Role of grafted chains for the in situ formation of Ag nanoparticles within poly(epichlorohydrin)-g-polymethacrylate films

2009 ◽  
Vol 9 (4) ◽  
pp. e298-e300
Author(s):  
Jung Tae Park ◽  
Kyung Ju Lee ◽  
Jong Kwan Koh ◽  
Jong Hak Kim ◽  
Ki Bong Lee
Author(s):  
Hwajoong Kim ◽  
Ammar Shaqeel ◽  
Solbi Han ◽  
Junseo Kang ◽  
Jieun Yun ◽  
...  

2021 ◽  
Vol 594 ◽  
pp. 824-835
Author(s):  
Guomin Yu ◽  
Qingyi Qian ◽  
Donghao Li ◽  
Zhenxi Zhang ◽  
Kexin Ren ◽  
...  

2009 ◽  
Vol 165 ◽  
pp. 012074 ◽  
Author(s):  
Akio Hirose ◽  
Hiroaki Tatsumi ◽  
Naoya Takeda ◽  
Yusuke Akada ◽  
Tomo Ogura ◽  
...  

2007 ◽  
Vol 111 (21) ◽  
pp. 7676-7681 ◽  
Author(s):  
Yan Lu ◽  
Yu Mei ◽  
Marc Schrinner ◽  
Matthias Ballauff ◽  
Michael W. Möller ◽  
...  

2004 ◽  
Vol 82 (2) ◽  
pp. 120-130 ◽  
Author(s):  
David R Williams ◽  
Kevin G Meyer ◽  
Khalida Shamim ◽  
Samarjit Patnaik

A series of nonracemic homoallylic alcohols have been prepared by asymmetric allylation using the (R,R)- and (S,S)-1,2-diamino-1,2-diphenylethane bis-sulfonamide controller ligands for in situ formation of chiral B-allyl-1,3,2-diazaborolidines. Diastereofacial selectivity is influenced by adjacent stereochemistry incorporated into the allyl moiety at C-2, in addition to the expected role of the chiral auxiliary. Additional asymmetry in the aldehyde reactant introduces threefold stereodifferentiation. A model is developed to identify reinforcing stereochemical relationships, and examples have ascertained the relative significance of these factors. The methodology supports the construction of complex homoallylic alcohols in a highly convergent fashion.Key words: asymmetric allylation, diastereofacial selectivity, 1,4-stereocontrol, homoallylic alcohols.


2014 ◽  
Vol 9 (S310) ◽  
pp. 204-207
Author(s):  
O. M. Guilera ◽  
D. Swoboda ◽  
Y. Alibert ◽  
G. C. de Elía ◽  
P. J. Santamaría ◽  
...  

AbstractIn the standard model of core accretion, the cores of the giant planets form by the accretion of planetesimals. In this scenario, the evolution of the planetesimal population plays an important role in the formation of massive cores. Recently, we studied the role of planetesimal fragmentation in the in situ formation of a giant planet. However, the exchange of angular momentum between the planet and the gaseous disk causes the migration of the planet in the disk. In this new work, we incorporate the migration of the planet and study the role of planet migration in the formation of a massive core when the population of planetesimals evolves by planet accretion, migration, and fragmentation.


Desalination ◽  
2013 ◽  
Vol 324 ◽  
pp. 48-56 ◽  
Author(s):  
Xin Li ◽  
Ruizhi Pang ◽  
Jiansheng Li ◽  
Xiuyun Sun ◽  
Jinyou Shen ◽  
...  

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