Finite point method

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The finite point method (FPM) is a meshfree method for solving partial differential equations (PDEs) on scattered distributions of points. The FPM was proposed in the mid-nineties in (Oñate, Idelsohn, Zienkiewicz & Taylor, 1996a),[1] (Oñate, Idelsohn, Zienkiewicz, Taylor & Sacco, 1996b)[2] and (Oñate & Idelsohn, 1998a)[3] with the purpose to facilitate the solution of problems involving complex geometries, free surfaces, moving boundaries and adaptive refinement. Since then, the FPM has evolved considerably, showing satisfactory accuracy and capabilities to deal with different fluid and solid mechanics problems.

Similar to other meshfree methods for PDEs, the finite point method (FPM) has its origins in techniques developed for scattered data fitting and interpolation, basically in the line of weighted least-squares methods (WLSQ). The latter can be regarded as particular forms of the moving least-squares method (MLS) proposed by Lancaster and Salkauskas.[4] WLSQ methods have been widely used in meshfree techniques because allow retaining most of the MLS, but are more efficient and simple to implement. With these goals in mind, an outstanding investigation which led to the development of the FPM began in (Oñate, Idelsohn & Zienkiewicz, 1995a)[5] and (Taylor, Zienkiewicz, Oñate & Idelsohn, 1995).[6] The technique proposed was characterized by WLSQ approximations on local clouds of points and an equations discretization procedure based on point collocation (in the line of Batina’s works, 1989,[7] 1992[8]). The first applications of the FPM focused on adaptive compressible flow problems (Fischer, Onate & Idelsohn, 1995;[9] Oñate, Idelsohn & Zienkiewicz, 1995a;[5] Oñate, Idelsohn, Zienkiewicz & Fisher, 1995b[10]). The effects on the approximation of the local clouds and weighting functions were also analyzed using linear and quadratic polynomial bases (Fischer, 1996).[11] Additional studies in the context of convection-diffusion and incompressible flow problems gave the FPM a more solid base; cf. (Oñate, Idelsohn, Zienkiewicz & Taylor, 1996a)[1] and (Oñate, Idelsohn, Zienkiewicz, Taylor & Sacco, 1996b).[2] These works and (Oñate & Idelsohn, 1998)[3] defined the basic FPM technique in use today.

Numerical approximation

FPM numerical approximation scheme

The approximation in the FPM can be summarized as follows. For each point in the analysis domain (star point), an approximated solution is locally constructed by using a subset of surrounding supporting points , which belong to the problem domain (local cloud of points ). The approximation is computed as a linear combination of the cloud unknown nodal values (or parameters) and certain metric coefficients. These are obtained by solving a WLSQ problem at the cloud level, in which the distances between the nodal parameters and the approximated solution are minimized in a LSQ sense. Once the approximation metric coefficients are known, the problem governing PDEs are sampled at each star point by using a collocation method. The continuous variables (and their derivatives) are replaced in the sampled equations by the discrete approximated forms, and the solution of the resulting system allows calculating the unknown nodal values. Hence, the approximated solution satisfying the governing equations of the problem can be obtained. It is important to note that the highly local character of the FPM makes the method suitable for implementing efficient parallel solution schemes.

The construction of the typical FPM approximation is described in (Oñate & Idelsohn, 1998).[3] An analysis of the approximation parameters can be found in (Ortega, Oñate & Idelsohn, 2007)[12] and a more comprehensive study is conducted in (Ortega, 2014).[13] Other approaches have also been proposed, see for instance (Boroomand, Tabatabaei and Oñate, 2005).[14] An extension of the FPM approximation is presented in (Boroomand, Najjar & Oñate, 2009).[15]

Applications

Current lines of investigation

References

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