STRUCTURE AND DYNAMICS OF STRUCTURE FORMATION IN MODEL TRIARM STAR BLOCK-COPOLYMERS OF POLYSTYRENE, POLY(ETHYLENE OXIDE), AND POLY(EPSILON-CAPROLACTONE)

Citation
G. Floudas et al., STRUCTURE AND DYNAMICS OF STRUCTURE FORMATION IN MODEL TRIARM STAR BLOCK-COPOLYMERS OF POLYSTYRENE, POLY(ETHYLENE OXIDE), AND POLY(EPSILON-CAPROLACTONE), Macromolecules, 31(21), 1998, pp. 7279-7290
Citations number
32
Categorie Soggetti
Polymer Sciences
Journal title
ISSN journal
00249297
Volume
31
Issue
21
Year of publication
1998
Pages
7279 - 7290
Database
ISI
SICI code
0024-9297(1998)31:21<7279:SADOSF>2.0.ZU;2-B
Abstract
The structure and dynamics of structure formation have been studied in model triarm star block copolymers composed of two crystallizable blo cks (poly(ethylene oxide) (PEO) and poly(epsilon-caprolactone) (PCL)) and one amorphous block (polystyrene(PS)). Crystallization starts from the homogeneous phase. For the structure investigation, X-ray scatter ing, optical microscopy, and atomic force microscopy have been employe d, whereas for the kinetics, we have used differential scanning calori metry, optical microscopy, and rheology. In the stars, there is a comp etition for crystallization between the two crystallizable blocks whic h have similar mobilities and melting temperatures but crystallize in different unit cells (monoclinic vs orthorhombic). When the crystalliz able block length ratio is 3 or higher, only the longer block will cry stallize. For comparable lengths both blocks can crystallize-however, not within the same molecule-but the crystallinity, long period, and c rystalline lamellar thickness are reduced with respect to the pure PEO and PCL. The latent heats, obtained in the isothermal crystallization calorimetric experiments, are analyzed in terms of the Avrami theory. Although similar Avrami exponents were found for all stars (n = 2, re flecting a disklike growth from heterogeneous nuclei), the crystalliza tion times were different depending on the nature of the crystallizabl e blocks. Optical microscopy revealed the formation of different super structures (spherulites/axialites) depending on the type of crystalliz able block (PEO/PCL). The growth rates of these superstructures were o btained and analyzed in terms of a kinetic nucleation theory, and the fold surface free energies were extracted. Notwithstanding the larger specific surface of bulk PCL as compared to that of PEG, the fold surf ace free energies in the stars were similar to that in PEG, indicating a pure PEO crystal and mixing of the amorphous blocks with the PCL cr ystal. This is supported from the results of the atomic force microsco py measurements on thin films, which have indicated the formation of p erforated PCL crystals.