Brownian simulations for fracture of star polymer phantom networks

Fuente: arXiv
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Autores principales: Masubuchi, Yuichi, Koide, Yusuke, Ishida, Takato, Uneyama, Takashi
Formato: Preprint
Publicado: 2024
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author Masubuchi, Yuichi
Koide, Yusuke
Ishida, Takato
Uneyama, Takashi
author_facet Masubuchi, Yuichi
Koide, Yusuke
Ishida, Takato
Uneyama, Takashi
contents Based on a recent simulation study [Masubuchi et al., Macromolecules, 56, 9359 (2023)], the cycle rank plays a significant role in determining the fracture characteristics of network polymers. However, the study only considered energy-minimized networks without the effects of thermal agitation. We conducted Brownian dynamics simulations at various stretch rates to address this gap. The results showed that even with Brownian motion, the strain and stress at the break obtained for different node functionalities and conversion ratios exhibited master curves if plotted against cycle rank. These master curves were dependent on the strain rate, with the curves tending to approach those observed in energy-minimized simulations as the strain rate decreased, even though the fracture process was affected by the competition against Brownian motion, elongation, and bond degradation.
format Preprint
id arxiv_https___arxiv_org_abs_2409_12449
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Brownian simulations for fracture of star polymer phantom networks
Masubuchi, Yuichi
Koide, Yusuke
Ishida, Takato
Uneyama, Takashi
Soft Condensed Matter
Based on a recent simulation study [Masubuchi et al., Macromolecules, 56, 9359 (2023)], the cycle rank plays a significant role in determining the fracture characteristics of network polymers. However, the study only considered energy-minimized networks without the effects of thermal agitation. We conducted Brownian dynamics simulations at various stretch rates to address this gap. The results showed that even with Brownian motion, the strain and stress at the break obtained for different node functionalities and conversion ratios exhibited master curves if plotted against cycle rank. These master curves were dependent on the strain rate, with the curves tending to approach those observed in energy-minimized simulations as the strain rate decreased, even though the fracture process was affected by the competition against Brownian motion, elongation, and bond degradation.
title Brownian simulations for fracture of star polymer phantom networks
topic Soft Condensed Matter
url https://arxiv.org/abs/2409.12449