Chapter 4: Problem 28
Let \(B=\left\\{\boldsymbol{X} \in \mathbb{E}^{3} \mid 0
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Chapter 4: Problem 28
Let \(B=\left\\{\boldsymbol{X} \in \mathbb{E}^{3} \mid 0
These are the key concepts you need to understand to accurately answer the question.
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Let \(B=\mathbb{E}^{3}\) and consider the motion \(\boldsymbol{x}=\boldsymbol{\varphi}(\boldsymbol{X}, t)\) defined by $$ x_{1}=(1+t) X_{1}, \quad x_{2}=X_{2}+t X_{3}, \quad x_{3}=X_{3}-t X_{2} $$ Moreover, consider the spatial field \(\phi(\boldsymbol{x}, t)=t x_{1}+x_{2}\) (a) Show that \(\operatorname{det} \boldsymbol{F}(\boldsymbol{X}, t)>0\) for all \(t \geq 0\) and find the components of the inverse motion \(\boldsymbol{X}=\boldsymbol{\psi}(\boldsymbol{x}, t)\) for all \(t \geq 0\) (b) Find the components of the spatial velocity field \(\boldsymbol{v}(\boldsymbol{x}, t)\). (c) Find the material time derivative of \(\phi\) using the definition \(\dot{\phi}=\left[\dot{\phi}_{m}\right]_{s}\) (d) Find the material time derivative of \(\phi\) using Result 4.7. Do you obtain the same result as in part (c)?
Let \(\boldsymbol{F}=\boldsymbol{R} \boldsymbol{U}=\boldsymbol{V} \boldsymbol{R}\) be the right and left polar decompositions of a deformation gradient \(\boldsymbol{F} .\) Show that: (a) \(\boldsymbol{U}\) and \(\boldsymbol{V}\) have the same eigenvalues, (b) if \(\left\\{\boldsymbol{u}_{i}\right\\}\) is a frame of eigenvectors of \(\boldsymbol{U}\), then \(\left\\{\boldsymbol{R} \boldsymbol{u}_{i}\right\\}\) is a frame of eigenvectors of \(\boldsymbol{V}\). Thus, in general, \(\boldsymbol{U}\) and \(\boldsymbol{V}\) have different eigenvectors.
Let \(B=\mathbb{E}^{3}\) and consider the motion \(\boldsymbol{x}=\boldsymbol{\varphi}(\boldsymbol{X}, t)\) defined by $$ x_{1}=e^{t} X_{1}+X_{3}, \quad x_{2}=X_{2}, \quad x_{3}=X_{3}-t X_{1} $$ (a) Show that the inverse motion \(\boldsymbol{X}=\boldsymbol{\psi}(\boldsymbol{x}, t)\) is given by $$ X_{1}=\frac{x_{1}-x_{3}}{t+e^{t}}, \quad X_{2}=x_{2}, \quad X_{3}=\frac{t x_{1}+e^{t} x_{3}}{t+e^{t}} $$ (b) Verify that \(\boldsymbol{\varphi}(\boldsymbol{\psi}(\boldsymbol{x}, t), t)=\boldsymbol{x}\) and \(\boldsymbol{\psi}(\boldsymbol{\varphi}(\boldsymbol{X}, t), t)=\boldsymbol{X}\).
Consider an arbitrary rigid motion \(\varphi: B \times[0, \infty) \rightarrow \mathbb{E}^{3}\) of the form $$ \boldsymbol{\varphi}(\boldsymbol{X}, t)=\boldsymbol{R}(t) \boldsymbol{X}+\boldsymbol{c}(t) $$ where \(\boldsymbol{R}(t)\) is a rotation tensor and \(\boldsymbol{c}(t)\) is a vector. (a) Find the inverse motion \(\boldsymbol{\psi}(\boldsymbol{x}, t)\). (b) Let \(\boldsymbol{\Omega}(t)=\dot{\boldsymbol{R}}(t) \boldsymbol{R}(t)^{T} .\) Show that \(\boldsymbol{\Omega}(t)\) is skew-symmetric. (c) Show that the spatial velocity field can be written in the form $$ \boldsymbol{v}(\boldsymbol{x}, t)=\boldsymbol{\Omega}(t)(\boldsymbol{x}-\boldsymbol{c}(t))+\dot{\boldsymbol{c}}(t). $$
For each deformation \(\boldsymbol{x}=\boldsymbol{\varphi}(\boldsymbol{X})\) given below find the components of the deformation gradient \(\boldsymbol{F}\) and determine if \(\varphi\) is homogeneous or non-homogeneous: (a) \(x_{1}=X_{1}, \quad x_{2}=X_{2} X_{3}, \quad x_{3}=X_{3}-1\), (b) \(x_{1}=2 X_{2}-1, \quad x_{2}=X_{3}, \quad x_{3}=3+5 X_{1}\) (c) \(x_{1}=\exp \left(X_{1}\right), \quad x_{2}=-X_{3}, \quad x_{3}=X_{2}\).
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