Differential approximation for viscoelasticity (Q1343030)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Differential approximation for viscoelasticity |
scientific article; zbMATH DE number 716116
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Differential approximation for viscoelasticity |
scientific article; zbMATH DE number 716116 |
Statements
Differential approximation for viscoelasticity (English)
0 references
10 September 1995
0 references
The paper pertains to the field of evolution equations containing hereditary effect due to the time non-locality which produces dissipation, and the goal is to devise approximate equations which accurately reproduce dissipation. \textit{R. C. MacCamy} [J. Math. Anal. Appl. 179, No. 1, 120-134 (1993; Zbl 0790.34059)] studied the equations of parabolic nature. Here the authors are dealing with the hyperbolic case by taking as a model the displacement problem \(P(\mu,\lambda)[b,u_ 0,u_ 1]\) of the linear, isotropic, and homogeneous viscoelasticity. The constitutive equation of the viscoelastic body is \(\sigma(x,t) = {\partial\over \partial t} \int^ t_{-\infty} L(\mu(t-r), \lambda(t - r)) [u(x,r)]dr\), where \(\sigma\) is the stress tensor, \(u\) denotes the displacement, \(\mu\) and \(\lambda\) are functions on \([0,\infty)\) characterizing the viscoelastic body, and \(L(\mu,\lambda)[u] = 2\mu E[u] + 2\lambda \text{tr }E [u]I\), \(E[u] = [\nabla u + \nabla u^ T]/2\). It is assumed that \(u\) is zero up to time \(t = 0\), and the density is taken equal to one. Under these conditions the problem \(P(\mu,\lambda) [b,u_ 0,u_ 1]\) takes the form \(\ddot u(x,t) = {\partial\over \partial t} \int^ t_ 0 \text{div }L(\mu(t - r),\lambda(t - r))[u (r,t)] dr + b(x,t)\) in \(\Omega\), \(u(x,t) = 0\) on \(\partial \Omega\), \(u(\cdot,0) = u_ 0\), \(\dot u(\cdot,0) = u_ 1\), where the dot indicates time derivative, \(b\) is the body force, \(\Omega\) is a bounded three- dimensional region representing a fixed configuration of the body, and \(u_ 0\), and \(u_ 1\) are given functions on \(\Omega\). The corresponding approximate problem is studied by using the procedure of the above mentioned work of MacCamy. The paper is of real theoretical and practical interest.
0 references
hereditary effect
0 references
dissipation
0 references
approximate equations
0 references
hyperbolic case
0 references
constitutive equation
0 references
0 references