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Effective Electrostatic Interactions in Solutions of Polyelectrolyte Stars with Rigid Rodlike Arms

机译:聚电解质溶液中的有效静电相互作用   明星与刚性棒状武器

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摘要

In solutions of star-branched polyelectrolytes, electrostatic interactionsbetween charged arms on neighboring stars can compete with intra-starinteractions and rotational entropy to induce anisotropy in the orientationaldistribution of arms. For model stars comprising rigid rodlike arms with evenlyspaced charged monomers interacting via an effective screened-Coulomb (Yukawa)potential, we explore the influence of arm orientational anisotropy oneffective star-star interactions. Monte Carlo simulation and density-functionaltheory are used to compute arm orientational distributions and effective pairpotentials between weakly charged stars. The degree of anisotropy is found toincrease with the strength of electrostatic interactions and proximity of thestars. As two stars begin to overlap, the forward arms are pushed back byinter-star arm-arm repulsion, but partially interdigitate due to rotationalentropy. At center-center separations approaching complete overlap, the armsrelax to an isotropic distribution. For nonoverlapping stars,anisotropy-induced changes in intra- and inter-star arm-arm interactionslargely cancel and the effective pair interactions are then well approximatedby a simple Yukawa potential, as predicted by linear response theory for acontinuum model of isotropic stars [A. R. Denton, Phys. Rev. E 67, 11804(2003)]. For overlapping stars, the effective pair interactions in the simplerigid-arm-Yukawa model agree closely with simulations of a molecular model thatincludes flexible arms and explicit counterions [A. Jusufi, C. N. Likos, and H.Lowen, Phys. Rev. Lett. 88, 018301 (2002); J. Chem. Phys. 116, 11011 (2002)].
机译:在星形支化的聚电解质溶液中,相邻恒星上带电臂之间的静电相互作用可与星内相互作用和旋转熵竞争,从而在臂的定向分布中引起各向异性。对于包含刚性杆状臂的模型恒星,该恒星具有通过有效的屏蔽库仑(Yukawa)势相互作用的均匀分布的带电单体,我们研究了臂向各向异性对有效恒星-恒星相互作用的影响。蒙特卡罗模拟和密度泛函理论用于计算微弱带电恒星之间的臂取向分布和有效对电位。发现各向异性程度随着静电相互作用的强度和星体的接近而增加。当两颗星开始重叠时,前星际臂间的排斥力将前臂向后推,但由于旋转熵而部分相互交叉。在中心-中心间距接近完全重叠的情况下,臂rel为各向同性分布。对于非重叠恒星,各向异性引起的星内和星际臂-臂相互作用的变化被大幅度抵消,然后通过简单的汤川势很好地近似有效的对相互作用,这是各向同性恒星的连续谱模型线性响应理论所预测的[A. R. Denton,物理学E 67,11804(2003)。对于重叠的恒星,简单刚性臂-汤川模型中的有效对相互作用与包含柔性臂和显性抗衡离子的分子模型的模拟非常吻合[A. Jusufi,C。N. Likos和H.Lowen,物理学。牧师88,018301(2002); J.化学物理116,11011(2002)]。

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    Wang, Hao; Denton, Alan R.;

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  • 年度 2005
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  • 正文语种 {"code":"en","name":"English","id":9}
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