Cyanonaphthalene and cyanonaphthyl radicals: Vibrational structures via computed negative ion photoelectron spectra and thermochemistry of 1-and 2-cyanonaphthalene

被引:0
作者
White, Nolan J. [1 ]
Vargas, Lucia A. [1 ,2 ]
Tunstall, Wyatt W. [1 ,2 ]
Abeysooriya, Dushmantha N. Koku Hannadige [1 ,3 ]
Gichuhi, Wilson K. [1 ]
机构
[1] Tennessee Technol Univ, Dept Chem, 1 William L Jones Dr, Cookeville, TN 38505 USA
[2] Tennessee Technol Univ, Dept Chem Engn, 1 William L Jones Dr, Cookeville, TN 38505 USA
[3] Tennessee Technol Univ, Sch Environm Studies, 1 William L Jones Dr, Cookeville, TN 38505 USA
关键词
POLYCYCLIC AROMATIC-HYDROCARBONS; INFRARED-SPECTRA; NAPHTHALENE; 1-CYANONAPHTHALENE; INTERSTELLAR; SPECTROSCOPY; ANIONS; WATER; SOOT; MOLECULES;
D O I
10.1063/5.0220823
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
A double harmonic oscillator model is applied to compute the negative ion photoelectron spectra (NIPES) of the 1- and 2-cyanonaphthalene (CNN) radical anions. The computed Franck-Condon factors utilize optimized structures and harmonic vibrational frequencies obtained using density functional theory with the B3LYP 6-311++G (2d,2p) basis set while considering the mode-mixing Duschinsky effects. To test the accuracy of our model, the NIPES of alpha and beta naphthyl radical anions were computed, and a strong agreement between the slow electron velocity-map ion imaging spectra and the predicted spectra was found. The adiabatic electron affinities (EAs) of the ground singlet states (S-0) in 1-CNN and 2-CNN are 0.856 and 0.798 eV, respectively. The origin of the lowest-lying triplet (T-1) states in 1-CNN and 2-CNN is found to be 3.226 and 3.266 eV, resulting in singlet-triplet energy splittings (Delta E-ST) of 2.370 and 2.468 eV, respectively. Both the NIPES for electron detachment to the S-0 and T-1 states exhibit well-resolved vibrational features, allowing for the assignment of several vibrational fundamental frequencies. Following deprotonation, several isomers are formed, with the most stable deprotonated radical anions in 1-CNN and 2-CNN, corresponding to the removal of the most acidic proton, with EAs of 2.062 and 2.16 eV. The rich spectroscopic and thermochemical data obtained in the current study make the CNN radical anions and their deprotonated species interesting systems for investigation in gas-phase, negative-ion experiments.
引用
收藏
页数:17
相关论文
共 78 条
[21]   Experimental and theoretical studies of the conformational structures of the mixed clusters of 1-cyanonaphthalene with water [J].
Fujiwara, T ;
Ramos, RC ;
Zgierski, MZ ;
Lim, EC .
JOURNAL OF CHEMICAL PHYSICS, 2005, 123 (24)
[22]   Projected CAP-EOM-CCSD method for electronic resonances [J].
Gayvert, James R. ;
Bravaya, Ksenia B. .
JOURNAL OF CHEMICAL PHYSICS, 2022, 156 (09)
[23]   The quest to uncover the nature of benzonitrile anion [J].
Gulania, Sahil ;
Jagau, Thomas-C. ;
Sanov, Andrei ;
Krylov, Anna I. .
PHYSICAL CHEMISTRY CHEMICAL PHYSICS, 2020, 22 (09) :5002-5010
[24]   A benchmark theoretical study of the electronic ground state and of the singlet-triplet split of benzene and linear acenes [J].
Hajgato, B. ;
Szieberth, D. ;
Geerlings, P. ;
De Proft, F. ;
Deleuze, M. S. .
JOURNAL OF CHEMICAL PHYSICS, 2009, 131 (22)
[25]   ELECTRON-AFFINITIES OF NAPHTHALENE, ANTHRACENE AND SUBSTITUTED NAPHTHALENES AND ANTHRACENES [J].
HEINIS, T ;
CHOWDHURY, S ;
KEBARLE, P .
ORGANIC MASS SPECTROMETRY, 1993, 28 (04) :358-365
[26]   CAN NEGATIVE MOLECULAR-IONS BE DETECTED IN DENSE INTER-STELLAR CLOUDS [J].
HERBST, E .
NATURE, 1981, 289 (5799) :656-657
[27]   Calculations on the formation rates and mechanisms for CnH anions in interstellar and circumstellar media [J].
Herbst, Eric ;
Osamura, Yoshihiro .
ASTROPHYSICAL JOURNAL, 2008, 679 (02) :1670-1679
[28]  
Homann KH, 1998, ANGEW CHEM INT EDIT, V37, P2435, DOI 10.1002/(SICI)1521-3773(19981002)37:18<2434::AID-ANIE2434>3.0.CO
[29]  
2-L
[30]   Resonance-stabilized hydrocarbon-radical chain reactions may explain soot inception and growth [J].
Johansson, K. O. ;
Head-Gordon, M. P. ;
Schrader, P. E. ;
Wilson, K. R. ;
Michelsen, H. A. .
SCIENCE, 2018, 361 (6406) :997-+