Rate coefficients for the reactions of C(3PJ) atoms with C2H2, C2H4, CH3C=CHand H2C=C=CH2 at temperatures down to 15 K

被引:85
作者
Chastaing, D [1 ]
Le Picard, SD [1 ]
Sims, IR [1 ]
Smith, IWM [1 ]
机构
[1] Univ Birmingham, Sch Chem, Birmingham B15 2TT, W Midlands, England
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 365卷 / 02期
关键词
molecular data; molecular processes; methods : laboratory; ISM : clouds;
D O I
10.1051/0004-6361:20000026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Rate coefficients for the reactions of ground state carbon atoms, C(P-3(J)), With the four unsaturated hydrocarbons C2H2, C2H4, CH3C = CH and H2C = C = CH2 have been measured at temperatures down to 15 K. The experiments have been performed in a continuous Row CRESU (Cinetique de Reaction en Ecoulement Supersonique Uniforme) apparatus using pulsed laser photolysis of C3O2 to generate C(P-3(J)) atoms and laser-induced fluorescence in the vacuum ultraviolet to observe the kinetic decays of the atoms and hence deter mine the rate coefficients. All four reactions are found to occur at rates close to the collision-determined limit and the rates show at most a very mild dependence on temperature. It is argued that normally these reactions proceed along a reaction path with no barrier to form a strongly bound energised adduct, which subsequently eliminates an H atom to form the reaction products. The rates of the reactions of C(P-3(J)) atoms with larger unsaturated hydrocarbons are discussed. Finally, the relevance of the results for the chemistry of dense interstellar clouds is considered.
引用
收藏
页码:241 / 247
页数:7
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共 37 条
[1]   ABUNDANCES OF THE ELEMENTS - METEORITIC AND SOLAR [J].
ANDERS, E ;
GREVESSE, N .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1989, 53 (01) :197-214
[2]   The formation of large hydrocarbons and carbon clusters in dense interstellar clouds [J].
Bettens, RPA ;
Herbst, E .
ASTROPHYSICAL JOURNAL, 1997, 478 (02) :585-593
[3]   THE IMPORTANCE OF CLASSES OF NEUTRAL-NEUTRAL REACTIONS IN THE PRODUCTION OF COMPLEX INTERSTELLAR-MOLECULES [J].
BETTENS, RPA ;
LEE, HH ;
HERBST, E .
ASTROPHYSICAL JOURNAL, 1995, 443 (02) :664-674
[4]  
BUONOMO E, 2000, COMMUNICATION
[5]  
Canosa A, 1997, ASTRON ASTROPHYS, V323, P644
[6]  
CANOSA A, 2000, IN PRESS
[7]   The abundance of interstellar carbon [J].
Cardelli, JA ;
Meyer, DM ;
Jura, M ;
Savage, BD .
ASTROPHYSICAL JOURNAL, 1996, 467 (01) :334-340
[8]   Neutral-neutral reactions at the temperatures of interstellar clouds:: Rate coefficients for reactions of atomic carbon, C(3P), with O2, C2H2, C2H4 and C3H6 down to 15 K [J].
Chastaing, D ;
James, PL ;
Sims, IR ;
Smith, IWM .
PHYSICAL CHEMISTRY CHEMICAL PHYSICS, 1999, 1 (09) :2247-2256
[9]   Direct kinetic measurements on reactions of atomic carbon, C(3P), with O2 and NO at temperatures down to 15 K [J].
Chastaing, D ;
Le Picard, SD ;
Sims, IR .
JOURNAL OF CHEMICAL PHYSICS, 2000, 112 (19) :8466-8469
[10]   Neutral-neutral reactions at the temperatures sf interstellar clouds -: Rate coefficients for reactions of C2H radicals with O2, C2H2, C2H4 and C3H6 down to 15 K [J].
Chastaing, D ;
James, PL ;
Sims, IR ;
Smith, IWM .
FARADAY DISCUSSIONS, 1998, 109 :165-181