2019
DOI: 10.1002/mats.201900012
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Universal Size and Shape Ratios for Arms in Star‐Branched Polymers: Theory and Mesoscopic Simulations

Abstract: Star polymer undergoes a transformation from a group of loosely coupled chains at low number of arms to a dense hairy colloid at their high number. This change affects solubility, aggregation, and rheological behavior and is of much practical interest. The range of size and shape properties of the star molecule and of its individual arms upon this transformation are studied. Theoretical calculations are based on a continuous chain model and are performed in the first order in ε = 4 −d. Computer simulations are… Show more

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Cited by 6 publications
(9 citation statements)
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References 50 publications
(191 reference statements)
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“…Another note is the presence of a formal limit g s = 1 at F = 1, and at F = 3 the meaning of g s (3) coincides with that for the size ratio g(3) between the star and a linear chain, as defined in Ref. 37. Both values are found to be the same, g s (3) ≈ g(3) ≈ 0.8, see Fig.…”
Section: Simulation Resultssupporting
confidence: 78%
See 3 more Smart Citations
“…Another note is the presence of a formal limit g s = 1 at F = 1, and at F = 3 the meaning of g s (3) coincides with that for the size ratio g(3) between the star and a linear chain, as defined in Ref. 37. Both values are found to be the same, g s (3) ≈ g(3) ≈ 0.8, see Fig.…”
Section: Simulation Resultssupporting
confidence: 78%
“…2 in Ref. 37. With the increase of F , both theoretical result and the simulation data show the decrease of g s in Fig.…”
Section: Simulation Resultsmentioning
confidence: 67%
See 2 more Smart Citations
“…[8,9] The majority of the simulation and theoretical studies deals with a single star properties in solvent, focusing mostly on the two factors: the effect of the environment (i.e., solvent quality) and the effect of the functionality. [10][11][12][13][14][15][16][17][18][19][20][21][22] Theoretical models describe the conformation of an isolated symmetric star through a blob picture, where each arm consists of a sequence of blobs, whose size depends on the relative distance of the blob from the star center, on the strength of the excluded volume interactions and the functionality. [13][14][15] This geometrical approach allows for the formulation of scaling predictions for the star size in different solvents and was extended for the star polymers dissolved in a melt of linear chains.…”
Section: Doi: 101002/mats202000067mentioning
confidence: 99%