1989
DOI: 10.1021/ma00194a064
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Synthesis and characterization of multiarm star polybutadienes

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Cited by 121 publications
(95 citation statements)
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“…The effective starlinear polymer interactions are shown to be responsible for the observed counterintuitive phenomena, via a depletionlike mechanism which explains the gel-liquid transition. Eventually, for very high molecular weights a reentrant gelation is observed and attributed to bridging flocculation induced by the long polymer chains.We used model 1,4-polybutadiene starlike entities that are virtually identical to ideal stars [11,13] with f 263 arms and arm molecular weight 42 300 g=mol, (hydrodynamic radius R st H 63 nm, gyration radius R st g 54 nm), coded as LS6, synthesized via hydrosilylation chemistry [14]. At a concentration of 2.5% weight (wt) in the athermal solvent toluene (the star overlap concentration being c 1:8%), a gel is formed, characterized by nearly frequency-independent dynamic storage (G 0 ) and loss (G 00 < G 0 ) moduli over a wide frequency range.…”
mentioning
confidence: 99%
See 1 more Smart Citation
“…The effective starlinear polymer interactions are shown to be responsible for the observed counterintuitive phenomena, via a depletionlike mechanism which explains the gel-liquid transition. Eventually, for very high molecular weights a reentrant gelation is observed and attributed to bridging flocculation induced by the long polymer chains.We used model 1,4-polybutadiene starlike entities that are virtually identical to ideal stars [11,13] with f 263 arms and arm molecular weight 42 300 g=mol, (hydrodynamic radius R st H 63 nm, gyration radius R st g 54 nm), coded as LS6, synthesized via hydrosilylation chemistry [14]. At a concentration of 2.5% weight (wt) in the athermal solvent toluene (the star overlap concentration being c 1:8%), a gel is formed, characterized by nearly frequency-independent dynamic storage (G 0 ) and loss (G 00 < G 0 ) moduli over a wide frequency range.…”
mentioning
confidence: 99%
“…We used model 1,4-polybutadiene starlike entities that are virtually identical to ideal stars [11,13] with f 263 arms and arm molecular weight 42 300 g=mol, (hydrodynamic radius R st H 63 nm, gyration radius R st g 54 nm), coded as LS6, synthesized via hydrosilylation chemistry [14]. At a concentration of 2.5% weight (wt) in the athermal solvent toluene (the star overlap concentration being c 1:8%), a gel is formed, characterized by nearly frequency-independent dynamic storage (G 0 ) and loss (G 00 < G 0 ) moduli over a wide frequency range.…”
mentioning
confidence: 99%
“…It is also advantageous for the large-scale synthesis of star polymers with many arms. Roovers et al, 136 Deffieux et al, 132,133 and Hadjichristidis et al 110 have reported the same subject on star polymer synthesis mentioned in introduction of this chapter. …”
Section: Densely Branched Polymers Carrying Single Branch In Every Rementioning
confidence: 62%
“…The synthesis of multiarm star polymers with 1,4-polybutadiene arms and a very high functionality (about 270) has been described in detail elsewhere [15]. Briefly, a short 1,2-polybutadiene backbone chain was hydrosilylated with HSi(CH 3 )Cl 2 yielding two coupling sites per monomer unit; the latter were substituted with 1,4-polybutadiene by adding of poly(butadienyl)lithium.…”
Section: Methodsmentioning
confidence: 99%