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Article: Essentially non-hourglass SPH elastic dynamics
Title | Essentially non-hourglass SPH elastic dynamics |
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Authors | |
Keywords | Elastic dynamics Hourglass modes Numerical instability Smoothed particle hydrodynamics Updated Lagrangian formulation |
Issue Date | 7-May-2024 |
Publisher | Elsevier |
Citation | Journal of Computational Physics, 2024, v. 510, p. 1-27 How to Cite? |
Abstract | More than two decades ago, the numerical instabilities of particle clustering and non-physical fractures encountered in the simulations of typical elastic dynamics problems using updated Lagrangian smoothed particle hydrodynamics (ULSPH) was identified as tensile instability. Despite continuous efforts in the past, a satisfactory resolution for the simulations of these problems has remained elusive. In this paper, the concept of hourglass modes, other than tensile instability, is first explored for the discretization of shear force, arguing that the former may actually lead to the numerical instabilities in these simulations. Based on such concept, we present an essentially non-hourglass formulation by utilizing the Laplacian operator which is widely used in fluid simulations. Together with the dual-criteria time stepping, adopted into the simulation of solids for the first time to significantly enhance computational efficiency, a comprehensive set of challenging benchmark cases is used to showcase that our method achieves accurate and stable SPH elastic dynamics. |
Persistent Identifier | http://hdl.handle.net/10722/344007 |
ISSN | 2023 Impact Factor: 3.8 2023 SCImago Journal Rankings: 1.679 |
DC Field | Value | Language |
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dc.contributor.author | Zhang, Shuaihao | - |
dc.contributor.author | Lourenço, Sérgio DN | - |
dc.contributor.author | Wu, Dong | - |
dc.contributor.author | Zhang, Chi | - |
dc.contributor.author | Hu, Xiangyu | - |
dc.date.accessioned | 2024-06-25T03:29:45Z | - |
dc.date.available | 2024-06-25T03:29:45Z | - |
dc.date.issued | 2024-05-07 | - |
dc.identifier.citation | Journal of Computational Physics, 2024, v. 510, p. 1-27 | - |
dc.identifier.issn | 0021-9991 | - |
dc.identifier.uri | http://hdl.handle.net/10722/344007 | - |
dc.description.abstract | <p>More than two decades ago, the numerical instabilities of particle clustering and non-physical fractures encountered in the simulations of typical elastic dynamics problems using updated Lagrangian smoothed particle hydrodynamics (ULSPH) was identified as tensile instability. Despite continuous efforts in the past, a satisfactory resolution for the simulations of these problems has remained elusive. In this paper, the concept of hourglass modes, other than tensile instability, is first explored for the discretization of shear force, arguing that the former may actually lead to the numerical instabilities in these simulations. Based on such concept, we present an essentially non-hourglass formulation by utilizing the Laplacian operator which is widely used in fluid simulations. Together with the dual-criteria time stepping, adopted into the simulation of solids for the first time to significantly enhance computational efficiency, a comprehensive set of challenging benchmark cases is used to showcase that our method achieves accurate and stable SPH elastic dynamics.<br></p> | - |
dc.language | eng | - |
dc.publisher | Elsevier | - |
dc.relation.ispartof | Journal of Computational Physics | - |
dc.rights | This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. | - |
dc.subject | Elastic dynamics | - |
dc.subject | Hourglass modes | - |
dc.subject | Numerical instability | - |
dc.subject | Smoothed particle hydrodynamics | - |
dc.subject | Updated Lagrangian formulation | - |
dc.title | Essentially non-hourglass SPH elastic dynamics | - |
dc.type | Article | - |
dc.description.nature | published_or_final_version | - |
dc.identifier.doi | 10.1016/j.jcp.2024.113072 | - |
dc.identifier.scopus | eid_2-s2.0-85192267514 | - |
dc.identifier.volume | 510 | - |
dc.identifier.spage | 1 | - |
dc.identifier.epage | 27 | - |
dc.identifier.eissn | 1090-2716 | - |
dc.identifier.issnl | 0021-9991 | - |