Coalescence Model for Crumpled Globules Formed in Polymer Collapse

The rapid collapse of a polymer, due to external forces or changes in solvent, yields a long-lived “crumpled globule.” The conjectured fractal structure shaped by hierarchical collapse dynamics has proved difficult to establish, even with large simulations. To unravel this puzzle, we study a coarse-...

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Main Authors: Bunin, Guy, Kardar, Mehran
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Physical Society 2015
Online Access:http://hdl.handle.net/1721.1/98178
https://orcid.org/0000-0002-1112-5912
https://orcid.org/0000-0002-3074-4217
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author Bunin, Guy
Kardar, Mehran
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Bunin, Guy
Kardar, Mehran
author_sort Bunin, Guy
collection MIT
description The rapid collapse of a polymer, due to external forces or changes in solvent, yields a long-lived “crumpled globule.” The conjectured fractal structure shaped by hierarchical collapse dynamics has proved difficult to establish, even with large simulations. To unravel this puzzle, we study a coarse-grained model of in-falling spherical blobs that coalesce upon contact. Distances between pairs of monomers are assigned upon their initial coalescence, and do not “equilibrate” subsequently. Surprisingly, the model reproduces quantitatively the dependence of distance on segment length, suggesting that the slow approach to scaling is related to the wide distribution of blob sizes.
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spelling mit-1721.1/981782022-10-02T07:18:53Z Coalescence Model for Crumpled Globules Formed in Polymer Collapse Bunin, Guy Kardar, Mehran Massachusetts Institute of Technology. Department of Physics Bunin, Guy Kardar, Mehran The rapid collapse of a polymer, due to external forces or changes in solvent, yields a long-lived “crumpled globule.” The conjectured fractal structure shaped by hierarchical collapse dynamics has proved difficult to establish, even with large simulations. To unravel this puzzle, we study a coarse-grained model of in-falling spherical blobs that coalesce upon contact. Distances between pairs of monomers are assigned upon their initial coalescence, and do not “equilibrate” subsequently. Surprisingly, the model reproduces quantitatively the dependence of distance on segment length, suggesting that the slow approach to scaling is related to the wide distribution of blob sizes. National Science Foundation (U.S.) (Grant DMR-12-06323) MIT Department of Physics Pappalardo Program (Fellowship) 2015-08-21T12:50:22Z 2015-08-21T12:50:22Z 2015-08 2015-03 2015-08-20T22:00:04Z Article http://purl.org/eprint/type/JournalArticle 0031-9007 1079-7114 http://hdl.handle.net/1721.1/98178 Bunin, Guy, and Mehran Kardar. "Coalescence Model for Crumpled Globules Formed in Polymer Collapse." Phys. Rev. Lett. 115, 088303 (August 2015). © 2015 American Physical Society https://orcid.org/0000-0002-1112-5912 https://orcid.org/0000-0002-3074-4217 en http://dx.doi.org/10.1103/PhysRevLett.115.088303 Physical Review Letters Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Physical Society application/pdf American Physical Society American Physical Society
spellingShingle Bunin, Guy
Kardar, Mehran
Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title_full Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title_fullStr Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title_full_unstemmed Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title_short Coalescence Model for Crumpled Globules Formed in Polymer Collapse
title_sort coalescence model for crumpled globules formed in polymer collapse
url http://hdl.handle.net/1721.1/98178
https://orcid.org/0000-0002-1112-5912
https://orcid.org/0000-0002-3074-4217
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