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142 Advances in Polymer Science Editorial Board: A. Abe. A.-C ...

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78 N. Hadjichristidis, S. Pispas, M. Pitsikalis, H. Iatrou, C. Vlahos<br />

hav<strong>in</strong>g n branches with molecular weight A and n branches with molecular weight<br />

B. A small quantity of THF was used to accelerate the second polymerization step.<br />

The last method for the synthesis of asymmetric stars suffers from the disadvantages<br />

that characterizes the DVB method: the broad molecular weight distributions,<br />

compared to stars prepared by chlorosilane chemistry, molecular heterogeneity,<br />

s<strong>in</strong>ce n is an average value, absence of complete control over the f<strong>in</strong>al<br />

product etc. More details will be given <strong>in</strong> Sect. 2.2.1.1. SEC analysis revealed the<br />

existence of high molecular weight species. This was attributed to the formation<br />

of l<strong>in</strong>ked stars. These structures can be produced when active anionic liv<strong>in</strong>g<br />

arms react with other DVB-l<strong>in</strong>ked cores. It is evident from the above that the<br />

products are not as pure as those produced by suitable chlorosilane chemistry.<br />

Asymmetric three-arm PS stars, possess<strong>in</strong>g cha<strong>in</strong>s of different molecular<br />

weights were also prepared by Quirk and Yoo [10] us<strong>in</strong>g 1,4-bis(1-phenylethenyl)benzene<br />

(PDDPE) as the l<strong>in</strong>k<strong>in</strong>g agent. It was observed that the addition reaction<br />

of polystyryllithium with PDDPE <strong>in</strong> THF leads primarily to the formation<br />

of the monoadduct product, due to the ability of the negative charge to be delocalized<br />

<strong>in</strong>to the phenyl r<strong>in</strong>gs and the rema<strong>in</strong><strong>in</strong>g v<strong>in</strong>yl group. The formation of this<br />

product was then followed by the addition of the second polystyryllithium cha<strong>in</strong><br />

<strong>in</strong> order to obta<strong>in</strong> the coupled product. The efficiency of the coupl<strong>in</strong>g reaction depends<br />

on the control of the stoichiometry between the reactants. F<strong>in</strong>ally the addition<br />

of styrene <strong>in</strong> the presence of THF to promote the crossover reaction leads<br />

to the formation of the asymmetric PS stars, as shown <strong>in</strong> Scheme 2. Unreacted<br />

monoadduct product and PS B homopolymer (the second arm) were also observed<br />

<strong>in</strong> the SEC trace of the f<strong>in</strong>al product due to <strong>in</strong>complete l<strong>in</strong>k<strong>in</strong>g reactions.<br />

2.2<br />

Stars with Chemical Symmetry<br />

2.2.1<br />

Miktoarm Stars<br />

Star polymers of chemically different arms are usually called miktoarm stars.<br />

Although there are several <strong>in</strong>dividual methods for the synthesis of miktoarm<br />

stars four general methodologies have been developed. Three of them are based<br />

on anionic polymerization and the fourth on cationic polymerization. In all of<br />

them the use of appropriate l<strong>in</strong>k<strong>in</strong>g agents is necessary.<br />

2.2.1.1<br />

General Strategies and Methods<br />

2.2.1.1.1<br />

Anionic <strong>Polymer</strong>ization Method with Div<strong>in</strong>ylbenzene (DVB)<br />

The synthesis of miktoarm stars by the DVB method is a three step procedure.<br />

The first step <strong>in</strong>volves the preparation of the liv<strong>in</strong>g arm by anionic polymeriza-

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