Structural arrest in dense star-polymer solutions

被引:103
作者
Foffi, G
Sciortino, F
Tartaglia, P
Zaccarelli, E
Lo Verso, F
Reatto, L
Dawson, KA
Likos, CN
机构
[1] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[2] Univ Roma La Sapienza, INFM, Ctr Stat Mech & Complex, I-00185 Rome, Italy
[3] Univ Milan, Ist Nazl Fis Mat, I-20133 Milan, Italy
[4] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy
[5] Univ Coll Dublin, Irish Ctr Colloid Sci & Biomat, Dept Chem, Dublin 4, Ireland
[6] Univ Dusseldorf, Inst Theoret Phys 2, D-40225 Dusseldorf, Germany
关键词
D O I
10.1103/PhysRevLett.90.238301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The dynamics of star polymers is investigated via extensive molecular and Brownian dynamics simulations for a large range of functionality f and packing fraction eta. The calculated isodiffusivity curves display both minima and maxima as a function of eta and minima as a function of f. Simulation results are compared with theoretical predictions based on different approximations for the structure factor. In particular, the ideal glass transition line predicted by mode-coupling theory is shown to exactly track the isodiffusivity curves, offering a theoretical understanding for the observation of disordered arrested states in star-polymer solutions.
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页数:4
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