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端基星型聚合物的网络形成与凝胶化。

Network formation and gelation in telechelic star polymers.

机构信息

Nakshatra I-Land, Flat I-308, Moshi-Alandi Road, Pune 412105, India.

IISER-Pune, 900 NCL Innovation Park, Dr. Homi Bhaba Road, Pune 411008, India.

出版信息

J Chem Phys. 2017 Feb 28;146(8):084906. doi: 10.1063/1.4975691.

Abstract

We investigate the efficiency of gelation and network formation in telechelic star polymer melt, where the tips of polymer arms are dipoles while the rest of the monomers are uncharged. Our work is motivated by the experimental observations [A. Kulkarni et al., Macromolecules 48, 6580 (2015)] in which rheological studies of telechelic star polymers of poly-(L-lactide), a bio-degradable polymer, showed a drastic increase in elastic properties (up to 2000 times) compared to corresponding star polymers without the telechelic arm ends. In contrast to previous studies, we avoid using effective attractive Lennard-Jones potentials or dipolar potentials to model telechelic interactions. Instead we use explicit Coulomb positive and negative charges at the tip of polymer-arms of our bead-spring model of star polymers. By our simulations we show that the dipoles at the tip of star arms aggregate together to form clusters of dipoles. Each cluster has contributions from several stars, and in turn each star contributes to several clusters. Thus the entire polymer melt forms a connected network. Network forming tendencies decrease with a decrease of the value of the effective charge constituting the dipole: this can be experimentally realized by choosing a different ionomer for the star tip. We systematically varied the value of dipole charges, the fraction of star-arms with dipoles at the tip, and the length of the arms. The choice of explicit charges in our calculations enables us to make better quantitative predictions about the onset of gelation; moreover we get qualitatively distinct results about structural organization of dipoles within a dipole-cluster.

摘要

我们研究了端基星型聚合物熔体中的胶凝和网络形成效率,其中聚合物臂的末端是偶极子,而其余单体是不带电的。我们的工作是受到实验观察的启发[Kulkarni 等人,Macromolecules 48, 6580 (2015)],其中聚(L-丙交酯)的端基星型聚合物的流变学研究表明,与没有端基臂末端的相应星型聚合物相比,弹性性能(高达 2000 倍)有了显著提高。与之前的研究不同,我们避免使用有效的吸引力 Lennard-Jones 势或偶极势来模拟端基相互作用。相反,我们在星型聚合物的珠-簧模型中使用聚合物臂末端的明确库仑正电荷和负电荷。通过我们的模拟,我们表明星型臂末端的偶极子聚集在一起形成偶极子簇。每个簇都有几个星的贡献,反过来每个星都对几个簇有贡献。因此,整个聚合物熔体形成了一个连通的网络。网络形成趋势随有效电荷(构成偶极子)值的减小而减小:这可以通过为星端选择不同的离聚物来在实验上实现。我们系统地改变了偶极子电荷、带偶极子的星型臂的分数和臂的长度。我们在计算中选择明确的电荷可以使我们对凝胶化的开始做出更好的定量预测;此外,我们还得到了关于偶极子簇内偶极子结构组织的定性不同的结果。

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