Abstract
This chapter presents the weak form of peridynamic (PD) equilibrium equations to impose displacement and traction boundary conditions without a fictitious material layer. It permits the direct imposition of traction and displacement boundary conditions. The nonlocal deformation gradient tensor is computed in a bond-associated (BA) domain of interaction using the PD differential operator. The weak form of PD equilibrium equation is derived for the neo-Hookean material model with slight compressibility. The results are free of oscillations and spurious zero-energy modes that are commonly observed in the PD correspondence models. The fidelity of the approach is established by comparison with those of finite element analysis. Numerical results concern the finite elastic deformation of a rubber sheet with a hole under stretch.
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Change history
30 October 2022
Extra supplementary materials were provided for chapters 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14 and 16 after the publication of the book. These were then updated in the chapters.
References
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Appendix
Appendix
Under plane strain assumptions of (∂/∂x3) = 0 and y3 = x3, the deformation gradient tensor reduces to F ∼ Fαβ with (α, β = 1, 2). For two-dimensional analysis, the isochoric part of Eq. (4.53) can be modified as
or
For a scaled right Cauchy–Green tensor aC, this equation becomes
or
Specifying n = m = 1 makes the isochoric part invariant, and the strain energy density function becomes
Finally, it can be rewritten as
where, \( {\overline{I}}_1=\frac{\mathrm{tr}\mathbf{C}}{J} \).
Thus, the first Piola–Kirchhoff stress tensor can be obtained as
or
Its derivative necessary in the evaluation of the incremental internal force vector ΔQ(k) can be written as
or
with \( \frac{\partial J}{\partial {F}_{ij}}={JF}_{ji}^{-1} \).
Under plane stress assumptions of σ13 = σ23 = σ33 = 0, the Cauchy stress tensor σ reduce to σ ∼ σαβ with (α, β = 1, 2). These conditions can be equivalently imposed on the second Piola–Kirchhoff stress tensor S as S13 = S23 = S33 = 0. The second Piola–Kirchhoff stress tensor S is related to the first Piola–Kirchhoff stress tensor as
By using the relation C−1 = F−1F−T, this expression can be simplified as
Enforcing S13Â =Â 0 and S23Â =Â 0 results in
and
Similarly, enforcing S33Â =Â 0 leads to an additional expression as
Substituting from Eq. (4.67c) into Eq. (4.68) results in the constraint condition for C33 in the form
Invoking Eq. (4.69) in Eq. (4.66) and performing algebraic manipulations result in the simplified form of S for plane stress analysis as
Finally, the first Piola–Kirchhoff stress tensor can be obtained as
For numerical implementation, trC and J are expressed as
and
where \( \mathrm{tr}\tilde{\mathbf{C}}={C}_{11}+{C}_{22} \) and \( \tilde{J}=\sqrt{C_{11}{C}_{22}-{C}_{12}^2} \).
With these expressions, Eqs. (4.71) and (4.69) can be rewritten as
and
Based on the displacement field obtained from the previous iteration within every load step, the value of \( {C}_{33}={C}_{33}^{\ast } \) is numerically determined by using the method of bisection.
Its derivative necessary in the evaluation of the incremental internal force vector ΔQ(k) can be written as
or
The derivative of C33 can be obtained from Eq. (4.75) as
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Madenci, E., Roy, P., Behera, D. (2022). Weak Form of Peridynamic Equilibrium Equations. In: Advances in Peridynamics. Springer, Cham. https://doi.org/10.1007/978-3-030-97858-7_4
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