SPH (smoothed particle hydrodynamics) is a gridless Lagrangian technique which is appealing as a possible alternative to numerical techniques currently used to analyze large deformation events. Recent tests of the standard SPH method using the cubic B-spline kernel indicated the possibility of an instability in the tensile regime, even though no such difficulties were observed in compression. A von Neumann stability analysis of the SPH algorithm has been carried out which identifies the criterion for stability or instability in terms of the stress state and the second derivative of the kernel function. The analysis explains the observation that the method is unstable in tension while apparently stable in compression but shows that it is pos...
Smooth Particle Hydrodynamics with a total Lagrangian formulation are, in general, more robust than ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The accuracy and stability of the classical formulation of the smoothed particle hydrodynamics (SPH)...
Grid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more efficacio...
AbstractGrid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more e...
The paper gives an overview of developments of the SPH method. Especial attention is given to the ma...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
Smooth Particle Hydrodynamics (SPH) are,in general, more robust than finite elements for large disto...
AbstractGrid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more e...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The numerical method, SPH, was first developed to model astrophysical problems. It has since been su...
Smooth Particle Hydrodynamics with a total Lagrangian formulation are, in general, more robust than ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The accuracy and stability of the classical formulation of the smoothed particle hydrodynamics (SPH)...
Grid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more efficacio...
AbstractGrid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more e...
The paper gives an overview of developments of the SPH method. Especial attention is given to the ma...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
The paper discusses the problem of tension instability of particle-based methods such as smooth part...
Smooth Particle Hydrodynamics (SPH) are,in general, more robust than finite elements for large disto...
AbstractGrid free methods, such as SPH (Smoothed Particle Hydrodynamics), may, eventually, be more e...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The numerical method, SPH, was first developed to model astrophysical problems. It has since been su...
Smooth Particle Hydrodynamics with a total Lagrangian formulation are, in general, more robust than ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...