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首页> 外文期刊>Polymer: The International Journal for the Science and Technology of Polymers >Synthesis of beta-cyclodextrin-based star polymers via a simplified electrochemically mediated ATRP
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Synthesis of beta-cyclodextrin-based star polymers via a simplified electrochemically mediated ATRP

机译:通过简化的电化学介导的ATRP合成基于β-环糊精的星形聚合物

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Cyclodextrin-based star polymers were synthesized using functionalized beta-cyclodextrin (beta-CD) core, and n-butyl acrylate (BA) as hydrophobic arms. The beta-CD core macroinitiator was prepared by the transesterification reaction of b-CD with 2-bromoisobutyryl bromide. The core-first method was chosen as the synthetic strategy as it allows good control over the polymer architecture. Star-shaped amphiphilic polymers were prepared via a simplified electrochemically mediated ATRP (seATRP) procedure under both potentiostatic and pseudo-galvanostatic conditions, utilizing only 50 ppm (40 ppm by weight (wt)) of Cu-II complex, much less than previously reported concentrations of catalyst of ca. 4,000-130,000 ppm (590-19,000 ppm (by wt)). The rate of the polymerizations (R-p) was controlled by applying different potentials E-app, with slower R-p observed using more positive E-app values thereby suppressing intermolecular termination reactions between growing arms, and subsequent starestar coupling. The polymerization results showed molecular weight evolution close to theoretical values while maintaining a narrow molecular weight distribution for the growing star polymer throughout the reaction. The differences between theoretical and measured MW originate in different hydrodynamic radii of stars and linear polymers used as standards for gel-permeation chromatography (GPC). Successful chain extension of the omega-functional arms with tert-butyl acrylate (tBA) resulted in star block copolymers and confirmed the living nature of the beta-CD-PBA star polymers prepared by seATRP. Moreover, the absence of radical coupling reactions during seATRP synthesis was confirmed by GPC analyses of the actual arm length of obtained star polymers and copolymers. (C) 2016 Elsevier Ltd. All rights reserved.
机译:使用功能化的β-环糊精(β-CD)核和丙烯酸正丁酯(BA)作为疏水臂,合成了基于环糊精的星形聚合物。 β-CD核心大分子引发剂是通过b-CD与2-溴异丁酰溴的酯交换反应制备的。选择核心优先的方法作为合成策略,因为它可以很好地控制聚合物结构。通过简化的电化学介导的ATRP(seATRP)程序在恒电位和拟恒电流条件下制备星形两亲聚合物,仅使用50 ppm(40 ppm重量(wt))的Cu-II配合物,比以前报道的要少得多催化剂的浓度约为4,000-130,000 ppm(590-19,000 ppm(重量))。通过施加不同的电势E-app来控制聚合速率(R-p),使用更正的E-app值可观察到较慢的R-p,从而抑制了增长臂之间的分子间终止反应以及随后的starestar偶联。聚合结果表明,分子量增长接近理论值,同时在整个反应过程中,对于正在生长的星形聚合物,分子量保持窄的分布。理论分子量与实测分子量之间的差异源自恒星和用作凝胶渗透色谱(GPC)标准的线性聚合物的不同流体力学半径。使用丙烯酸叔丁酯(tBA)成功完成欧米茄功能臂的扩链,形成了星形嵌段共聚物,并证实了seATRP制备的β-CD-PBA星形聚合物的活性。此外,通过GPC分析获得的星形聚合物和共聚物的实际臂长可以确认seATRP合成过程中不存在自由基偶联反应。 (C)2016 Elsevier Ltd.保留所有权利。

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