Solid-State Methylamine VUV Irradiation Study Using Carbon Monoxide as an H Radical Scavenger

被引:18
作者
Bossa, Jean-Baptiste [1 ]
Borget, Fabien [1 ]
Duvernay, Fabrice [1 ]
Danger, Gregoire [1 ]
Theule, Patrice [1 ]
Chiavassa, Thierry [1 ]
机构
[1] Aix Marseille Univ, CNRS, Ctr St Jerome, UMR 6633, F-13397 Marseille 20, France
关键词
INTERSTELLAR ICE ANALOGS; VACUUM ULTRAVIOLET PHOTOLYSIS; INFRARED SPECTRUM; PHOTOCHEMICAL FORMATION; LOW-TEMPERATURE; AMINO-ACIDS; GLYCINE; FORMAMIDE; COMETARY; AMMONIA;
D O I
10.1071/CH11409
中图分类号
O6 [化学];
学科分类号
0703 ;
摘要
Solid-phase methylamine (CH3NH2) was vacuum ultraviolet (VUV) photoprocessed at low temperature (20 K) using a hydrogen flow discharge lamp, which allows irradiation down to 120 nm. Methanimine (CH2=NH), the methylammonium cation (CH3NH3+) and the counterion CN, as well as the amino radical (NH2), methane (CH4) and ammonia (NH3), were identified as the photoproducts by using FTIR spectroscopy. So far, the branching ratios of the photodissociation pathways of methylamine in the solid phase remain unknown. The methylamine molecule holds two non-equivalent hydrogen atoms on the methyl and the amino group, so we can expect the formation of two distinct radicals via a carbon-hydrogen or a nitrogen-hydrogen bond cleavage, namely CH2NH2 and CH3NH. These radicals are highly reactive and may reform methylamine with hydrogen atom recombination. Their direct infrared spectroscopic detection is therefore tricky. To solve that problem, we use carbon monoxide (CO) as an H radical scavenger, forming the intermediate species HCO. After the irradiation of a CH3NH2 : CO binary ice mixture, formamide (NH2CHO) and N-methylformamide (CH3NHCHO) were identified as the main photoproducts using both infrared and mass spectrometry. We give a rough approximation of the branching ratios, which are in agreement with previous studies in the gas phase.
引用
收藏
页码:129 / 137
页数:9
相关论文
共 49 条
[1]  
[Anonymous], 1963, SPECTROMETRIC IDENTI
[2]   The formation of acetic acid (CH3COOH) in interstellar ice analogs [J].
Bennett, Chris J. ;
Kaiser, Ralf I. .
ASTROPHYSICAL JOURNAL, 2007, 660 (02) :1289-1295
[3]   A combined experimental and computational investigation on the synthesis of acetaldehyde [CH3CHO(X1A′)] in interstellar ices [J].
Bennett, CJ ;
Jamieson, CS ;
Osamura, Y ;
Kaiser, RI .
ASTROPHYSICAL JOURNAL, 2005, 624 (02) :1097-1115
[4]   ORGANIC-COMPOUNDS PRODUCED BY PHOTOLYSIS OF REALISTIC INTERSTELLAR AND COMETARY ICE ANALOGS CONTAINING METHANOL [J].
BERNSTEIN, MP ;
SANDFORD, SA ;
ALLAMANDOLA, LJ ;
CHANG, S ;
SCHARBERG, MA .
ASTROPHYSICAL JOURNAL, 1995, 454 (01) :327-344
[5]  
Bockelée-Morvan D, 2000, ASTRON ASTROPHYS, V353, P1101
[6]   Methylammonium methylcarbamate thermal formation in interstellar ice analogs: a glycine salt precursor in protostellar environments [J].
Bossa, J. -B. ;
Duvernay, F. ;
Theule, P. ;
Borget, F. ;
d'Hendecourt, L. ;
Chiavassa, T. .
ASTRONOMY & ASTROPHYSICS, 2009, 506 (02) :601-608
[7]   Formation of neutral methylcarbamic acid (CH3NHCOOH) and methylammonium methylcarbamate [CH3NH3+][CH3NHCO2-] at low temperature [J].
Bossa, Jean-Baptiste ;
Borget, Fabien ;
Duvernay, Fabrice ;
Theule, Patrice ;
Chiavassa, Thierry .
JOURNAL OF PHYSICAL CHEMISTRY A, 2008, 112 (23) :5113-5120
[8]   How a usual carbamate can become an unusual intermediate: a new chemical pathway to form glycinate in the interstellar medium [J].
Bossa, Jean-Baptiste ;
Borget, Fabien ;
Duvernay, Fabrice ;
Theule, Patrice ;
Chiavassa, Thierry .
JOURNAL OF PHYSICAL ORGANIC CHEMISTRY, 2010, 23 (04) :333-339
[9]   An infrared study of pure and ion irradiated frozen formamide [J].
Brucato, J. R. ;
Baratta, G. A. ;
Strazzulla, G. .
ASTRONOMY & ASTROPHYSICS, 2006, 455 (02) :395-399
[10]   THE INFRARED SPECTRA OF SOLID METHYLAMMONIUM HALIDES [J].
CABANA, A ;
SANDORFY, C .
SPECTROCHIMICA ACTA, 1962, 18 (06) :843-861