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 103<br />
Accord<strong>in</strong>g to the simulation results the mean conformation achieved by the<br />
miktoarm stars <strong>in</strong> solution is characterized by a significant deformation along<br />
the arms, ma<strong>in</strong>ly near the star center where the possibility of <strong>in</strong>teractions is<br />
high and a change <strong>in</strong> the relative orientation of the vectors c anci cB (cie-<br />
term<strong>in</strong>ed fiom their angle) extends the center of mass separat~on <strong>in</strong> or2er to<br />
dim<strong>in</strong>ish the repulsions. The results show that both mechanisms have a similar<br />
<strong>in</strong>fluence on the <strong>in</strong>crease of the < G: , > . The values of the ratio showever<br />
correspond<strong>in</strong>g to an artificial segreggtpd model (also considered <strong>in</strong> this work)<br />
are very large compared to the value of a s<strong>in</strong>gle cha<strong>in</strong> <strong>in</strong> various solvents. It is<br />
concludeci that <strong>in</strong> dilute solutions the miktoarm cha<strong>in</strong> does not segregate <strong>in</strong>tramolecularly.<br />
As <strong>in</strong> the previous case experimental results are not available.<br />
Vlahos et al. [65] have determ<strong>in</strong>ed the dimensionless ratio s,;<br />
by <strong>in</strong>tr<strong>in</strong>sic<br />
viscosity analysis for the A,B and A,B miktoarm stars <strong>in</strong> various solvent conditions.<br />
Consider<strong>in</strong>g the ratios gs* and gSg<br />
to be close to 1 for the particular<br />
miktoarms studied <strong>in</strong> this work they arrived at the follow<strong>in</strong>g equations:<br />
F<br />
h s h s h<br />
F<br />
F<br />
h s h s h<br />
F<br />
Monte Carlo calculations based on the lower bound method were applied to<br />
estimate the Flory parameter Ffor<br />
asymmetric stars, whereas, for the symmetric<br />
stars, experimental results on three- and four-arm homopolymer stars were<br />
used. The obta<strong>in</strong>ed values of s for different macroscopic states together with<br />
those obta<strong>in</strong>ed from RG and MC calculations are presented <strong>in</strong> Table 2. p is the<br />
ratio of the lengths of the B and A arms (p=NH/NA).<br />
Table 2. The ratio s,<br />
of miktoarm stars 122,651<br />
Coxlxlorl good MC RG Exp.<br />
A,B (p-1) 1.294k0.005 1.249<br />
A,B (p=1.7) 1.289k0.006 1.238<br />
A4 (p=2) 1.342k0.010 1.316<br />
A,B (p-3.9) 1.241k 0.017 1.262<br />
Selective ( qfor<br />
A)<br />
A2B (p=l) 1.419k0.005 1.374<br />
A,<br />
F<br />
F<br />
F<br />
F