Abstract

The Symmetric Galerkin Boundary Element Method is advantageous for the linear elastic fracture and crackgrowth analysis of solid structures, because only boundary and crack-surface elements are needed. However, for engineering structures subjected to body forces such as rotational inertia and gravitational loads, additional domain integral terms in the Galerkin boundary integral equation will necessitate meshing of the interior of the domain. In this study, weakly-singular SGBEM for fracture analysis of three-dimensional structures considering rotational inertia and gravitational forces are developed. By using divergence theorem or alternatively the radial integration method, the domain integral terms caused by body forces are transformed into boundary integrals. And due to the weak singularity of the formulated boundary integral equations, a simple Gauss-Legendre quadrature with a few integral points is suffcient for numerically evaluating the SGBEM equations. Some numerical examples are presented to verify this approach and results are compared with benchmark solutions.

Highlights

  • The Symmetric Galerkin Boundary Element Method (SGBEM) [1–3] has gained increasing popularity in fracture and crack-growth analysis of solid structures due to its attractive features of symmetric coef cient matrices, weak-singularity, and that only boundary & crack-surface elements are needed

  • For the fracture mechanics problems such as turbine discs and turbine blades of aircraft engines, concrete gravity dam, etc., SGBEM may lose its advantages, because evaluation of domain integral terms resulting from body forces such as rotational inertia and gravitational loads leads to the meshing of the interior of the domain

  • This paper presents the weakly singular traction boundary integral equation for solids undergoing rotational inertia and gravitational Loads

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Summary

Introduction

The Symmetric Galerkin Boundary Element Method (SGBEM) [1–3] has gained increasing popularity in fracture and crack-growth analysis of solid structures due to its attractive features of symmetric coef cient matrices, weak-singularity, and that only boundary & crack-surface elements are needed. This paper presents the weakly singular traction boundary integral equation for solids undergoing rotational inertia and gravitational Loads. By using the divergence theorem (div) or the radial integration method (RIM), domain integrals induced by rotational inertia or gravitational forces are transformed into boundary integrals correspondingly. The developed SGBEM with only weakly-singular boundary integrals are applied to simulate various examples of 3D solids with/without considering rotational inertia and gravitational loads. Appearing in traction boundary integral Eq (2) considering rotational inertia and gravitational loads is transformed into weakly singular boundary integral, using the divergence theorem or the radial integration method. In Subsections 2.1 and 2.2, the domain integral terms with rotational inertia and gravitational loads in tBIE are transformed into weakly singular boundary integral terms by two methods of divergence theorem and radial integration method, respectively

Transformation of Domain Integrals with Gravitational Loads to Boundary Integrals
Using Divergence Theorem to Transform Domain
Using the Radial Integration Method to Transform Domain Integrals with
Transform Domain Integrals with Rotational Inertia to Boundary Integrals
Using Divergence Theorem to Transform Domain Integrals with Inertial Force
Using Radial Integration method to Transform Domain Integrals with Inertial
Weakly-Singular SGBEM with Numerical Implementation
Traction and Displacement BIEs Considering Rotational Inertia and Gravitational Loads by Divergence Theorem
Traction and
Numerical Evaluation of Weakly-Singular Double Surface Integrals Using
Numerical Test of the Effect of the Number of Integration Points
A Cube Undergoing Gravitational Loads
A Rotating Disk
Numerical Examples with Cracks
A Cuboid Hanging under Its Own Weight with a Through-Thickness Crack
A Rotating Disk with a through-Thickness Crack
A Rotating Disk with Semi-Elliptic Surface Cracks
Conclusions
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