Ab initio studies on cyanoacetylenes of astrochemical interest: [Y(C≡C)CN, Y = C2H5, C3H7, C4H9, F, Cl, Br and CN]

被引：2

作者：

Ramanah, D. Kodi ^{[1
,2
]}

Surajbali, P. ^{[1
,2
]}

Rhyman, L. ^{[1
]}

Alswaidan, I. A. ^{[3
]}

Fun, H. -K. ^{[3
,4
]}

Somanah, R. ^{[2
]}

Ramasami, P. ^{[1
,3
]}

机构：

[1] Univ Mauritius, Dept Chem, Computat Chem Grp, Fac Sci, Reduit 80837, Mauritius

[2] Univ Mauritius, Dept Phys, Fac Sci, Reduit 80837, Mauritius

[3] King Saud Univ, Coll Pharm, Dept Pharmaceut Chem, Riyadh 11451, Saudi Arabia

[4] Univ Sains Malaysia, Sch Phys, Xray Crystallog Unit, George Town 11800, Malaysia

来源：

NEW ASTRONOMY | 2016年 / 42卷

关键词：

Cyanoacetylenes; Astromolecules; Density functional theory; Coupled cluster method; RAMAN-SPECTRA; INTERSTELLAR-MEDIUM; DICYANOACETYLENE; CHEMISTRY; IDENTIFICATION; PREDICTION; IRC+10216; MOLECULES; CONSTANTS; DISCOVERY;

D O I：

10.1016/j.newast.2015.07.001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Theoretical studies were performed on seven potential interstellar and circumstellar substituted cyanoacetylenes, Y(C equivalent to C)CN [Y = C2H5, C3H7, C4H9, F, Cl, Br and CN]. Geometry optimizations were carried out using the DFT/B3LYP, the CCSD and CCSD(T) levels of theory. The cc-pVTZ basis set was used for all atoms. Frequency computations were also carried out at the same level of theory as for the optimization to check the nature of the stationary points. The molecular and spectroscopic parameters of the cyanoacetylenes were computed. An analysis of these parameters is in line with the satisfactory performance of the B3LYP/cc-pVTZ level compared to the golden standard, the CCSD(T) level. The theoretical data reported in this work should facilitate future identifications of these cyanoacetylenes in extraterrestrial locations. Plausible mechanisms for the formation of these molecules have been proposed. (C) 2015 Elsevier B.V. All rights reserved.

引用

页码：42 / 48

页数：7

共 76 条

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