scholarly journals α-C–C agostic interactions and C–H bond activation in scandium cyclopropyl complexes

2020 ◽  
Vol 7 (24) ◽  
pp. 4822-4831
Author(s):  
Cheng Xu ◽  
Guangyu Li ◽  
Michel Etienne ◽  
Xuebing Leng ◽  
Yaofeng Chen

Electron deficient scandium cyclopropyl complexes have been synthesized and fully characterized for the first time, and a combination of solid XRD, solution NMR and theoretical studies well demonstrated the α-C–C agostic interactions in the complexes.

Author(s):  
Francesca Ferrari ◽  
Maicol Bissaro ◽  
Simone Fabbian ◽  
Jessica de Almeida Roger ◽  
Stefano Mammi ◽  
...  

<p>In this manuscript, for the first time, we presented a fragment library and we validated its performance by comparison with a well-established technique for fragment screening as solution NMR. We were able to screen 400 different fragments producing a total of 1200 independent fragment-protein recognition pathways. As far as we know, this represents the largest screening based on Molecular dynamics ever reported. Our simulations successfully detected the true binders in the library in a prospective study, showing a notable agreement with a state-of-art screening we performed by NMR on the same dataset.</p>


2008 ◽  
Vol 27 (7) ◽  
pp. 1384-1392 ◽  
Author(s):  
Ping Yang ◽  
Ingolf Warnke ◽  
Richard L. Martin ◽  
P. Jeffrey Hay

2020 ◽  
Vol 44 (22) ◽  
pp. 9238-9247
Author(s):  
Xin Ji ◽  
Yong Guo ◽  
Shugui Hua ◽  
Huiyan Li ◽  
Sunchen Zhang

In this paper, the sensitization photodegradation of single and mixed dyes by wide band gap boron nitride (BN, 3.94 eV) under visible light irradiation has been investigated for the first time.


2015 ◽  
Vol 51 (36) ◽  
pp. 7685-7688 ◽  
Author(s):  
Shunsuke Sueki ◽  
Yoichiro Kuninobu

We successfully developed rhodium-catalysed synthesis of multi-substituted silylindenes from 2 equivalents of aryl alkynes and 1 equivalent of hydrosilanes in moderate to good yields via C–H bond activation for the first time.


1995 ◽  
Vol 12 (2) ◽  
pp. 190-196 ◽  
Author(s):  
J. Bland-Hawthorn

AbstractIt has long been suspected that winds of thermal and/or relativistic particles are a common feature of both active and normal galaxies. Galactic winds are likely to be an important mechanism, particularly at high redshift, by which energy and metals from galaxies are subsequently dumped into the intergalactic medium. Both observational and theoretical studies of wind processes remain in their infancy, largely because astrophysical winds are difficult to detect. Future satellite missions will make systematic surveys possible for the first time. In this review, we summarise the current evidence for galactic-scale winds, particularly in energy bands where the wind emission is spatially resolved. We also discuss observational limitations and problems of interpretation.


2020 ◽  
pp. 56-59
Author(s):  
E.E. Badiyan ◽  
Ye.V. Ftomov ◽  
O.V. Shekhovtsov ◽  
A.G. Tonkopryad

Theoretical studies of feasible rotations of the crystal lattice during the deformation of samples with an FCC structure under uniaxial tension are carried out. The results of the experimental determination of the magnitudes of these rotations for various grains of two-dimensional polycrystalline aluminum samples after their deformation by the same strain value are presented. For the first time, it has been theoretically shown and experimentally confirmed that under uniaxial tension of a specimen under the conditions of operation of only one slip system, regardless of the scheme of rotation, the magnitude of the rotation is determined only by the angle between the direction of the tensile axis and the slip direction before deformation of the specimen.


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