Neil McCartney

Properties for Design of Composite Structures


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href="#ulink_2a4bcde2-c305-5db1-bdb6-95d1b181fc94">2.22) that

(2.25)

      where use has been made of the following identity

      On using the divergence theorem, the identity (2.25) may then be written as

      The first term on the right-hand side accounts for any changes of the property ϕ locally at points within the region V, whereas the second term accounts for the mean advection of the property across the bounding surface S where n is the outward unit normal to the surface S bounding the region V. The important identities (2.22) and (2.27) are used repeatedly in the following analysis.

      2.6 Continuity Equation

      Consider at time t a moving sample of material occupying a fixed volume V bounded by a closed surface S. In the absence of mass source and sink terms, the total mass of material within the region V is fixed so that on setting ϕ = ρ in (2.27) the global form of the mass balance equation for the medium may be written as

      As (2.29) must be valid for any region V of the system, the following local form of the mass balance equation for the medium must be satisfied at all points in the system for all times t

      On using (2.22) and the identity (2.26), the continuity equation (2.30) may be written in the equivalent form

      2.7 Equations of Motion and Equilibrium

      The global form of the linear momentum balance equation for a fixed region V bounded by the closed surface S having outward unit normal n is written as

      where σ is the stress tensor and where b is the body force per unit mass acting on the medium. Such body forces usually arise from the effects of gravity. On using (2.27) and the divergence theorem, the linear momentum balance equation (2.32) may be written as

      As relation (2.33) must be satisfied for any region V of the system, it follows that the local form of the linear momentum balance equation has the form

      As

      nabla period left-parenthesis rho v v right-parenthesis identical-to rho v nabla period v plus v period nabla left-parenthesis rho v right-parenthesis comma(2.35)

      it follows from (2.34) on using (2.22) that

      On using (2.31), relation (2.36) reduces to the well-known equation of motion