Formation of C4H4 from photolysis of icy C2H2 with 175 nm at 60 K

被引:1
作者
Lo, Jen-Iu [1 ]
Peng, Yu-Chain [1 ]
Chou, Sheng-Lung [2 ]
Lu, Hsiao-Chi [2 ]
Cheng, Bing-Ming [1 ,3 ]
机构
[1] Hualien Tzu Chi Hosp, Buddhist Tzu Chi Med Fdn, Dept Med Res, 707 Sec 3,Chung Yang Rd, Hualien 970, Taiwan
[2] Natl Synchrotron Radiat Res Ctr, 101 Hsin Ann Rd,Hsinchu Sci Pk, Hsinchu 300, Taiwan
[3] Tzu Chi Univ Sci & Technol, 880 Sec 2,Chien Kuo Rd, Hualien 970, Taiwan
关键词
astrochemistry; molecular processes; methods: laboratory: solid state; ISM: molecules; infrared: ISM; INFRARED-ABSORPTION SPECTRA; COSMIC-RAY PARTICLES; VACUUM-ULTRAVIOLET; CROSS-SECTIONS; INTERSTELLAR ICES; CARBON CLUSTERS; ION IRRADIATION; HIGH-RESOLUTION; ACETYLENE; PHOTODISSOCIATION;
D O I
10.1093/mnras/staa2756
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The absorption spectrum of solid acetylene (C2H2) at 10 K was measured in wavelength range 107-250 nm with UV light from a synchrotron source. Based on the absorption spectrum, we irradiated at 175 nm the icy acetylene at 60 K; the results yielded a new set of IR absorption lines with similar temporal profiles of production during the photolysis periods. From icy (C2H2)-C-12, these new features were recorded at 3276.8, 1598.7, 963.0, 936.3, and 671.3 cm(-1), which are assigned to modes nu(1), nu(6), nu(14), nu(15), and nu(11) (mixing with nu(17)), respectively, of vinylacetylene (C4H4) based on the results of C-13- and D-isotopic experiments and quantum-chemical calculations. These calculations using density-functional theory (B3LYP/6-311++G**) predict vibrational wavenumbers and IR intensities of vinylacetylene that agree satisfactorily with our experimental results. This work enhances our understanding of the photochemistry of icy acetylene in cold astronomical environments; for instance, the present result can be applied directly to the photochemical processes on Titan's surface.
引用
收藏
页码:543 / 549
页数:7
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