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Challenging Tube and Slip-Link Models: Predicting the Linear Rheology of Blends of Well-Characterized Star and Linear 1,4-Polybutadienes

机译:具有挑战性的管和滑模模型:预测特征明确的星形和线性1,4-聚丁二烯混合物的线性流变学

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We compare predictions of two of the most advanced versions of the tube model, namely the "Hierarchical model" by Wang et al. [J. Rheol. 2010, 54, 223] and the BoB (branch-on-branch) model by Das et al. [J. Rheol. 2006, SO, 207], against linear viscoelastic G' and G '' data of binary blends of nearly monodisperse 1,4-polybutadiene 4-arm star polymer of arm molar mass 24 000 g/mol with a monodisperse linear 1,4-polybutadiene of molar mass 58 000 g/mol. The star was carefully synthesized and characterized by temperature gradient interaction chromatography and by linear rheology over a wide frequency region through time temperature superposition. We found large failures of both the Hierarchical and BoB models to predict the terminal relaxation behavior of the star/linear blends, despite their success in predicting the rheology of the pure star and pure linear polymers. This failure occurred regardless of the choices made concerning constraint release, such as assuming arm retraction in "fat" or "skinny" tubes. Allowing for "disentanglement relaxation" to cut off the constraint release Rouse process at long times does lead to improved predictions for our blends, but leads to much worse predictions for other star/linear blends described in the literature, especially those of Shivokhin et al. [Macromolecules 2014, 47, 2451]. In addition, our blends and those of Shivokhin et al. were also tested against a coarse-grained slip-link model, the "clustered fixed slip-link model (CFSM)" of Schieber and co-workers [J. Rheol. 2014, 58, 723], in which several Kuhn steps are clustered together for computational efficiency. The CFSM with only two molecular-weight- and chain-architecture-independent parameters was able to give very good agreement with all experimental data for both of these sets of blends. In light of its success, the CFSM slip-link model may be used to address the constraint release issue more rigorously and potentially help develop improved tube models.
机译:我们比较了两种最高级版本的管模型的预测,即Wang等人的“分层模型”。 [J. he 2010,54,223]和Das等人的BoB(branch-on-branch)模型。 [J. he 2006,SO,207],针对线性摩尔弹性G'和G''数据,该数据为臂摩尔质量为24000 g / mol的几乎单分散的1,4-聚丁二烯4-臂星形聚合物与单分散的线性1,4-摩尔质量为58 000 g / mol的聚丁二烯。通过温度梯度相互作用色谱和通过时温度叠加在宽频率范围内的线性流变学,仔细合成了该恒星并对其进行了表征。我们发现,分层和BoB模型均无法预测星形/线性共混物的最终弛豫行为,尽管它们在预测纯星形和线性聚合物的流变学方面也取得了成功。不管选择哪种约束释放方式都发生此故障,例如假设手臂在“胖”或“瘦”管中缩回。长时间允许“解缠结松弛”来切断约束释放的Rouse过程确实可以改善我们的混合预测,但对于文献中描述的其他星/线性混合,尤其是Shivokhin等人的预测,则导致更差的预测。 [Macromolecules 2014,47,2451]。此外,我们的混合物与Shivokhin等人的混合物。还针对粗粒度滑动链接模型,Schieber及其同事的“群集固定滑动链接模型(CFSM)”进行了测试[J. he 2014,58,723],其中几个Kuhn步骤被聚类在一起以提高计算效率。仅具有两个与分子量和链结构无关的参数的CFSM能够与这两组共混物的所有实验数据很好地吻合。鉴于其成功,CFSM滑移链接模型可用于更严格地解决约束释放问题,并有可能帮助开发改进的管模型。

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