We
investigated the morphology formed in the binary blend of six-arm
star-shaped (poly(methyl methacrylate)-block-polystyrene)6 copolymer [(PMMA-b-PS)6] and
PMMA-b-PS linear diblock copolymer by varying their
molecular weights as well as volume fractions of the blocks. When
the molecular weight of PMMA-b-PS is much larger
(> ∼4) than that of one arm of (PMMA-b-PS)6, PMMA-cylindrical microdomains are formed even though the
volume fraction of PMMA (f
PMMA) in both
(PMMA-b-PS)6 and PMMA-b-PS is nearly symmetric (f
PMMA ∼0.5).
On the other hand, when the ratio of molecular weights between these
two copolymers is not large, lamellar morphology is observed in the
blend as expected. Very interestingly, we found that even for a binary
blend with the overall volume fraction of the PMMA block (f̅
PMMA) as large as 0.71, the major PMMA
blocks still aggregate into cylindrical microdomains, and thus, “inverted
cylinders” are formed, although PS-cylinders are observed in
the neat (PMMA-b-PS)6 and PMMA-b-PS melts. This interesting inverted cylinder is mainly
stabilized by two factors. On the one hand, the long linear diblock
copolymer swells the domain significantly, thus preventing the short
(PMMA-b-PS)6 star copolymer from forming
the favorable bridging configurations in order to avoid the high stretching
energy. As long as the bridging configurations are prohibited, the
PMMA-core blocks of (PMMA-b-PS)6 prefer
to stay inside the curvature, amplifying the tendency of forming a
spontaneous curvature toward PMMA-blocks. On the other hand, the radial
distribution of the long PMMA-block of the diblock and the short PMMA-block
of the star increases the spontaneous curvature. The experimental
results as well as the formation of the inverted cylinders have been
verified by self-consistent field theory (SCFT).