Please use this identifier to cite or link to this item: https://open.uns.ac.rs/handle/123456789/4139
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dc.contributor.authorPortet S.en
dc.contributor.authorTuszynski J.en
dc.contributor.authorDixon J.en
dc.contributor.authorSataric M.en
dc.date.accessioned2019-09-23T10:32:13Z-
dc.date.available2019-09-23T10:32:13Z-
dc.date.issued2003-01-01en
dc.identifier.issn1063651Xen
dc.identifier.urihttps://open.uns.ac.rs/handle/123456789/4139-
dc.description.abstractTabony and co-workers [C. Papaseit, N. Pochon, and J. Tabony, Proc. Natl. Acad. Sci. U.S.A. 97, 8364 (2000)] showed that the self-organization of microtubules from purified tubulin solutions is sensitive to gravitational conditions. In this paper, we propose two models of spatial and orientational self-organization of microtubules in a gravitational field. First, the spatial model is based on the dominant chemical kinetics. The pattern formation of microtubule concentration is obtained (1) in terms of a moving kink in the limit when the disassembly rate is negligible, and (2) for the case of no free tubulin and only assembled microtubules present. Second, the orientational pattern of striped microtubule domains is consistent with predictions from a phenomenological Landau-Ginzburg free energy expansion in terms of an orientational order parameter. © 2003 The American Physical Society.en
dc.relation.ispartofPhysical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topicsen
dc.titleModels of spatial and orientational self-organization of microtubules under the influence of gravitational fieldsen
dc.typeJournal/Magazine Articleen
dc.identifier.doi10.1103/PhysRevE.68.021903en
dc.identifier.pmid68en
dc.identifier.scopus2-s2.0-85035233854en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85035233854en
dc.relation.firstpage9en
dc.relation.issue2en
dc.relation.volume68en
item.grantfulltextnone-
item.fulltextNo Fulltext-
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