Efficient Synthesis of Asymmetric Miktoarm Star Polymers
Asymmetric miktoarm star polymers produce unique material properties, yet existing synthetic strategies are beleaguered by complicated reaction schemes restricted in both the monomer scope and yield. Here, we introduce a new synthetic approach coined “μSTAR”, miktoarm synthesis by termination after...
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Published in | Macromolecules Vol. 53; no. 2; pp. 702 - 710 |
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Main Authors | , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
United States
American Chemical Society
28.01.2020
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Subjects | |
Online Access | Get full text |
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Summary: | Asymmetric miktoarm star polymers produce unique material properties, yet existing synthetic strategies are beleaguered by complicated reaction schemes restricted in both the monomer scope and yield. Here, we introduce a new synthetic approach coined “μSTAR”, miktoarm synthesis by termination after ring-opening metathesis polymerization, that circumvents these traditional synthetic limitations by constructing the block–block junction in a scalable one-pot process involving (1) grafting-through polymerization of a macromonomer followed by (2) in situ enyne-mediated termination to install a single mikto-arm with exceptional efficiency. This modular μSTAR platform cleanly generates AB n and A(BA′) n miktoarm star polymers with unprecedented versatility in the selection of A and B chemistries as demonstrated using many common polymer building blocks. The average number of B or BA′ arms (n) is easily controlled by the equivalents of Grubbs catalyst. While these materials are characterized by dispersity in n that arises from the statistics of polymerization, they self-assemble into mesophases that are identical to those predicted for precise miktoarm stars. In summary, the μSTAR technique provides a significant boost in design flexibility and synthetic simplicity while retaining the salient phase behavior of precise miktoarm star materials. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 USDOE Office of Science (SC), Basic Energy Sciences (BES) SC0019001; AC02-76SF00515; AC02-05CH11231; DMR-1720256; CNS-1725797 National Science Foundation (NSF) Author Contributions The manuscript was written by AEL, LF, WG, and CMB. Experiments were designed by AEL, LF, WG, and CMB and performed by AEL, LF, JH, JB, and TZ. Simulations were designed by JL and GHF and performed by JL. All authors have given approval to the final version of the manuscript. |
ISSN: | 0024-9297 1520-5835 |
DOI: | 10.1021/acs.macromol.9b02380 |