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Multiscale dynamics of an interacting sheet by a bond-fluctuating Monte Carlo simulation

✍ Scribed by R. B. Pandey; Kelly L. Anderson; B. L. Farmer


Book ID
105338379
Publisher
John Wiley and Sons
Year
2006
Tongue
English
Weight
764 KB
Volume
44
Category
Article
ISSN
0887-6266

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✦ Synopsis


Abstract

The conformation and dynamics of sheets with attractive and repulsive node–node interactions (nn) are examined in an effective solvent medium using Monte Carlo simulations. A bond‐fluctuating coarse grained description is used to model the sheet by a set of nodes (N) tethered together by flexible bonds in a planar structure with linear scale L~s~ = 16–64, N = L on a cubic lattice with characteristic dimensions of L^3^ = 64^3^–200^3^. Variations of the mean square displacement of the center of mass of the sheet (R) and that of its center node (R) and radius of gyration (R~g~) of the sheet with the time step (t) are analyzed to characterize the nature of its global motion, segmental dynamics, and conformational relaxation at a low (T = 2) and a high (T = 10) temperature with the range (r = √8) of interaction nn = 1, –1. We find that sheets achieve their global diffusive motion, that is, Rt, in the long‐time (asymptotic) regime while their segmental dynamics exhibits a range of power‐law behavior Rt^ν^ with ν = 1/4−1 from short to long‐time regimes. The magnitude of the exponent ν and their crossover (and relaxation) from one power‐law to the next depend on temperature, interaction, and molecular weight N of the sheet. The radius of gyration of the sheet relaxes well to its equilibrium with its distinct patterns of expansion (swelling with relatively stiffer bonds (nn = 1)) and contraction (crumpling with nn = −1). Both the relaxation time and the rate of change of R~g~ depends on N, L~s~, and T. Data for the equilibrium value of the gyration radius scale with its size R~g~ ∝ N^1/2^ suggesting that sheets remain nearly flat with localized wrinkles and crumpling.© 2006 Wiley Periodicals, Inc. J Polym Sci Part B: Polym Phys 44: 2512–2523, 2006


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