Bulletin of the American Physical Society
APS March Meeting 2020
Volume 65, Number 1
Monday–Friday, March 2–6, 2020; Denver, Colorado
Session U32: Polymers with Special Architectures: From Molecular Design to Physical Properties I
2:30 PM–5:30 PM,
Thursday, March 5, 2020
Room: 504
Sponsoring
Units:
DPOLY DSOFT
Chair: Reika Katsumata, Univ of Mass - Amherst
Abstract: U32.00007 : Effect of Branches and Cycles on Polymer Melt Surface Dynamics*
Presenter:
Mark Foster
(Dept. of Polymer Science, University of Akron)
Author:
Mark Foster
(Dept. of Polymer Science, University of Akron)
The dynamics of the thermally stimulated surface height fluctuations in a polymer melt dictate wetting, adhesion, and tribology at that surface. These surface fluctuations can be profoundly altered by tethering of the chains. One type of tethering is the tethering of one part of a molecule to another part of the same molecule. This tethering is found in both long chain branched polymers and in macrocycles. We have studied the surface fluctuations with X-ray Photon Correlation Spectroscopy for melts of well-defined, anionically polymerized polystyrenes of various architectures, including linear, 6 arm star, pom-pom, comb and cyclic architectures. For linear chains, the variation of surface relaxation time with in-plane scattering vector can be fit using a hydrodynamic continuum theory (HCT) of thermally stimulated capillary waves that knows nothing of the chain architecture. Assuming the theory is applicable, apparent viscosities of the films may then be inferred from the XPCS data. For unentangled linear chains, the viscosity inferred from XPCS data for sufficiently thick films is the same as that measured by conventional bulk rheometry. For star-branched chains the film thickness relative to chain size must be much larger to obtain this agreement. Densely branched combs, cyclic and bicyclic chains show yet another behavior. It appears these differences are related to the manner in which the chains organize at the substrate interface.
*Acknowledgement: Thanks to the Advanced Photon Source, supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Science, under contract No. W-31-109-ENG-38.
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