The Calculated Infrared Spectra of Functionalized Hexamethylenetetramine (HMT) Molecules

被引:10
作者
Bera, Partha P. [1 ,2 ]
Sandford, Scott A. [1 ]
Lee, Timothy J. [3 ]
Nuevo, Michel [1 ,2 ]
机构
[1] NASA, Ames Res Ctr, MS 245-6, Moffett Field, CA 94035 USA
[2] NASA, Bay Area Environm Res Inst, Res Pk,MS 18-4, Moffett Field, CA 94035 USA
[3] NASA, Ames Res Ctr, MS 245-3, Moffett Field, CA 94035 USA
基金
美国国家航空航天局;
关键词
astrobiology; astrochemistry; ISM: molecules; methods: laboratory: molecular; methods: numerical; molecular processes; QUARTIC FORCE-FIELD; INTERSTELLAR ICE ANALOGS; AROMATIC HYDROCARBON CORONENE; SIDE-GROUP ADDITION; ULTRAVIOLET-IRRADIATION; AMINO-ACIDS; VIBRATIONAL FREQUENCIES; ORGANIC-COMPOUNDS; PREBIOTIC MOLECULES; UV-IRRADIATION;
D O I
10.3847/1538-4357/ab3c4f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Numerous laboratory studies have shown that exposure of mixed ices of astrophysical interest to ionizing radiation leads to the production of large numbers of new, more complex compounds. A significant portion of these new species appear to belong to a family of molecules that consist of hexamethylenetetramine (HMT; C(6)H(12)N4) and hexamethylenetetramine to which different functional side groups have been added. In this paper, we present the computed harmonic vibational infrared spectra of a number of HMT variants that include HMT-OH, HMT-NH2, HMT-CH3, HMT-CN, HMT-OCN, HMT-OCH3 HMT-CH(OH)CHO, and HMT-NHCHO. Since all of the members of this family share the common HMT framework as a major part of their structure, they produce a number of infrared bands that fall at similar positions and have similar strengths, which will make them easier to detect in space as a family. However, each molecular HMT variant also produces additional unique bands due to its attached side group, so it is possible to distinguish between different variants.
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页数:16
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