Abstract
This paper develops a dynamic finite-strain plate theory consistent with three-dimensional Hamilton’s principle under general loadings with a fourth-order error. Starting from the three-dimensional field equations for a compressible hyperelastic material and by a series expansion about the bottom surface, we deduce a vector dynamic plate equation with three unknowns, which exhibits the local momentum-balance structure. Associated weak formulations are considered, in connection with various boundary conditions. Then, by linearization, we provide a novel linear plate theory for orthotropic materials, which takes into account both stretching and bending effects. For isotropic materials, it is further modified to a refined linear plate theory, leading to higher-order results under certain circumstances. To verify the present plate theory, an exhaustive study of the free vibration and static bending problems is carried out. Comparing with the available exact three-dimensional solutions for these problems, it is shown that the plate theory indeed provides correct asymptotic results for displacements and stresses distributions. The advantages of this linear plate theory include (i) its simplicity (as simple as the Kirchhoff-Love theory), (ii) high accuracy for frequencies and deflections, as well as capability of capturing the distributions of all concerned quantities, and (iii) applicability for general loadings.
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Notes
The general formula is \(\bar{\mathbf{x}}=\sum_{k=0}^{n} \frac{2^{k}}{(k+1)!} h^{k} \mathbf {x}^{(k)} + O(h^{n+1})\), and we will use the high-order terms in Sect. 6.2 to calculate the high-order results for frequency.
There is no need to distinguish the moduli tensor associated with different pairs of conjugate stress-strain variables for small-strain cases.
For the foundation case, we should substitute \(\mathbf{q}^{-}=-k_{s} x_{3}^{(0)} \mathbf{k}\) or \(q_{j}^{-}=-k_{s} x_{3}^{(0)} \delta_{3j}\).
Symmetric (antisymmetric) means in-plane displacements are symmetric (antisymmetric) about mid-plane, and it is reversed for the transverse displacement.
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Acknowledgements
The work described in this paper was supported by a GRF grant (Project No.: CityU 11303015) from the Research Grants Council of Hong Kong SAR, China and a grant from the National Nature Science Foundation of China (Project No.: 11572272).
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Appendices
Appendix A: Recursion Relations and Moduli Tensors in the Linear Case
The component forms of (42) and (41)1 read
where
It is easy to verify the symmetry and the special values
which imply that \(S_{m i}^{(0)}\) in (110) does not involve \({x}_{3}^{(0)}\) and \(S_{m 3}^{(0)}\) only involves \(q_{k}^{-}\). Furthermore, for isotropic or orthotropic materials, \(\tilde{\mathbb{B}}\) is always a diagonal matrix, and as a result
which imply that \({x}_{\gamma}^{(1)}\) in (110) only involves derivatives of \({x}_{3}^{(0)}\), while \({x}_{3}^{(1)}\) only involves the derivatives of \({x}_{\alpha}^{(0)}\).
Now we analyze
For isotropic or orthotropic cases, \({x}_{\gamma}^{(2)}\) only involves \(\ddot{x}_{\alpha}^{(0)}\) and spatial derivatives of \({x}_{3}^{(1)}\) and \(S_{\alpha\beta}^{(0)}\), and thus derivatives of \({x}_{\alpha}^{(0)}\); on the other hand, \({x}_{3}^{(2)}\) only involves \(\ddot{x}_{3}^{(0)}\) and spatial derivatives of \({x}_{\gamma}^{(1)}\) (\(S_{\alpha3}^{(0)}\) becomes \(-q_{\alpha}^{-}\)), and thus derivatives of \({x}_{3}^{(0)}\). Then, we can calculate
For isotropic or orthotropic cases, \(S_{\alpha\beta}^{(1)}\) only involves \(\ddot{x}_{3}^{(0)}\) and spatial derivatives of \({x}_{\gamma}^{(1)}\), thus only derivatives of \({x}_{3}^{(0)}\); while \(S_{\alpha 3}^{(1)}\) only involves \(\ddot{x}_{\gamma}^{(0)}\) and spatial derivatives of \({S}_{\beta\gamma}^{(0)}\), thus only derivatives of \({x}_{\gamma}^{(0)}\); and \(S_{3 3}^{(1)}\) only involves \(\ddot{x}_{3}^{(0)}\).
We might also express \({x}_{i}^{(2)}\) and \(S_{m i}^{(1)}\) in terms of \({x}^{(0)}\) by combining the above recursion relations
where (changing \(\alpha\rightarrow m\), \(\beta\rightarrow k\))
with the properties
And
where (changing \(\alpha\rightarrow p\), \(\beta\rightarrow j\))
with symmetry properties
Appendix B: Recursion Relations, Stress Coefficients and Functions for Isotropic Case
The high-order coefficients of current position \(\mathbf{x}\) are
and
The subsequent coefficients of \(\mathbf{x}\) are given by (for \(i\ge1\))
The stress coefficients are given by
and
The components of \(\mathbb{S}^{(i)}\) (\(i\ge2\)) can be obtained by using (39) and the above formulas of \(\mathbf{x}^{(k)}\) together with the explicit expressions \(\mathscr{A}_{0}^{1}\) for isotropic case.
The functions \(f_{i}(\mathbf{q}^{-})\) in the isotropic linear system (62) are given by
where \(q_{\phi}^{-}\) are given in (64). And the functions in (65) are given by
The functions \(F_{i}(\mathbf{q}^{\pm})\) in the refined dynamic system (81) are given by
Appendix C: The Replacement Procedure in Sect. 6.2
The replacement procedure takes the following steps in sequence
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1.
Replace \(\ddddot{u}\) in (80)1 by utilizing (62)1, i.e., by taking twice time derivative of
$$\frac{1}{2} \bar{E} \bigl[(1-\nu) \Delta u+ (1+\nu)\phi_{X} \bigr] + \bar{q}_{1} + f_{1} =\rho \ddot{u}, $$and similarly replace \(\ddddot{v}\) in (80)2 by utilizing (62)2.
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2.
Replace \(\Delta^{2} u\) in (80)1 by also utilizing (62)1, i.e., by taking a \(\Delta\) on the equation
$$\frac{1}{2} \bar{E} \bigl[(1-\nu) \Delta u+ (1+\nu)\phi_{X} \bigr] - \bar{E} h \Delta w_{X} +\bar{q}_{1} + f_{1} =\rho \ddot{u}, $$and similarly replace \(\Delta^{2} v\) in (80)2 by utilizing (62)2.
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3.
Replace \(\Delta\phi_{X}\) and \(\Delta\phi_{Y}\) in (80)1,2 by using (65)1, i.e., by taking proper derivative of
$$\bar{E} \Delta\phi - \bar{E} h \Delta^{2} w + \bar{q}_{\phi}+ f_{\phi}=\rho \ddot{\phi}, $$and replace \(\Delta^{2} \phi\) in (80)3 by conducting a \(\Delta\) on the above equation without the term \(\rho \ddot{\phi}\).
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4.
Replace \(\Delta^{2} w_{X}\) and \(\Delta^{2} w_{Y}\) in (80)1,2 by using (66), i.e., taking proper derivative of
$$-\frac{1 }{3} \bar{E} h^{2} \Delta^{2} w + \bar{q}_{3} + f_{3} + h(\bar{q}_{\phi}+ f_{\phi})= \rho \ddot{w} + \frac{\rho\nu h}{\nu-1} \ddot{\phi}, $$and replace \(\Delta^{3} w\) in (80)3 by conducting a \(\Delta\) on the above equation without the term \(\ddot{\phi}\).
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5.
Eliminate the term \(\Delta\phi\) in the resulting (80)3 by utilizing the first two equations (like the derivation of (66)), and neglect the resulting \(\rho h^{3} \Delta\ddot{\phi }\) term on the right hand side.
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Song, Z., Dai, HH. On a Consistent Dynamic Finite-Strain Plate Theory and Its Linearization. J Elast 125, 149–183 (2016). https://doi.org/10.1007/s10659-016-9575-4
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DOI: https://doi.org/10.1007/s10659-016-9575-4