scholarly journals Examining the Influence of Anion Nucleophilicity on the Polymerisation Initiation Mechanism of Phenyl Glycidyl Ether

Polymers ◽  
2019 ◽  
Vol 11 (4) ◽  
pp. 657 ◽  
Author(s):  
Binks ◽  
Cavalli ◽  
Henningsen ◽  
Howlin ◽  
Hamerton

The reaction of phenyl glycidyl ether (PGE) with 1‐ethyl‐3‐methylimidazolium acetateand 1‐ethyl‐3‐methylimidazolium thiocyanate to initiate the polyetherification reaction wasexamined using thermal and spectral analysis techniques. The influence of the nucleophilicity of theanions on the deprotonation of the 1‐ethyl‐3‐methylimidazolium cation determined the reactionpathway. The thermal degradation of the ionic liquid liberated the acetate ion and led, subsequently,to the deprotonation of the acidic proton in the imidazole ring. Thus, polymerisation of PGEoccurred via a carbene intermediate. The more nucleophilic thiocyanate anion was not sufficientlybasic to deprotonate the 1‐ethyl‐3‐methylimidazolium cation, and thus proceeded through directreaction with the PGE, unless the temperature was elevated and a competing carbene mechanismensued.


2006 ◽  
Vol 89 (1) ◽  
pp. 149-156 ◽  
Author(s):  
Dae-Won Park ◽  
Na-Young Mun ◽  
Eun-Ha Lee ◽  
Youngson Choe ◽  
Sang-Wook Park


Author(s):  
Ghada Ali ◽  
Ali G. Hafez ◽  
El-Sayed Soliman A. Said ◽  
Kamal Abdelrahman ◽  
Elkhedr Ibrahim ◽  
...  




1974 ◽  
Vol 8 (7) ◽  
pp. 455-466 ◽  
Author(s):  
K.P.Radha Krishnan ◽  
J.J. Lizcano ◽  
L.T. Fan ◽  
L.E. Erickson


Author(s):  
Priya Saini ◽  
Naveen Kumar ◽  
Shadil Ibrahim Wani ◽  
Shilpi Sharma ◽  
Swapandeep Singh Chimni ◽  
...  


1967 ◽  
Vol 25 (11) ◽  
pp. 1036-1041
Author(s):  
Kjeni NEGORO ◽  
Toshihide OHZUKA


2017 ◽  
Vol 12 (S330) ◽  
pp. 271-272
Author(s):  
M. Tsantaki ◽  
D. T. Andreasen ◽  
G. D. C. Teixeira ◽  
S. G. Sousa ◽  
N. C. Santos ◽  
...  

AbstractCurrent Galactic surveys, including the Gaia mission, rely on the efficiency of the spectral analysis techniques to provide precise and accurate spectral information (i.e. effective temperature, surface gravity, metallicity, and chemical abundances) in the shortest computational time. In this work, we present a new package to preform complete spectral analyses based on the spectral synthesis technique (Tsantaki et al. 2017, submitted). We focus on deriving atmospheric parameters for FGK-type stars using both high and medium resolution (GIRAFFE) spectra. This method is implemented on the Gaia-ESO benchmark stars to confirm its validity, achieving similar accuracy for the two resolution setups.



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