conformational composition
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2021 ◽  
Vol 47 (4) ◽  
pp. 318-324
Author(s):  
I. Doroshenko ◽  
Ye. Vaskivsky ◽  
Ye. Chernolevskaya ◽  
O. Doroshenko


Photochem ◽  
2021 ◽  
Vol 1 (1) ◽  
pp. 10-25
Author(s):  
İsa Sıdır ◽  
Sándor Góbi ◽  
Yadigar Gülseven Sıdır ◽  
Rui Fausto

The conformational stability, infrared spectrum, and photochemistry of phenyl 1-hydroxy-2-naphthoate (PHN) were studied by matrix isolation infrared spectroscopy and theoretical computations performed at the DFT(B3LYP)/6-311++G(d,p) level of theory. The main intramolecular interactions determining the relative stability of seven conformers of the molecule were evaluated. According to the calculations, the twofold degenerated O–H···O=C intramolecularly hydrogen-bonded conformer with the phenyl ring ester group ±68.8° out of the plane of the substituted naphtyl moiety is the most stable conformer of the molecule. This conformer is considerably more stable than the second most stable form (by ~15 kJ mol−1), in which a weaker O–H···O–C intramolecular hydrogen bond exists. The compound was isolated in cryogenic argon and N2 matrices, and the conformational composition in the matrices was investigated by infrared spectroscopy. In agreement with the predicted relative energies of the conformers, the analysis of the spectra indicated that only the most stable conformer of PHN was present in the as-deposited matrices. The matrices were then irradiated at various wavelengths by narrowband tunable UV light within the 331.7–235.0 nm wavelength range. This resulted in the photodecarbonylation of PHN, yielding 2-phenoxynaphthalen-1-ol, together with CO. The extension of the decarbonylation was found to depend on the excitation wavelength.



2020 ◽  
Vol 132 (52) ◽  
pp. 23932-23938 ◽  
Author(s):  
Katherine Cobos ◽  
Rafael Rodríguez ◽  
Emilio Quiñoá ◽  
Ricardo Riguera ◽  
Félix Freire


2020 ◽  
Vol 59 (52) ◽  
pp. 23724-23730
Author(s):  
Katherine Cobos ◽  
Rafael Rodríguez ◽  
Emilio Quiñoá ◽  
Ricardo Riguera ◽  
Félix Freire




Soft Matter ◽  
2020 ◽  
Vol 16 (48) ◽  
pp. 10954-10968
Author(s):  
Lalitha Sruthi ◽  
Vishal Srivastava ◽  
Lars E. Schmidt ◽  
Abhijit P. Deshpande ◽  
Susy Varughese

Rheology and microstructure of casein dispersions undergoing drying are investigated. Drying alters conformational composition of secondary structures of the protein (α-helix, β-sheets, turns and random) and hence the packing behavior of molecular assemblies of casein.



2018 ◽  
Vol 73 ◽  
pp. 355-364 ◽  
Author(s):  
David J. Belton ◽  
Robyn Plowright ◽  
David L. Kaplan ◽  
Carole C. Perry


2017 ◽  
Vol 2017 ◽  
pp. 1-10 ◽  
Author(s):  
Zuzana Hanzlíková ◽  
Michael Kenneth Lawson ◽  
Peter Hybler ◽  
Marko Fülöp ◽  
Mária Porubská

Wool scoured in tap water with no special degreasing and containing a balanced humidity responding to usual laboratory conditions was irradiated by accelerated electron beam in the range of 0–350 kGy dose. Time variations of the wool structure were measured using FTIR, Raman, and EPR spectroscopy. The aim was to determine whether preexposure treatment of the wool, as well as postexposure time, affects the properties of the irradiated wool. Reactive products such as S-sulfonate, cystine monoxide, cystine dioxide, cysteic acid, disulphides, and carboxylates displayed a considerable fluctuation in quantity depending on both the absorbed dose and time. Mutual transformations of S-oxidized products into cysteic acid appeared to be faster than those in dry and degreased wool assuming that the present humidity inside the fibres is decisive as an oxygen source. EPR results indicated a longer lifetime for free radicals induced by lower doses compared with the radicals generated by higher ones. The pattern of the conformational composition of the secondary structure (α-helix, β-sheet, random, and residual conformations) also showed a large variability depending on absorbed dose as well as postexposure time. The most stable secondary structure was observed in nonirradiated wool but even this showed a small but observable change after a longer time, too.



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