Stimuli-Induced Star-Globule Shape Transitions of Dually Responsive Binary Heterografted Three-Arm Star Molecular Brushes in Aqueous Solution
journal contributionposted on 2019-08-28, 16:36 authored by Ethan W. Kent, Bin Zhao
This article reports on the synthesis of doubly responsive binary heterografted, three-arm star molecular brushes and the study of their stimuli-induced star-to-globule shape transitions in aqueous solution. The star brushes were prepared using the highly efficient copper(I)-catalyzed azide–alkyne cycloaddition reaction to simultaneously graft an alkyne end-functionalized thermoresponsive polymer of ethoxydi(ethylene glycol) acrylate (PDEGEA), with a lower critical solution temperature (LCST) of 9 °C, and a pH-responsive polymer of 2-(N,N-diethylamino)ethyl methacrylate (PDEAEMA), with a pKa of 7.4 at room temperature, onto an azide-bearing three-arm star backbone polymer. The star architecture of the formed brushes was confirmed by atomic force microscopy. The use of two different stimuli-responsive polymers as side chains allowed for the stabilization of collapsed brushes against aggregation when one side chain polymer became insoluble in water and for the formation of two distinct globular states with different polymers in the core. At temperatures below the LCST of PDEGEA, upon increasing the pH from 5.00 to 9.40, the brushes underwent a shape transition from an extended starlike to a collapsed globular state stabilized by the hydrated PDEGEA side chains. On the other hand, at pH values slightly lower than the pKa of PDEAEMA, upon heating across the LCST of PDEGEA, the brushes also exhibited a star-to-globule shape transition, forming a globular state distinct from the one induced by pH changes.
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stimuli-induced star-to-globule shape transitionsp KPDEGEA side chainsLCSTglobular statealkyne end-functionalized thermoresponsive polymerHeterografted Three-Arm Star Molecular BrushespHPDEAEMAazide-bearing three-arm star backbone polymerside chain polymerstar-to-globule shape transitionStimuli-Induced Star-Globule Shape Transitions