INFLUENCE OF INCLUSION MICROGEOMETRY ON SOME THERMOMECHANICAL PROPERTIES OF ISOTROPIC POLYMER-MATRIX COMPOSITES

Authors
Citation
J. Li et Gj. Weng, INFLUENCE OF INCLUSION MICROGEOMETRY ON SOME THERMOMECHANICAL PROPERTIES OF ISOTROPIC POLYMER-MATRIX COMPOSITES, Journal of engineering materials and technology, 119(3), 1997, pp. 242-250
Citations number
23
Categorie Soggetti
Engineering, Mechanical","Material Science
ISSN journal
00944289
Volume
119
Issue
3
Year of publication
1997
Pages
242 - 250
Database
ISI
SICI code
0094-4289(1997)119:3<242:IOIMOS>2.0.ZU;2-1
Abstract
The influence of inclusion shape on some selected thermomechanical pro perties of isotropic viscoelastic composites is investigated by a micr omechanical theory. These properties include: (i) the cyclic stress-st rain behavior; (ii) cyclic creep; (iii) the master compliance curve; a nd (iv) the effective thermal expansion coefficient. It is found that these viscoelastic properties are all strongly dependent upon the incl usion shape. Specifically, under a strain-controlled cyclic loading th e transient stress-strain curves of the composites all exhibit cyclic hardening behavior, but the level of flow stress reached is controlled by the inclusion shape. Except for the disk-reinforced case the per-c ycle energy loss of the composite at 20 percent of inclusion concentra tion is found to be greater than the loss of the pure viscoelastic mat rix. The complex shear modulus of the composite with various inclusion shapes is shown to lie on or within Milton and Berryman's bounds (199 7). Creep under cyclic stress tends to oscillate around the creep curv e under a constant, mean stress for all inclusion shapes, with disks s howing the greatest resistance. To uncover the influence of temperatur e, the creep compliance of the composite with a thermorheologically si mple matrix is investigated and it is demonstrated that the compliance curves at various temperatures can all be plotted into a single maste r one on a reduced time scale. Finally, the effective thermal expansio n coefficient of the composite is shown to be generally time-dependent , but the degree of time-dependence is low with spherical inclusions a nd very high with disks, others lying in-between.