The l.h.s integral I can be approximated by the Q - point Gauss quadrature [1,2,3,4]
1 | 1 | Q | ||||
I = | ∫ | dL1 | ∫ | dL2 |det J| f(L1, L2, L3) ∼ | ∑ | fq(L1, L2, L3)Wq |
0 | 0 | q=1 |
where Wq denotes the weights for q - points of the numerical integration, and can be found in the Table 5.3 in[1]. As it was already said, a set of Nk(L1, L2, L3) shape functions where k = 1, 2, 3 can be used to evaluate each f function in the interpolation series which, for instance, in the highest order 10 – nodal cubic triangular element has the following form
3 | 9 | ||||
f(L1, L2, L3) = | ∑ | Nk(L1, L2, L3)fk + | ∑ | Nk(L1, L2, L3)Δfk + | N10ΔΔf10 |
k=1 | k=4 |
where fk are nodal values of f function, fk denote departures from linear interpolation for mid – side nodes, and f10 is departure from both previous orders of approximation for the central nodeC[1]. For linear triangular elements only the first term is important which gives an approximation
f(L1, L2, L3) = | ∑ | Lkfk |
k=1 |
Note, that the r.h.s sum does not include the jacobian j det Jj that should be incorporated by the weights Wq but it is not (in their values given in Table 5.3 from[1]). Thus let's add the triangle area to the above – recalled formula
|det J|/(2Δ) | ∑ | fq(L1, L2, L3)Wq |
q=1 |
and in that way we end up with the final expression for the Q – point Gauss quadrature.