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 ...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
104 N. Hadjichristidis, S. Pispas, M. Pitsikalis, H. Iatrou, C. Vlahos<br />
F<strong>in</strong>ally Kosmas and Hadjichristidis [66] by us<strong>in</strong>g a s<strong>in</strong>gle molecule argument<br />
predicted the analytical relations<br />
M = f m , M = M +<br />
n i<br />
i<br />
which l<strong>in</strong>ks the average molecular weights of the homopolymer precursors and<br />
those of the f<strong>in</strong>al miktoarm macromolecule; here, f i is the number of the precursors<br />
of the i-th k<strong>in</strong>d (i=1, 2 ,...n), m ni , m wi , their number and weight average molecular<br />
weight and M w , M n the molecular weights correspond<strong>in</strong>g to the miktoarm<br />
cha<strong>in</strong>. Express<strong>in</strong>g m ni , m wi and M w , M n <strong>in</strong> terms of the Laplace tranform<br />
of the distributions of molecular weights of the precursors P i (m) and the whole<br />
molecule P c (M) they found that both equations at Eq. 6 are valid for any P i (m).<br />
Experimental values of M w based on LALLS and a comb<strong>in</strong>ation of MO and SEC<br />
are found to be close to those calculated from the theory.<br />
3.1.2<br />
Experimental Results<br />
Star polymers, with a structure where cha<strong>in</strong>s of different molecular weight<br />
and/or chemical nature radiate from a common junction po<strong>in</strong>t, are expected to<br />
have different solution behavior compared to regular or symmetric star polymers.<br />
By forc<strong>in</strong>g chemically different arms to be jo<strong>in</strong>ed, expansion of the molecular<br />
dimensions is predicted (see Sect. 3.1.1) as a consequence of the <strong>in</strong>crease <strong>in</strong><br />
the number of heterocontacts <strong>in</strong> good and theta solvents or new k<strong>in</strong>ds of structures<br />
can be formed <strong>in</strong> selective solvents.<br />
The dilute solution properties of asymmetric three-arm polystyrene stars<br />
were studied by Fetters and coworkers [67] under different solvent conditions.<br />
These materials comprised two series of samples, the first hav<strong>in</strong>g a short third<br />
arm with half the molecular weight of the two identical arms (SAS) and the second<br />
a long arm hav<strong>in</strong>g twice the molecular weight of the other two arms (LAS).<br />
In toluene, a good solvent for PS, the two types of asymmetric stars exhibited<br />
identical values of g', def<strong>in</strong>ed as<br />
g'=[h] star /[h] l<strong>in</strong>ear<br />
ni w n<br />
i<br />
fm ( m -m)<br />
i ni wi ni<br />
M<br />
where [h] l<strong>in</strong>ear is the <strong>in</strong>tr<strong>in</strong>sic viscosity of the l<strong>in</strong>ear polymer with the same molecular<br />
weight. Values of g' are a little higher than values of g' for a regular threearm<br />
star. In the theta solvent cyclohexane at 35 °C the value of g' for SAS is lower<br />
than that of LAS which was equal to g' value of regular three-arm stars. It has to<br />
be mentioned that <strong>in</strong> both solvents the value of a <strong>in</strong> the Mark-Houw<strong>in</strong>k-<br />
Sakurada equation, [h]=KM a , was higher for the SAS than LAS. The latter has a<br />
similar a value as the symmetric stars.<br />
The dilute solution characteristics of asymmetric stars, with equal number of<br />
short and long arms, prepared by the DVB method, were studied by Mays et al.<br />
n<br />
(6)<br />
(7)