The static scattering function for a regular star-branched polymer is calculated in the full excluded-volume limit with renormalization group techniques, and a closed-form expression for the scattering intensity Z(k) is given. The influence of the excluded-volume interaction between monomers becomes more noticeable as the functionality f of the star increases, qualitative differences appearing between Z(k) and the Gaussian liiit I&). A simplified formula for Z(k) is provided, which can be used for the treatment of experimental data. The scattering of one labeled arm of the star is also investigated and the radius of gyration of the arm is calculated, giving a quantitative expression for the stretching of the branches. I. Introduction Star polymers are receiving nowadays considerable attention in the literature from both e~perimental'-~ and theoreticalG13 points of view. The star-shaped polymers are the simplest branched structures in nature, and their study appears as the first step to the understanding of more complex systems such as gels and rubber. The topological constraint imposed by the presence of a seed or center molecule changes considerably the configura- tional and dynamical properties of the star polymers from a system of linear chains of the same molecular weight. The theoretical treatment pioneered by Zimm and Stockmayer14 on the random-walk model of stars off branches was followed more recently by computer simulationsell and numerical12 and analytical develop- mental3 with the purpose of incorporating in a realistic way the effect of the excluded-volume interactions between monomers in good solvents. The conformational space renormalization group (RG) technique, introduced by Oono and FreedI5 to study linear polymer chains, has been applied to starlike polymers by Miyake and Freed.13 They evaluated the distribution function for intersegment distance vectors and several averages in order to determine the configurational properties of uniform star polymers, in the asymptotic N- m limit, where Nis the total length of the chain. Their results show some departure from the scaling blob theorye but agree with Monte Carlo simula- tions8 for a low (f I 6) degree of branching. Here we concentrate on the calculation of the scattering form factor of f-branched star polymers with the confor- mational space renormalization group method. It is related of course to the segmental density distribution function around the center of the star and is directly measured in standard elastic scattering experiments. The whole range of transfer momenta gives information about concentration fluctuations at different scales within the polymer coil. Moreover, some authors215 extract the radius of gyration of the stars in good solvents from a fit of the scattering intensity with the static structure factor of regular stars with Gaussian statistics.16 Hence, we explore in this paper the predictions of the RG theory about the full excluded- volume regime of the scattering function. We recover then some of the results obtained in ref 13 by another route, and we discuss the influence of the number of branches
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