TY - JOUR
T1 - Effect of number of arms on diffusion of star polymers
AU - Shull, Kenneth R.
AU - Kramer, Edward J.
AU - Fetters, Lewis J.
PY - 1990/1/1
Y1 - 1990/1/1
N2 - UNLIKE small-molecule liquids, polymer melts can display complex and often highly non-newtonian flow behaviour, which reflects the dynamics of the entangled polymer chains. Star-branched polymers, which have f arms each containing Na monomeric units, joined covalently at a common branch point, provide good model systems for understanding the slow dynamics of branched polymers. These dynamics may be probed by measurement of the diffusion coefficient, D. It is well established1-3 that for three-armed star polymers, Dα exp(-αNa), where α is a constant. This result is consistent with early theories4,5, which assumed that to diffuse, all but two arms of the star must retract simultaneously to the branch point; these theories predict Dα exp(-α(f-2)Na). Here we present experimental measurements of D for polymers with f = 3-12, which indicate a much weaker decrease with f: Dα exp (-0.41f). This result is consistent with more recent theories6 which predict that a star can diffuse by retracting just one arm at a time.
AB - UNLIKE small-molecule liquids, polymer melts can display complex and often highly non-newtonian flow behaviour, which reflects the dynamics of the entangled polymer chains. Star-branched polymers, which have f arms each containing Na monomeric units, joined covalently at a common branch point, provide good model systems for understanding the slow dynamics of branched polymers. These dynamics may be probed by measurement of the diffusion coefficient, D. It is well established1-3 that for three-armed star polymers, Dα exp(-αNa), where α is a constant. This result is consistent with early theories4,5, which assumed that to diffuse, all but two arms of the star must retract simultaneously to the branch point; these theories predict Dα exp(-α(f-2)Na). Here we present experimental measurements of D for polymers with f = 3-12, which indicate a much weaker decrease with f: Dα exp (-0.41f). This result is consistent with more recent theories6 which predict that a star can diffuse by retracting just one arm at a time.
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U2 - 10.1038/345790a0
DO - 10.1038/345790a0
M3 - Article
AN - SCOPUS:0025435772
SN - 0028-0836
VL - 345
SP - 790
EP - 791
JO - Nature
JF - Nature
IS - 6278
ER -