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A mixed BEM-FEM formulation for layered soil-superstructure interaction<br />

65<br />

where p and S are, respectively, the source point where a unit force is applied and a<br />

boundary point of the surface, u i and p i are, respectively, the real displacement field<br />

*<br />

*<br />

and surface forces on the boundary S in the j-th direction, while u ij and p ij represent<br />

weighted field coefficients which indicate the response obtained in the direction j in S,<br />

of a force applied on the direction i of the point p. This identity is based on the Betti’s<br />

reciprocal theorem and weighted or fundamental solutions given by u ij<br />

* and<br />

represent particular solutions of the partial differential equations of (1) for a given<br />

boundary condition.<br />

The strategy to obtain the boundary integral equations involves transporting the<br />

p, which is inside the body, to the boundary. Thus, expression (2) can be written as<br />

follows:<br />

p ij<br />

*<br />

*<br />

*<br />

C ( P)<br />

⋅ u ( P)<br />

+ p ( P,<br />

S)<br />

⋅ u ( S)<br />

⋅ ∂Γ(<br />

S)<br />

= u ( P,<br />

S)<br />

⋅ p ( S)<br />

⋅ ∂Γ(<br />

S)<br />

(3)<br />

ij<br />

j<br />

∫<br />

Γ<br />

ij<br />

j<br />

∫<br />

Γ<br />

ij<br />

j<br />

where the integral in (3) is defined in the sense of the Cauchy principal value, PARÍS &<br />

CAÑAS (1997), and C ij are coefficients that depend on the problem’s geometry<br />

HARTMANN (1980). The fundamental solutions used herein are the known Kelvin<br />

solutions presented in LOVE (1944) for the three-dimensional case.<br />

Since the analytical solutions of expression (3) are not given in closed form,<br />

they have to be estimated numerically. Hence, the Boundary Element Method (BEM) is<br />

based on the assembly of a system of algebraic equations resulting from boundary<br />

integral equations, equation (3), written in terms of nodal parameters that are<br />

approximated to the boundary values using shape functions. Hence, the integral<br />

equations of (3) are written without considering the domain forces as:<br />

ij<br />

j<br />

NE<br />

∑<br />

∫<br />

k = 1 Γ<br />

*<br />

ij<br />

C ( P)<br />

⋅u<br />

( P)<br />

+ J ⋅ p ( P,<br />

S)<br />

⋅ Ψ(<br />

S)<br />

∂ξ<br />

( S)<br />

⋅(<br />

U ) = J ⋅ u ( P,<br />

S)<br />

⋅ Ψ(<br />

S)<br />

∂ξ<br />

( S)<br />

⋅(<br />

P<br />

i<br />

k<br />

NE<br />

∑<br />

k = 1<br />

∫<br />

Γ<br />

*<br />

ij<br />

(4)<br />

where NE, ψ, J are, respectively, the number of boundary elements, the shape<br />

function and the Jacobian transformation. In this paper, we will adopt linear shape<br />

functions of the form Ψ i ( ξ 1 , ξ 2 , ξ 3 ) = ξ i , where ξ i are homogeneous coordinates defined<br />

for the triangular element BREBBIA & DOMINGUEZ (1989).<br />

The integrals proposed in (4) cannot, however, be solved analytically for any<br />

generic surface; hence the use of numerical techniques such as those given in<br />

ALIABADI et al. (1985) and TELLES (1987) can be used. In the present paper, the<br />

integral equations are calculated numerically by using a three-dimensional triangular<br />

quadrature integral BREBBIA & DOMINGUEZ (1989).<br />

It is therefore possible to assemble the shape matrix of expression (4), which<br />

takes on the following form:<br />

[ H ] ⋅ { U}<br />

= [ G]<br />

⋅{<br />

P}<br />

(5)<br />

Cadernos de Engenharia de Estruturas, São Carlos, v.9, n. 38, p. 63-82, 2007

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