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Determining the Dilution Exponent for Entangled 1,4-Polybutadienes Using Blends of Near-Monodisperse Star with Unentangled, Low Molecular Weight Linear Polymers

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dc.contributor.authorHall, Ryan-
dc.contributor.authorKang, Beom-Goo-
dc.contributor.authorLee, Sanghoon-
dc.contributor.authorChang, Taihyun-
dc.contributor.authorVenerus, David C.-
dc.contributor.authorHadjichristidis, Nikos-
dc.contributor.authorMays, Jimmy-
dc.contributor.authorLarson, Ronald G.-
dc.date.available2020-09-14T08:12:29Z-
dc.date.created2020-06-25-
dc.date.issued2019-02-
dc.identifier.issn0024-9297-
dc.identifier.urihttp://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/39083-
dc.description.abstractWe determine experimentally the "dilution exponent" alpha for entangled polymers from the scaling of terminal crossover frequency with entanglement density from the linear rheology of three 1,4-polybutadiene star polymers that are blended with low-molecular-weight, unentangled linear 1,4-polybutadiene at various star volume fractions, phi(s). Assuming that the rheology of monodisperse stars depends solely on the plateau modulus G(N)(phi(s)) proportional to phi(1+alpha)(s), the number of entanglements per chain M-e(phi(s)) proportional to phi(-alpha)(s), and the tube-segment frictional Rouse time tau(e)(phi(s)) proportional to phi(-2 alpha)(s), we show that only an alpha = 1 scaling superposes the M-e(phi(s)) dependence of the terminal crossover frequency omega(x,t) of the blends with those of pure stars, not alpha = 4/3. This is the first determination of a for star polymers that does not rely on any particular tube model implementation. We also show that a generalized tube model, the "Hierarchical model", using the "Das" parameter set with alpha = 1 reasonably predicts the rheological data of the melts and blends featured in this paper.-
dc.language영어-
dc.language.isoen-
dc.publisherAMER CHEMICAL SOC-
dc.relation.isPartOfMACROMOLECULES-
dc.titleDetermining the Dilution Exponent for Entangled 1,4-Polybutadienes Using Blends of Near-Monodisperse Star with Unentangled, Low Molecular Weight Linear Polymers-
dc.typeArticle-
dc.identifier.doi10.1021/acs.macromol.8b01828-
dc.type.rimsART-
dc.identifier.bibliographicCitationMACROMOLECULES, v.52, no.4, pp.1757 - 1771-
dc.description.journalClass1-
dc.identifier.wosid000460199600038-
dc.identifier.scopusid2-s2.0-85061894337-
dc.citation.endPage1771-
dc.citation.number4-
dc.citation.startPage1757-
dc.citation.titleMACROMOLECULES-
dc.citation.volume52-
dc.contributor.affiliatedAuthorKang, Beom-Goo-
dc.type.docTypeArticle-
dc.description.isOpenAccessN-
dc.subject.keywordPlusCHAIN-LENGTH FLUCTUATIONS-
dc.subject.keywordPlusTEMPORARY NETWORK MODEL-
dc.subject.keywordPlusDYNAMIC DILUTION-
dc.subject.keywordPlusVISCOELASTIC PROPERTIES-
dc.subject.keywordPlusCONSTRAINT-RELEASE-
dc.subject.keywordPlusBINARY BLENDS-
dc.subject.keywordPlusTUBE DILATION-
dc.subject.keywordPlusRHEOLOGY-
dc.subject.keywordPlusMELTS-
dc.subject.keywordPlusRELAXATION-
dc.relation.journalResearchAreaPolymer Science-
dc.relation.journalWebOfScienceCategoryPolymer Science-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
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