6742 Themistou and Patrickios
Macromolecules, Vol. 37, No. 18, 2004
4. Table 5 suggests that the lowest sol fraction was
extracted from the N-N network, 6.9%, whose both
types of cores are based exclusively on the more efficient
nonhydrolyzable cross-linker EGDMA. From the other
two networks, the N-H network contained a higher sol
fraction, 20.5%, because its secondary cores, more
essential for gel formation, are based on the hydrolyz-
able DMDMAES cross-linker. The sol fraction from the
H-N network was significantly lower, at 12.7%. From
the MWDs in Figure 9, it seems that the extractables
from all three networks contain a large percentage of
linear chains. Table 5 shows the percentage of the
extractables from each network in linear chains, as
calculated from the areas under the MWDs in Figure
9. The extractables from the N-N network are almost
exclusively linear chains, with 93.0% w/w linear poly-
mer, whereas the linear content of the extractables from
the other two networks are approximately 75% w/w, also
containing a respectable amount of star polymers. These
data are again consistent with the higher cross-linking
efficiency of EGDMA compared to that of DMDMAES,
which would imply that, once formed, star polymers
based on and cross-linked by EGDMA are less likely to
remain unattached to the network.
precursor to the network. Characterization by static
light scattering was possible only on the hydrolysis
product of the H-N network which could dissolve in
THF after precipitation and drying. The absolute MW
was determined to be 1 220 000 g mol-1, in fair agree-
ment with the GPC MW.
Con clu sion s
A novel hydrolyzable silicon-containing dimethacry-
late cross-linker was synthesized and polymerized by
GTP with MMA to prepare star polymers and CSPMNs.
The bulkiness of this cross-linker did not allow a large
number of arms at the cores as with more traditional
dimethacrylate cross-linkers such as EGDMA. The star
polymers and the CSPMNs were hydrolyzed in THF
using hydrochloric acid to give lower MW polymer
products. The star polymers yielded hydrolysis products
with the expected MWs, corresponding to the linear
arms. Although, upon hydrolysis, the CSPMNs readily
dissolved to give homogeneous polymer solutions, the
MWs of the resulting polymers were much higher than
expected, indicating extensive coupling of the star
polymers produced.
Ack n ow led gm en t. The Cyprus Research Promotion
Foundation is gratefully acknowledged for providing
financial support to E.T. via a PENEK 2001 Program.
The A. G. Leventis Foundation is also thanked for a
generous donation, which enabled the purchase of the
NMR spectrometer of the University of Cyprus. The
University of Cyprus Research Committee (Grant 2000-
2003) is thanked for providing funds for the purchase
of the static light scattering spectrophotometer.
Hyd r olysis P r od u cts of th e CSP MNs. The acid
hydrolysis of the H-N and N-H networks was first
confirmed qualitatively by observing the dissolution of
∼1 cm3 pieces of the THF-swollen gel in excess THF
containing HCl, in approximately 5 min. When the
network hydrolysis products were recovered by precipi-
tation in water and vacuum-dried at room temperature,
the redissolution in THF of the products from the N-H
network was impossible, either due to their very high
molecular weight or due to re-formation of some of the
network bonds upon drying. Thus, the hydrolysis prod-
ucts were characterized by GPC from the hydrolysis
solution, without recovery by precipitation. Their MWDs
are displayed in Figure 9, and the calculated MWs are
listed in Table 4. Very high MWs, with Mps at 1 600 000
and 7 400 000 g mol-1, much higher than that of the
“in-out” star precursors, were observed, indicating
interstar linkage.
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