Review of Continuum Mechanics

Review of Continuum Mechanics

7 Review of Continuum Mechanics 7–1 Chapter 7: REVIEW OF CONTINUUM MECHANICS 7–2 TABLE OF CONTENTS Page §7.1. The FEM Discretization 7–3 §7.2. Notation: Continuum vs. Discrete Mechanics 7–3 §7.3. Particles, Motions, Displacements, Configurations 7–4 §7.3.1. Distinguished Configurations ............. 7–4 §7.3.2. Kinematic Descriptions .............. 7–6 §7.3.3. Coordinate Systems ................ 7–7 §7.3.4. Configurations and Staged Analysis .......... 7–8 §7.4. Kinematics 7–8 §7.4.1. Deformation and Displacement Gradients ......... 7–8 §7.4.2. Stretch and Rotation Tensors ............. 7–9 §7.4.3. Green-Lagrange Strain Measure ............ 7–10 §7.4.4. Strain-Gradient Matrix Expressions .......... 7–11 §7.4.5. Pull Forward and Pull Back .............. 7–12 §7.5. Stress Measure 7–12 §7.6. Constitutive Equations 7–13 §7.7. Strain Energy Density 7–14 §7. Exercises ....................... 7–15 7–2 7–3 §7.2 NOTATION: CONTINUUM VS. DISCRETE MECHANICS §7.1. The FEM Discretization In Chapters 3 through 6 we have studied some general properties of the governing force-equilibrium equations of geometricallynonlinear structural systemswith finite number of degrees of freedom (DOF). The DOFs are collected in the state variable vector u. Those residual equations, being algebraic, are well suited for numerical computation. Mathematical models of real structures, however, possess an infinite number of DOFs. As such they cannot be handled bynumerical computations. The reduction to a finite number is accomplished by discretization methods. As noted in Chapter 1, for nonlinear problems in solid and structural mechanics the finite element method (FEM) is the most widelyused discretization method. This section provides background material for the derivation of geometricallynonlinear finite elements. The material gives a review of kinematic, kinetic and constitutive concepts from the three-dimensional continuum mechanics of an elastic deformable body, as needed in following Chapters. Readers familiar with continuum mechanics should peruse it to grab notation. §7.2. Notation: Continuum vs. Discrete Mechanics Continuum mechanics deals with vector and tensor fields such as displacements, strains and stresses. Four types of notation are in common use: 1. Indicial Notation. Also called component notation. This notation uses indexed components along with abbreviation rules such as commas for partial derivatives and Einstein’s summation convention. It is a powerful notation, and as such is preferred in journals and monographs. It has the advantage of readilyhandling arbitrarytensors of anyorder, arbitrarycoordinate systemsand nonlinear relations. It sharplydistinguishes between covariant and contravariant quantities, which is necessaryin non- Cartesian coordinates. Tends to conceal or mask intrinsic properties, however, and as such is not suitable for basic instruction. 2. Direct Notation. Sometimes called algebraic notation. Vectors and tensors are represented bysingle symbols, usually bold letters. Has the advantage of compactness and quick visualization of intrinsic properties. Some operations correspond to matrix notations while others do not. This fuzzyoverlap can lead to confusion in FEM work. 3. Matrix Notation. This is similar to the previous one, but entities are rearranged as appropriate so that onlymatrix operations are used. It can be translated directlyto discrete equations as well as matrix-oriented programming languages such as Matlab. It has the disadvantage of losing contact with the original physical entities along the way. For example, stress is a symmetric second-order tensor that is rearranged as a 6-component vector for FEM developments. This change loses essential properties. For instance it makes sense to talk of principal stresses as eigenvalues of the stress tensor. But those get lost (as or least moved to the background) when rearranged as a stress vector. 4. Full Notation. In the full-form notation everyterm is spelled out. No ambiguities of interpretation can arise; consequentlythis works well as a notation of last resort, and also as a “comparison template” against one can check out the meaning of more compact expressions. It is also useful for programming in low-order languages. As an example, consider the well known dot product between two physical vectors in 3D space, a = (a1, a2, a3) and b = (b1, b2, b3) done in the four different notations: = . = T = + + .(. ) ai bi a b a b a1b1 a2b2 a3b3 7 1 indicial direct matrix full 7–3 Chapter 7: REVIEW OF CONTINUUM MECHANICS 7–4 In the following review the direct, matrix and full notation are preferred, whereas the indicial notation is avoided. Usuallythe expression is first given in direct form and confirmed byfull form if feasible. Then it is transformed to matrix notation for later used in FEM developments. The decision leads to possible ambiguities against reuse of vector symbols in two contexts: continuum mechanics and FEM discretizations. Such ambiguities are resolved in favor of keeping FEM notation simple. §7.3. Particles, Motions, Displacements, Configurations In the present section a structure is mathematicallytreated as a continuum body B. The bodyis considered as being formed bya set of points P called particles, which are endowed with certain mechanical properties. For FEM analysis the body is divided into elements. Particles displace or move in response to external actions characterized bycontrol parameters i or, following the stage reduction discussed in Chapter 3, the single stage parameter λ. A one-parameter series of positions occupied bythe particles as theymove in space is called a motion. The motion may be described bythe displacement u(P) ≡ u(x) of the particles with respect to a base or reference state in which particle P is labelled P0. [The underlining is used to distinguish the physical displacement vector from the finite element node displacement array, which is a computational vector.] The displacements of all particles u(x, y, z) such that x ≡ x, y, z ∈ B, constitutes the displacement field. The motion is said to be kinematically admissible if: 1. Continuityof particles positions is preserved so that no gaps or voids appear. (The mathematical statement of this condition is given later.) 2. Kinematic constraints on the motion (for example, support conditions) are preserved. A kinematicallyadmissible motion along a stage will be called a staged motion. For one such motion the displacements u(x) characterize the state and the stage control parameter λ characterizes the control or action. Both will be generallyparametrized bythe pseudo-time t introduced in Chapter 3, so that a staged motion can be generallyrepresented by λ = λ(t), u = u(x, t), x ∈ B. (7.2) If in these equations we freeze t,wehaveaconfiguration of the structure. Thus a configuration is formallythe union of state and control. It maybe informallyviewed as a “snapshot” taken of the structure and actions upon it when the pseudotime is frozen. If the configuration satisfies the equilibrium equations, it is called an equilibrium configuration. In general, however, a randomlygiven configuration is not in equilibrium unless artificial bodyand surface forces are applied to it. A staged response, or simply response, can be now mathematicallydefined as a series of equilibrium configurations obtained as λ is continuouslyvaried. §7.3.1. Distinguished Configurations A particular characteristic of geometricallynonlinear analysisis the need to carefullydistinguish among different configurations of the structure. As noted above, each set of kinematicallyadmissible displacements u(x) plus a staged control parameter λ defines a configuration. This is not necessarilyan equilibrium configuration; in fact it will not usually 7–4 7–5 §7.3 PARTICLES, MOTIONS, DISPLACEMENTS, CONFIGURATIONS Table 7.1 Distinguished Configurations in Nonlinear Analysis Name Alias Definition Equilibrium Identification Required? Admissible A kinematicallyadmissible configuration No C Perturbed Kinematicallyadmissible variation No C + δC of an admissible configuration. Deformed Current Actual configuration taken during No C D or C(t) Spatial the analysis process. Contains others as special cases. Base∗ Initial The configuration defined as the Yes C0, C B or C(0) Undeformed origin of displacements. Strain free but Material not necessarilystress free. Reference Configuration to which stepping TL,UL: Yes. TL: C0, UL: Cn−1, computations are referred CR: C R no, C0 yes CR: C R and C0 th Cn Iterated† Configuration taken at the k No k iteration of the nth increment step Target† Equilibrium configuration accepted Yes Cn at the nth increment step Corotated‡ Shadow Bodyor element-attached configuration No C R Ghost obtained from C0 through a rigid bodymotion (CR description only) Aligned Preferred A fictitious bodyor element configuration No C A Directed aligned with a particular set of axes (usuallyglobal axes) ∗ C0 is often the same as the natural state in which body(or element) is undeformed and stress-free. † Used onlyin the description of solution procedures. ‡ In dynamic analysis C0 and C R are called the inertial and dynamic-reference configurations, respectively, when they apply to the entire structure. be one. It is also important to realize that an equilibrium configuration is not necessarilya physical configuration assumed bythe actual structure. 1 Some configurations that are important in geometricallynonlinear analysisreceive special qualifiers: admissible, perturbed, deformed, base, reference, iterated, target, corotated, aligned This terminologyis collected in Table 7.1.

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