Endo or Exo? Structures of Gas-Phase Alkali Metal Cation/Aromatic Half-Belt Complexes

被引:4
作者
Chen, Yanyang [1 ]
Jami-Alahmadi, Yasaman [1 ]
Unikela, Kiran Sagar [1 ]
Bodwell, Graham J. [1 ]
Fridgen, Travis D. [1 ]
机构
[1] Mem Univ, Mem Univ Newfoundland, Dept Chem, St John, NF A1B 3X7, Canada
基金
加拿大自然科学与工程研究理事会; 加拿大创新基金会;
关键词
blackbody infrared radiative dissociation; cyclophane; host-guest complexes; IRMPD spectroscopy; mass spectrometry; NONPLANAR AROMATIC-COMPOUNDS; INFRARED RADIATIVE DISSOCIATION; PI-ELECTRON DELOCALIZATION; CROWN-ETHER COMPLEXES; HOST-GUEST CHEMISTRY; PROTON-BOUND DIMERS; SUPRAMOLECULAR CHEMISTRY; MOLECULAR RECOGNITION; BICYCLIC CYCLOPHANE; HYDROGEN-BONDS;
D O I
10.1002/cphc.201800371
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
1,1,9,9-Tetramethyl[9](2,11)teropyrenophane (TM9TP), a belt-shaped molecule, has a sizable cavity that molecules or ions could occupy. In this study, the question of whether TM9TP forms gas-phase ion-molecule complexes with metal cations (K+, Rb+, Cs+) situated inside or outside the TM9TP cavity was addressed using both experimental and computational methods. Complexes were trapped in a Fourier transform ion cyclotron resonance mass spectrometer and their structures were explored by some novel physical chemistry/mass spectrometry methods. Blackbody infrared radiative dissociation kinetics reveal two populations of ions, a fast dissociating fraction and a persistent fraction. Infrared multiphoton dissociation spectra (vibrational spectra) provide very strong evidence that the most abundant population is a complex where the metal cation is inside the TM9TP cavity, endo-TM9TP. Red-shifted C-H stretching bands present in the gas-phase vibrational spectra of these ionic complexes show that there is an interaction between the metal cation and bridge C-H bonds due to the cation sitting inside the cavity of TM9TP. B3LYP/6-31+G(d,p) calculations showed the endo complexes to be the lowest in energy; about 60kJmol(-1) more thermodynamically stable and more than 120kJmol(-1) kinetically more stable than the exo complex.
引用
收藏
页码:2194 / 2199
页数:6
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