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首页> 外文期刊>Macromolecules >Role of architecture on the conformation, rheology, and orientation behavior of linear, star, and hyperbranched polymer melts. 2. Linear viscoelasticity and flow birefringence
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Role of architecture on the conformation, rheology, and orientation behavior of linear, star, and hyperbranched polymer melts. 2. Linear viscoelasticity and flow birefringence

机译:体系结构对线性,星形和超支化聚合物熔体的构象,流变学和取向行为的作用。 2.线性粘弹性和流动双折射

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In the preceding publication, we showed that the hyperbranched polystyrenes (HBPS) synthesized as part of this study may be viewed as starlike molecules with a high branch density, which are either unentangled or weakly entangled. In this paper, the role of architecture, especially the branch density, on the rheological and orientation behavior is investigated using simultaneous, quantitative stress and flow birefringence measurements in the melt state. Linear PS and eight-arm symmetric PS stars follow the stress-optical rule (SOR) over a wide dynamic range, with the stress-optical coefficient (C) governed by the arm molecular weight. When the branch density is "moderate" (greater than similar to20 arms), there is only a hint of nonterminal behavior in the viscoelastic moduli, while the C drops by 30% compared to a star with eight arms of comparable length. When the branch density is "high" (similar to50 arms), and the arms are unentangled, the nonterminal behavior in G* is clearly apparent, and there is a dramatic breakdown in the stress-optical rule in these homopolymer melts. The quantitative birefringence measurements suggest that the "excess" birefringence may be due to the "form" contributions from the core-shell structure. Such a structure may be formed by the preferential radial stretching of the chain segments near the core, as suggested by other studies on hyperstars. For comparable chain density, the core would be bigger than the shell when the arm length is smaller. Therefore, the 5K-HBPS exhibits a more severe breakdown compared to the 10K-HBPS. [References: 74]
机译:在之前的出版物中,我们表明,作为本研究的一部分,合成的超支化聚苯乙烯(HBPS)可以被视为具有高分支密度的星形分子,该分子要么是无缠结的,要么是弱缠结的。在本文中,使用熔融状态下同时进行的定量应力和流双折射测量,研究了体系结构(尤其是分支密度)在流变和取向行为方面的作用。线性PS星和八臂对称PS星在很宽的动态范围内遵循应力光学法则(SOR),应力光学系数(C)受臂分子量控制。当分支密度为“中等”(大于类似于20个臂的密度)时,粘弹性模量仅显示出非末端行为的提示,而与具有八个长度相当的臂的恒星相比,C下降了30%。当支链密度为“高”(类似于50个支链)且支链未缠结时,G *的非末端行为显而易见,并且在这些均聚物熔体中,应力-光学规则显着破坏。定量双折射测量表明“过量”双折射可能是由于核-壳结构的“形式”贡献所致。如其他有关超级巨星的研究所建议的那样,这种结构可能是通过在核附近的链段进行优先的径向拉伸而形成的。对于相当的链密度,当臂长较小时,核将比壳大。因此,与10K-HBPS相比,5K-HBPS表现出更严重的击穿。 [参考:74]

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