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with:<br />

F.E.M. for Prestressed Saint Venant-Kirchhoff Hyperelastic Membranes 127<br />

eij = 1<br />

2 (ui,j + uj,i) (6)<br />

The difference between the Green-Lagrange strain tensor for the primary and<br />

secondary states can be carried out in a straightforward manner as:<br />

By applying the chain rule:<br />

E ∗<br />

AB − EAB = X pret<br />

i,A Xpret Xj,B eij + 1<br />

2 ui,Aui,B<br />

E ∗ AB − EAB = X pret<br />

i,A Xpret X j,B<br />

(eij + 1<br />

2 us,ius,j) = X pret<br />

i,A Xpret Xj,B E ∗relat<br />

ij<br />

where the tensor E ∗relat<br />

ij has been introduced for the sake ofconvenience and it<br />

represents a relative measure of the strain at the secondary state by taking the<br />

primary one as an adequate reference.<br />

In nonlinear problems, various stress measures can be defined. In this paper,<br />

in addition to the Cauchy or real stress tensor, two tensorial entities referred to<br />

as the second Piola-Kirchhoff and the nominal stress tensors are to be used. The<br />

latter is known as well as the transpose of the first Piola-Kirchhoff stress tensor. By<br />

considering as initial configuration the initial nominally stressed one, the Cauchy<br />

stress tensor σ ∗ ij may be related to the nominal stress tensor P ∗ PAj and the second<br />

Piola-Kirchhoff stress tensor S ∗ AB as:<br />

J ∗ σ ∗ ij = xi,AP ∗ P Aj = xi,Axj,BS ∗ AB xi,A = ∂xi<br />

∂XA<br />

The same relationship may be developed when the initial prestressed configuration<br />

is adopted to be the reference state. The super index relat is added to distinguish<br />

the new nonlinear stress tensors with respect to those shown in the above formula:<br />

J ′ σ ∗ ij = xi,sP ∗relat<br />

P sj = xi,sxj,tS ∗relat<br />

st xi,s = ∂xi<br />

∂X pret<br />

s<br />

Formulae (9) and (10) can be modified to set up expressions (11) which summarize<br />

the relationship among the nominal and second Piola-Kirchhoff stress tensors<br />

obtained in both the initial undeformed configuration ℜ0 and the primary state ℜt.<br />

P ∗relat<br />

P sj = J −1 X pret<br />

s,A Xpret<br />

t,B xj,tS ∗ AB<br />

S ∗relat<br />

st<br />

= J −1 X pret<br />

s,A Xpret<br />

t,B S∗ AB<br />

The local equilibrium equations in the secondary state may be expressed with<br />

respect to three possible descriptions: ℜ0, ℜt and ℜt∗,thesebeingaLagrangian formulation for the first two configurations and an Eulerian formulation for the final<br />

configuration. These expressions may be gathered as follows:<br />

σ ∗<br />

ji,j + ρ ∗ bi = 0 in ℜt<br />

∗<br />

∗, with f = σ ∗<br />

i<br />

jin ∗<br />

j dΓ ∗<br />

(7)<br />

(8)<br />

(9)<br />

(10)<br />

(11)<br />

(12)<br />

P ∗ P Ai,A + ρ0bi =0 in ℜ0, with f ∗ f i = P ∗ PAinAdΓ0 Γ (13)

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