAP, F-14000 Caen, France
关键词
amino acid; valine; MeV ion irradiation; radiolysis; infrared absorption spectroscopy; destruction cross section; stopping power dependence; AMINO-ACIDS; COSMIC-RAY; INDUCED DESORPTION; CROSS-SECTIONS; GLYCINE; RADIATION; RADIORESISTANCE; BIOMOLECULES; COMPACTION; SEARCH;
D O I
10.3390/ijms21051893
中图分类号
Q5 [生物化学]; Q7 [分子生物学];
学科分类号
071010 ; 081704 ;
摘要
Radiolysis of biomolecules by fast ions has interest in medical applications and astrobiology. The radiolysis of solid D-valine (0.2-2 mu 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, sigma(d), on the beam stopping power in valine is found to follow the power law sigma(d) = aS(e)(n), with n close to 1. Thus, sigma(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.
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页数:21
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