This thesis is devoted to the study of multiphase jet fragmentation using Smoothed Particle Hydrodynamics (SPH). The theoretical aspects of three hydrodynamic instabilities, namely the Kelvin-Helmholtz instability (KHI), Rayleigh-Taylor instability (RTI), and Rayleigh Plateau instability (RPI) are reviewed. The linear growth rate of the combined KHI and RTI are derived by means of linear perturbation in chapter 2. The linear growth rate of the multiphase RPI is presented in chapter 7. An overview of the Smoothed Particle Hydrodynamics is given in chapter 3. A pseudo-consistent SPH scheme is presented for the simulation of multiphase flow problems. Additionally, two interface stabilisation models are presented: quasi-buoyancy model and ga...
A Smoothed Particle Hydrodynamics (SPH) solution to the Rayleigh-Taylor Instability (RTI) problem in...
The numerical method, SPH, was first developed to model astrophysical problems. It has since been su...
We present fully three-dimensional hydrodynamical and magnetohydrodynamical simulations of supersoni...
The growth of the Kelvin–Helmholtz instability generated at the interface between two ideal gases is...
We adapt the smoothed-particle hydrodynamics (SPH) technique to allow a multiphase fluid in which SP...
We focus on the use of a meshless numerical method called Smooth Particle Hydrodynamics (SPH), to so...
We introduce a Smoothed Particle Hydrodynamics (SPH) concept for the stabilization of the interface ...
La méthode Smoothed Particle Hydrodynamics (SPH) est une méthode lagrangienne, sans maillage dévelop...
In this paper, we have modeled the Kelvin-Helmholtz Instability (KHI) problem of an incompressible t...
This thesis is concerned with the development and application of Smoothed Particle Hydrodynamics (SP...
Smoothed Particle Hydrodynamics (SPH) is a particle-based method for solving Navier-Stokes and simil...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Smoothed Particle Hydrodynamics (SPH) is a relatively new meshless numerical approach which has attr...
In this paper, the Rayleigh Taylor Instability (RTI) is investigated for high density ratios and inf...
L'approche Smoothed Particle Hydrodynamics (SPH) est une méthode de calcul pour simuler des écouleme...
A Smoothed Particle Hydrodynamics (SPH) solution to the Rayleigh-Taylor Instability (RTI) problem in...
The numerical method, SPH, was first developed to model astrophysical problems. It has since been su...
We present fully three-dimensional hydrodynamical and magnetohydrodynamical simulations of supersoni...
The growth of the Kelvin–Helmholtz instability generated at the interface between two ideal gases is...
We adapt the smoothed-particle hydrodynamics (SPH) technique to allow a multiphase fluid in which SP...
We focus on the use of a meshless numerical method called Smooth Particle Hydrodynamics (SPH), to so...
We introduce a Smoothed Particle Hydrodynamics (SPH) concept for the stabilization of the interface ...
La méthode Smoothed Particle Hydrodynamics (SPH) est une méthode lagrangienne, sans maillage dévelop...
In this paper, we have modeled the Kelvin-Helmholtz Instability (KHI) problem of an incompressible t...
This thesis is concerned with the development and application of Smoothed Particle Hydrodynamics (SP...
Smoothed Particle Hydrodynamics (SPH) is a particle-based method for solving Navier-Stokes and simil...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Smoothed Particle Hydrodynamics (SPH) is a relatively new meshless numerical approach which has attr...
In this paper, the Rayleigh Taylor Instability (RTI) is investigated for high density ratios and inf...
L'approche Smoothed Particle Hydrodynamics (SPH) est une méthode de calcul pour simuler des écouleme...
A Smoothed Particle Hydrodynamics (SPH) solution to the Rayleigh-Taylor Instability (RTI) problem in...
The numerical method, SPH, was first developed to model astrophysical problems. It has since been su...
We present fully three-dimensional hydrodynamical and magnetohydrodynamical simulations of supersoni...