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High Resolution Image Download MS PowerPoint Slide Based on computer simulations, we analyze how different forms of labeling the network components allow us to extract complementary structural information. The analysis relies upon simulations of heterocomplementary bound four-functional star polymers A 4 and B 4 . For optimized contrast between A and B stars, the calculated dynamic scattering intensity resembles A-B block copolymers with an apparent repulsion between both components, accounting for ordering effects due to the complementary coupling scheme. The position of the observed scattering peak is compatible with the radius of gyration of A-B chains connecting adjacent star centers. Labeling the star centers or small regions around them reveals a correlation hole of the star centers and their mutual repulsion, compatible with a Gaussian core repulsion. Accordingly, scattering is suppressed toward small wave vectors, allowing for a decomposition of the observed scattering intensity into a product of the form factor of the labeled star sections and a structure factor describing the distribution of cross-links in space. When choosing opposite scattering amplitudes for the central regions of A and B stars, static scattering directly reveals the distance between connected star centers.
Scholz et al. (Fri,) studied this question.