The energetics for hydrogen addition to naphthalene cations

被引:15
作者
Ricca, Alessandra
Bakes, E. L. O.
Bauschlicher, Charles W., Jr.
机构
[1] SETI Inst, Mountain View, CA 94043 USA
[2] NASA Ames Res Ctr, Space Technol Div, Moffett Field, CA 94035 USA
关键词
astrochemistry; ISM : molecules; methods : numerical; molecular processes;
D O I
10.1086/512037
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Energetics of H-addition reactions to the naphthalene cation are determined using computational chemistry techniques. While most of the reactions have little to no barrier, the shape of the potential energy surfaces favors the formation of the product with the added hydrogen atoms being on adjacent carbons. Thus, while many products will be formed, one expects that the product in which all the hydrogen atoms are added to the same or adjacent rings will be favored over a random distribution of added hydrogen atoms. This has implications on the species that will be formed when polycyclic aromatic hydrocarbons (PAHs) are photolyzed in ices in the interstellar medium ( ISM). Barrierless reactions are consistent with the view that PAHs with extra hydrogens contribute to the 3.4 mu m band.
引用
收藏
页码:858 / 861
页数:4
相关论文
共 22 条
[1]   DENSITY-FUNCTIONAL THERMOCHEMISTRY .3. THE ROLE OF EXACT EXCHANGE [J].
BECKE, AD .
JOURNAL OF CHEMICAL PHYSICS, 1993, 98 (07) :5648-5652
[2]  
Bernstein M. P., 1996, APJ, V472, P127
[3]   UV irradiation of polycyclic aromatic hydrocarbons in ices: Production of alcohols, quinones, and ethers [J].
Bernstein, MP ;
Sandford, SA ;
Allamandola, LJ ;
Gillette, JS ;
Clemett, SJ ;
Zare, RN .
SCIENCE, 1999, 283 (5405) :1135-1138
[4]   Side group addition to the polycyclic aromatic hydrocarbon coronene by proton irradiation in cosmic ice analogs [J].
Bernstein, MP ;
Moore, MH ;
Elsila, JE ;
Sandford, SA ;
Allamandola, LJ ;
Zare, RN .
ASTROPHYSICAL JOURNAL, 2003, 582 (01) :L25-L29
[5]   Side group addition to the polycyclic aromatic hydrocarbon coronene by ultraviolet photolysis in cosmic ice analogs [J].
Bernstein, MP ;
Elsila, JE ;
Dworkin, JP ;
Sandford, SA ;
Allamandola, LJ ;
Zare, RN .
ASTROPHYSICAL JOURNAL, 2002, 576 (02) :1115-1120
[6]  
DEMUIZON MJ, 1990, ASTRON ASTROPHYS, V235, P367
[7]   Laboratory and theoretical simulation of 3.4 μm spectra of hydrocarbons in interstellar sources [J].
Duley, WW ;
Grishko, VI ;
Kenel, J ;
Lee-Dadswell, G ;
Scott, A .
ASTROPHYSICAL JOURNAL, 2005, 626 (02) :933-939
[8]   Solvent effects .5. Influence of cavity shape, truncation of electrostatics, and electron correlation ab initio reaction field calculations [J].
Foresman, JB ;
Keith, TA ;
Wiberg, KB ;
Snoonian, J ;
Frisch, MJ .
JOURNAL OF PHYSICAL CHEMISTRY, 1996, 100 (40) :16098-16104
[9]   FORMATION OF POLYCYCLIC AROMATIC-HYDROCARBONS IN CIRCUMSTELLAR ENVELOPES [J].
FRENKLACH, M ;
FEIGELSON, ED .
ASTROPHYSICAL JOURNAL, 1989, 341 (01) :372-384
[10]  
Frisch M. J., 2016, J AM CHEM SOC, DOI DOI 10.1021/JA205566W