2010
DOI: 10.1007/s11075-010-9371-3
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Numerical integration schemes for space–time hypersingular integrals in energetic Galerkin BEM

Abstract: Here we consider exterior Neumann wave propagation problems reformulated in terms of space-time hypersingular boundary integral equations. We deal with quadrature schemes required, in the discretization phase, by the energetic Galerkin boundary element method.

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Cited by 9 publications
(6 citation statements)
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“…Further, we observe that the Heaviside function H[Δhki MathClass-bin−r] in Equation and the function (Δhk i )2 MathClass-bin− r2 in the kernel scriptSi(rMathClass-punc,thMathClass-punc,tk), give rise to other different type of troubles, which have to be properly faced, exactly as described in for the case of monodomain wave propagation problems. Hence, the numerical treatment of Equation has been done through quadrature schemes widely used in the context of Galerkin BEM coming from elliptic problems , coupled with a suitable regularization technique , after a careful subdivision of the integration domain due to the presence of the Heaviside function.…”
Section: Galerkin Boundary Element Methods Discretizationmentioning
confidence: 99%
“…Further, we observe that the Heaviside function H[Δhki MathClass-bin−r] in Equation and the function (Δhk i )2 MathClass-bin− r2 in the kernel scriptSi(rMathClass-punc,thMathClass-punc,tk), give rise to other different type of troubles, which have to be properly faced, exactly as described in for the case of monodomain wave propagation problems. Hence, the numerical treatment of Equation has been done through quadrature schemes widely used in the context of Galerkin BEM coming from elliptic problems , coupled with a suitable regularization technique , after a careful subdivision of the integration domain due to the presence of the Heaviside function.…”
Section: Galerkin Boundary Element Methods Discretizationmentioning
confidence: 99%
“…In the case of the undamped wave equation, the analysis of the space hypersingularity O(1/r 2 ) of the integrand function has been performed in detail in [20]; furthermore, the presence in the kernels of the Heaviside distribution H [c (t − τ ) − r ], which represents the wavefront, and of the square root c 2 (t − τ ) 2 − r 2 can cause numerical troubles that in [28] have been solved by suitable splitting of the outer integral over Γ and using quadrature schemes which regularize integrand functions with mild singularities. We stress the fact that all the above-recalled space singularities appear after analytical integration in time variables.…”
Section: Handling Hypersingular Kernel Space-time Integration In Matrmentioning
confidence: 99%
“…where r = r (s, z) andw i ,w j define one of the Lagrangian basis functions in local space variables over the elements e i and e j , respectively. Due to the hypersingularity O(1/r 2 ) for r → 0, the evaluation of double integrals of type (29) is troublesome when e i ≡ e j and when e i , e j are consecutive, and it has been performed similarly as in [28]. Anyway, for reader's convenience, in the following we describe the double integration over coincident elements of the boundary mesh, i.e., i = j, which is the the most difficult case since hypersingularity appears at any point of e i .…”
Section: Proposition 4 Using Piece-wise Linear Time Basis Functions mentioning
confidence: 99%
“…The boundary integral method typically requires the construction of ad hoc quadrature formulas to handle weak, strong and hyper singularities that appear in the boundary integral equations (see for example [24]). But, when applied to this context, only weak singularities arise and no particular quadrature rules have been implemented for the evaluation of integrals in the system entries and in the postprocessing.…”
Section: Remarks About Numerical Integrationmentioning
confidence: 99%