We compare the results for a set of hydrodynamical tests performed with the adaptive mesh refinement finite volume code, MG, and the smoothed particle hydrodynamics (SPH) code, SEREN. The test suite includes shock tube tests, with and without cooling, the non-linear thin-shell instability and the Kelvin–Helmholtz instability. The main conclusions are the following. (i) The two methods converge in the limit of high resolution and accuracy in most cases. All tests show good agreement when numerical effects (e.g. discontinuities in SPH) are properly treated. (ii) Both methods can capture adiabatic shocks and well-resolved cooling shocks perfectly well with standard prescriptions. However, they both have problems when dealing with under-resolve...
We test and improve the numerical schemes in our smoothed particle hydrodynamics (SPH) code for cosm...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We compare the results for a set of hydrodynamical tests performed with the Adaptive Mesh Refinement...
This paper investigates the hydrodynamic performances of an smoothed particle hydrodynamics (SPH) co...
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison with moving-mesh...
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison with moving-mesh...
We present a novel implementation of smoothed particle hydrodynamics that uses the spatial derivativ...
We have carried out a comparison study of hydrodynamical codes by investigating their performance in...
We have carried out a hydrodynamical code comparison study of interacting multiphase fluids. The two...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
We have carried out a comparison study of hydrodynamical codes by investigating their performance in...
We test and improve the numerical schemes in our smoothed particle hydrodynamics (SPH) code for cosm...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We compare the results for a set of hydrodynamical tests performed with the Adaptive Mesh Refinement...
This paper investigates the hydrodynamic performances of an smoothed particle hydrodynamics (SPH) co...
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison with moving-mesh...
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison with moving-mesh...
We present a novel implementation of smoothed particle hydrodynamics that uses the spatial derivativ...
We have carried out a comparison study of hydrodynamical codes by investigating their performance in...
We have carried out a hydrodynamical code comparison study of interacting multiphase fluids. The two...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
We have carried out a comparison study of hydrodynamical codes by investigating their performance in...
We test and improve the numerical schemes in our smoothed particle hydrodynamics (SPH) code for cosm...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...