142 Advances in Polymer Science Editorial Board: A. Abe. A.-C ...
142 Advances in Polymer Science Editorial Board: A. Abe. A.-C ...
142 Advances in Polymer Science Editorial Board: A. Abe. A.-C ...
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Asymmetric Star <strong>Polymer</strong>s Synthesis and Properties 77<br />
Scheme 2<br />
arms by fractionation, the f<strong>in</strong>al products and the different k<strong>in</strong>d of arms, which<br />
were isolated before the coupl<strong>in</strong>g reaction, were characterized by membrane osmometry<br />
(MO) and static light scatter<strong>in</strong>g (SLS), reveal<strong>in</strong>g that well def<strong>in</strong>ed star<br />
polymers were prepared.<br />
Us<strong>in</strong>g the same procedure Pennisi and Fetters prepared a series of asymmetric<br />
polybutadiene (PB) stars <strong>in</strong> which the third arm was of variable molecular<br />
weight [2]. It was found more efficient to add the liv<strong>in</strong>g PB solution to the methyltrichlorosilane<br />
l<strong>in</strong>k<strong>in</strong>g agent <strong>in</strong> order to reduce the formation of the coupled<br />
byproduct. Similar characterization techniques were also employed <strong>in</strong> this case.<br />
Asymmetric polyisoprene (PI) three-arm stars with variable length of the<br />
third arm were synthesized us<strong>in</strong>g the same method [8]. The reaction of the liv<strong>in</strong>g<br />
PI cha<strong>in</strong>s with excess methyltrichlorosilane was performed at 5 °C. This low<br />
temperature was selected <strong>in</strong> an effort to m<strong>in</strong>imize the coupled byproduct. Nevertheless<br />
the reduced steric h<strong>in</strong>drance of the PILi cha<strong>in</strong> end <strong>in</strong> association with<br />
the low molecular weight of the polydienes used (M n =5500 and 1100) led to the<br />
formation of an appreciable amount of the coupled byproduct, which was later<br />
separated by fractionation, with the excess of the last coupled arm, us<strong>in</strong>g a solvent-precipitant<br />
system. Pure products were f<strong>in</strong>ally isolated as evidenced by the<br />
molecular characterization techniques used (SEC, MO, SLS).<br />
Asymmetric PS stars of the type (PS A ) n (PS B ) n were also prepared by the div<strong>in</strong>ylbenzene<br />
(DVB) method [9]. Liv<strong>in</strong>g PS cha<strong>in</strong>s, prepared by sec-BuLi <strong>in</strong>itiation, were<br />
reacted with a small amount of DVB produc<strong>in</strong>g star homopolymers. The DVB core<br />
of the stars conta<strong>in</strong>s active anions which, if no accidental deactivation occurs, are<br />
equal to the number of the arms that have been l<strong>in</strong>ked to this core. These active<br />
sites are available for the polymerization of an additional quantity of monomer.<br />
Consequently further addition of styrene produced asymmetric star polymers