β-Heterosubstituted Acrylonitriles - Electronic Structure Study by UV-Photoelectron Spectroscopy and Quantum Chemical Calculations

被引:19
作者
Chrostowska, Anna [1 ]
Nguyen, Thi Xuan Mai [1 ]
Dargelos, Alain [1 ]
Khayar, Said [1 ]
Graciaa, Alain [2 ]
Guillemin, Jean-Claude [3 ]
机构
[1] Univ Pau & Pays Adour, Inst pluridisciplinaire Rech Environm & Mat, CNRS, UMR 5254, F-64000 Pau, France
[2] Univ Pau & Pays Adour, Lab Fluides Complexes, CNRS, UMR 5150, F-64000 Pau, France
[3] Ecole Natl Super Chim Rennes, CNRS, F-35708 Rennes, France
关键词
MICROWAVE-SPECTRUM; PREBIOTIC SYNTHESIS; TITANS ATMOSPHERE; GAS-PHASE; MOLECULES; NITRILES; CROTONONITRILE; CYANOACETYLENE; DEPROTONATION; DERIVATIVES;
D O I
10.1021/jp8087447
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
beta-Heterosubstituted acrylonitriles correspond to the formal addition of nucleophiles on cyanoacetylene, Acrylonitriles substituted with an amino, methoxy, mercapto group, or halogeno atom have been synthesized. Rearrangements between Z and E stereoisomers or tautomerizations have been studied by NMR spectroscopy and by quantum calculations. The photoelectron spectra were recorded and analyzed with the aid or a time-dependent density functional theory, ab initio OVGF, and so-called "corrected" ionization energy calculations. The electronic structure of the studied species was determined, and strong differences between beta-heterosubstituted acrylonitriles and the corresponding nitrile-free heteroalkenes were clearly documented. A "push-pull" effect was noticed, due to the combined donor effect of the substituent on one side of the carbon-carbon double bond and the electron-withdrawing effect of the nitrile group on the other side. Thus, the presence of a nitrile group strongly stabilizes the electronic structure. The efficient pi-donor contribution of the NH(2) and SH groups was evidenced.
引用
收藏
页码:2387 / 2396
页数:10
相关论文
共 30 条
  • [1] Microwave spectrum, structure, and quantum chemical studies of a compound of potential astrochemical and astrobiological interest:: Z-3-amino-2-propenenitrile
    Askeland, Eva
    Mollendal, Harald
    Uggerud, Einar
    Guillemin, Jean-Claude
    Moreno, Juan-Ramon Aviles
    Demaison, Jean
    Huet, Therese R.
    [J]. JOURNAL OF PHYSICAL CHEMISTRY A, 2006, 110 (46) : 12572 - 12584
  • [3] Infrared spectra of a species of astrochemical interest:: Aminoacrylonitrile (3-amino-2-propenenitrile)
    Benidar, A
    Guillemin, JC
    Mó, O
    Yáñez, M
    [J]. JOURNAL OF PHYSICAL CHEMISTRY A, 2005, 109 (21) : 4705 - 4712
  • [4] Charnley S, 2003, PHYS WORLD, V16, P35
  • [5] Cheikh A.Ben., 1991, J ORG CHEM, V56, P970
  • [6] ETHENETHIOL AND 1-PROPENE-1-THIOL - A PHOTOELECTRON SPECTROSCOPIC STUDY
    CHIN, WS
    MOK, CY
    HUANG, HH
    [J]. JOURNAL OF ELECTRON SPECTROSCOPY AND RELATED PHENOMENA, 1994, 67 (01) : 173 - 179
  • [7] Synthesis and characterization of (E)- and (Z)-3-mercapto-2-propenenitrile.: Microwave spectrum of the Z-isomer
    Cole, George C.
    Mollendal, Harald
    Khater, Brahim
    Guillemin, Jean-Claude
    [J]. JOURNAL OF PHYSICAL CHEMISTRY A, 2007, 111 (07) : 1259 - 1264
  • [8] Experimental laboratory simulation of Titan's atmosphere:: aerosols and gas phase
    Coll, P
    Coscia, D
    Smith, N
    Gazeau, MC
    Ramírez, SI
    Cernogora, G
    Israël, G
    Raulin, F
    [J]. PLANETARY AND SPACE SCIENCE, 1999, 47 (10-11) : 1331 - 1340
  • [9] MODELING TITANS THERMAL INFRARED-SPECTRUM FOR HIGH-RESOLUTION SPACE OBSERVATIONS
    COUSTENIS, A
    ENCRENAZ, T
    BEZARD, B
    BJORAKER, G
    GRANER, G
    DANGNHU, M
    ARIE, E
    [J]. ICARUS, 1993, 102 (02) : 240 - 260
  • [10] EXPERIMENTAL SIMULATION OF TITANS ORGANIC-CHEMISTRY AT LOW-TEMPERATURE
    DEVANSSAY, E
    GAZEAU, MC
    GUILLEMIN, JC
    RAULIN, F
    [J]. PLANETARY AND SPACE SCIENCE, 1995, 43 (1-2) : 25 - 31